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1. One-Dimensional Disordered Bosonic Systems

Author

Chiara D’Errico and Marco G. Tarallo

Subjects
Bose–Einstein condensates, cold gases in optical lattices, quantum phase transitions, disordered systems, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract

Disorder is everywhere in nature and it has a fundamental impact on the behavior of many quantum systems. The presence of a small amount of disorder, in fact, can dramatically change the coherence and transport properties of a system. Despite the growing interest in this topic, a complete understanding of the issue is still missing. An open question, for example, is the description of the interplay of disorder and interactions, which has been predicted to give rise to exotic states of matter such as quantum glasses or many-body localization. In this review, we will present an overview of experimental observations with disordered quantum gases, focused on one-dimensional bosons, and we will connect them with theoretical predictions.

Published
2021
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3. Quantum Monte Carlo study of the role of p-wave interactions in ultracold repulsive Fermi gases

Author

Gianluca Bertaina, Marco G. Tarallo, and Sebastiano Pilati

Subjects
Quantum Physics, Quantum Gases (cond-mat.quant-gas), Atomic Physics (physics.atom-ph), FOS: Physical sciences, Condensed Matter - Quantum Gases, Quantum Physics (quant-ph), Physics - Atomic Physics
Abstract

Single-component ultracold atomic Fermi gases are usually described using noninteracting many-fermion models. However, recent experiments reached a regime where $p$-wave interactions among identical fermionic atoms are important. In this paper, we employ variational and fixed-node diffusion Monte Carlo simulations to investigate the ground-state properties of single-component Fermi gases with short-range repulsive interactions. We determine the zero-temperature equation of state, and elucidate the roles played by the $p$-wave scattering volume and the $p$-wave effective range. A comparison against recently derived second-order perturbative results shows good agreement in a broad range of interaction strength. We also compute the quasiparticle effective mass, and we confirm the perturbative prediction of a linear contribution in the $p$-wave scattering volume, while we find significant deviations from the beyond-mean-field perturbative result, already for moderate interaction strengths. Finally, we determine ground-state energies for two-component unpolarized Fermi gases with both interspecies and intraspecies hard-sphere interactions, finding remarkable agreement with a recently derived fourth-order expansion that includes $p$-wave contributions., Comment: 9 pages, 4 figures. Extended data for the effective mass and changed title. Post-print version

Published
2022
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4. INRIM Sr Optical Clock: An Optically Loaded Apparatus for High-Stability Metrology

Author

Marco G. Tarallo, Davide Calonico, Filippo Levi, Matteo Barbiero, Cecilia Clivati, Federica Rullo, and Matias Risaro

Subjects
Condensed Matter::Quantum Gases, Optical lattice, Strontium, Materials science, business.industry, chemistry.chemical_element, Optical switch, Metrology, law.invention, Finesse, chemistry, law, Optical cavity, Atom optics, Optoelectronics, Physics::Atomic Physics, business, Spectroscopy
Abstract

We report on the development of a new compact strontium optical lattice clock employing a 2D-MOT as cold atomic source. The clock system reliability is currently studied using the most abundant isotope, the bosonic 88Sr. More than 105 88Sr atoms are loaded in the optical lattice at 813 nm at temperatures of few microKelvin. All the needed optical frequencies are stabilized to a zero-CTE high finesse optical resonator, and can be operated without frequency adjustments for weeks. The system shows the advantage of optical guiding and switching the atomic source to the clock spectroscopy region by demonstrating more than 17 s lifetime. First spectroscopy tests on the clock transition on 88Sr atoms has been performed by magnetic-field induced spectroscopy.

Published
2021
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5. Optically loaded Strontium lattice clock with a single multi-wavelength reference cavity

Author

Davide CALONICO, Marco G. Tarallo, Filippo Levi, and Matteo Barbiero

Subjects
Condensed Matter::Quantum Gases, Physics - Instrumentation and Detectors, Atomic Physics (physics.atom-ph), Physics::Optics, FOS: Physical sciences, Physics::Atomic Physics, Instrumentation and Detectors (physics.ins-det), Electrical and Electronic Engineering, Instrumentation, Physics - Atomic Physics
Abstract

We report on the realization of a new compact strontium optical clock using a 2-D magneto-optical-trap (2D-MOT) as cold atomic source and a multi-wavelength cavity as the frequency stabilization system. All needed optical frequencies are stabilized to a zero-thermal expansion high-finesse optical resonator and can be operated without frequency adjustments for weeks. We present the complete characterization of the apparatus. Optical control of the atomic source allows us to perform low-noise clock operation without atomic signal normalization. Long- and short-term stability tests of the clock have been performed for the 88 Sr bosonic isotope by means of interleaved clock operation. Finally, we present the first preliminary accuracy budget of the system.

Published
2021
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6. Toward a quantum-enhanced strontium optical lattice clock at INRIM

Author

Marco G. Tarallo

Subjects
Electromagnetic field, Atomic Physics (physics.atom-ph), QC1-999, Quantum measurement, chemistry.chemical_element, FOS: Physical sciences, 02 engineering and technology, 01 natural sciences, Physics - Atomic Physics, Optics, 0103 physical sciences, Enhanced sensitivity, Physics::Atomic Physics, 010306 general physics, Quantum, Physics, Strontium, Optical lattice, business.industry, 021001 nanoscience & nanotechnology, Atomic clock, chemistry, 0210 nano-technology, business, Coherence (physics)
Abstract

The new strontium atomic clock at INRIM seeks to establish a new frontier in quantum measurement by joining state-of-the-art optical lattice clocks and the quantized electromagnetic field provided by a cavity QED setup. The goal of our experiment is to apply advanced quantum techniques to state-of-the-art optical lattice clocks, demonstrating enhanced sensitivity while preserving long coherence times and the highest accuracy. In this paper we describe the current status of the experiment and the prospected sensitivity gain for the designed cavity QED setup., Comment: Proceedings of the Italian National Conference on the Physics of Matter (FisMat 2019), held in Catania, Italy, September 30-October 4, 2019, E. Puppin (Ed.). Journal version is open access

Published
2020

7. A Sideband-Enhanced Cold Atomic Source For Optical Clocks

Author

Marco G. Tarallo, Giacomo Lamporesi, Matteo Barbiero, Filippo Levi, Gabriele Ferrari, and Davide Calonico

Subjects
Brightness, Atomic Physics (physics.atom-ph), Monte Carlo method, General Physics and Astronomy, Flux, FOS: Physical sciences, atomic source, 02 engineering and technology, optical clock, 01 natural sciences, Collimated light, law.invention, Physics - Atomic Physics, Optics, law, 0103 physical sciences, strontium, Physics::Atomic Physics, 010306 general physics, Physics, Condensed Matter::Quantum Gases, Optical lattice, Sideband, business.industry, 021001 nanoscience & nanotechnology, Laser, Power (physics), Physics::Accelerator Physics, 0210 nano-technology, business
Abstract

We demonstrate the enhancement and optimization of a cold strontium atomic beam from a two-dimensional magneto-optical trap (2D MOT) transversely loaded from a collimated atomic beam by adding a side-band frequency to the cooling laser. The parameters of the cooling and sideband beams are scanned to achieve the maximum atomic beam flux and are compared with Monte Carlo simulations. We obtain a 2.3 times larger total atomic flux and a brightness increase of a factor 4 compared with a conventional, single-frequency 2D MOT for a given total power of 200 mW. We show that the sideband-enhanced 2D MOT can reach the loading-rate performances of space-demanding Zeeman-slower-based systems, while it can overcome systematic effects due to thermal-beam collisions and hot-black-body-radiation shift, making it suitable for both transportable and accurate optical lattice clocks. Finally, we numerically study possible extensions of the sideband-enhanced 2D MOT to other alkaline-earth species.

Published
2019
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8. A strontium optical lattice clock apparatus for precise frequency metrology and beyond

Author

Davide Calonico, Giacomo Lamporesi, Gabriele Ferrari, Filippo Levi, Marco G. Tarallo, and Matteo Barbiero

Subjects
Trapping, 01 natural sciences, law.invention, 010309 optics, Optics, law, Lattice (order), 0103 physical sciences, Thermal, Electronic, 2D MOT, strontium, Optical and Magnetic Materials, Physics::Atomic Physics, cavity QED, 010306 general physics, Instrumentation, Optical lattice clock, Condensed Matter::Quantum Gases, Physics, Optical lattice, business.industry, Electronic, Optical and Magnetic Materials, Laser, Metrology, Optical cavity, Atom optics, business
Abstract

We present the advancement toward the realization of a new optical clock apparatus based on ultracold strontium atoms. The atomic source employs a novel design based on two dimensional magneto optical trapping which is advantageous because of the suppression of thermal atoms in the interrogation volume, and the elimination of hot BBR in the view of the science cell. Compact frequency stabilization of cooling and trapping lasers is achieved via single PDH lock to a three-color ultrastable optical resonator. We also study different lattice topologies to operate the ultracold atomic ensemble in the high-cooperativity regime toward sub-quantum projection noise instability and millihertz-linewidth frequency stabilization by cavity QED.

Published
2017
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9. BaH molecular spectroscopy with relevance to laser cooling

Author

Geoffrey Z. Iwata, Tanya Zelevinsky, and Marco G. Tarallo

Subjects
Physics, Laser ablation, Absorption spectroscopy, Atomic Physics (physics.atom-ph), FOS: Physical sciences, 02 engineering and technology, Rotational–vibrational spectroscopy, 021001 nanoscience & nanotechnology, 01 natural sciences, 7. Clean energy, Spectral line, Physics - Atomic Physics, Thermalisation, Fragmentation (mass spectrometry), Laser cooling, 0103 physical sciences, Physics::Atomic and Molecular Clusters, Molecule, Physics::Atomic Physics, Atomic physics, 010306 general physics, 0210 nano-technology
Abstract

We describe a simple experimental apparatus for laser ablation of barium monohydride (BaH) molecules and the study of their rovibrational spectra that are relevant to direct laser cooling. We present a detailed analysis of the properties of ablation plumes that can improve the understanding of surface ablation and deposition technologies. A range of absorption spectroscopy and collisional thermalization regimes has been studied. We directly measured the Franck-Condon factor of the $\mathrm{B}^2\Sigma^+(v'=0)\leftarrow\mathrm{X}^2\Sigma^+(v"=1)$ transition. Prospects for production of a high luminosity cryogenic BaH beam are outlined. This molecule is a promising candidate for laser cooling and ultracold fragmentation, both of which are precursors to novel experiments in many-body physics and precision measurement., Comment: 11 pages, 10 figures

Published
2016
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10. A high-stability semiconductor laser system for a 88Sr-based optical lattice clock

Author

Marco G. Tarallo, Guglielmo M. Tino, Denis Sutyrin, Nicola Poli, and Marco Schioppo

Subjects
Physics, Optical lattice, Physics and Astronomy (miscellaneous), Atomic Physics (physics.atom-ph), business.industry, General Engineering, FOS: Physical sciences, Physics::Optics, General Physics and Astronomy, Laser, Noise (electronics), Physics - Atomic Physics, law.invention, Finesse, Semiconductor, law, Optical Carrier transmission rates, Optical Lattice clock, laser stabilization, Optoelectronics, Physics::Atomic Physics, Atomic physics, business, Spectroscopy, Diode
Abstract

We describe a frequency stabilized diode laser at 698 nm used for high resolution spectroscopy of the 1S0-3P0 strontium clock transition. For the laser stabilization we use state-of-the-art symmetrically suspended optical cavities optimized for very low thermal noise at room temperature. Two-stage frequency stabilization to high finesse optical cavities results in measured laser frequency noise about a factor of three above the cavity thermal noise between 2 Hz and 11 Hz. With this system, we demonstrate high resolution remote spectroscopy on the 88Sr clock transition by transferring the laser output over a phase-noise-compensated 200 m-long fiber link between two separated laboratories. Our dedicated fiber link ensures a transfer of the optical carrier with frequency stability of 7 \cdot 10^{-18} after 100 s integration time, which could enable the observation of the strontium clock transition with an atomic Q of 10^{14}. Furthermore, with an eye towards the development of transportable optical clocks, we investigate how the complete laser system (laser+optics+cavity) can be influenced by environmental disturbances in terms of both short- and long-term frequency stability., 9 pages, 9 figures, submitted to Appl. Phys. B

Published
2010
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11. Search for gravitational-wave bursts in LIGO data from the fourth science run

Author

Pamela J. Russell, Roger K. Route, K. A. Thorne, J. Betzwieser, D. Ugolini, Stefan Hild, D. B. Kozak, David Jones, C. Vorvick, F. Ya. Khalili, Atsushi J. Nishizawa, Erika D'Ambrosio, Peter R. Saulson, V. Kondrashov, Roman Schnabel, R. Abbott, R. DeSalvo, J. E. Brau, Subhasish Mitra, H. Bantilan, Nicolás Yunes, M. A. Barton, Vincenzo Matta, Benno Willke, J. Clark, Pankaj Sarin, D. Meyers, L. Ruet, S. Gossler, D.B. DeBra, P. J. Sutton, K. Y. Franzen, A. L. Stuver, T. Demma, A. M. Rogan, Giuseppe Castaldi, P. Schwinberg, I. Gholami, Albrecht Rüdiger, Alessandra Buonanno, J. A. Sidles, E. E. Doomes, Fabio Postiglione, Martin P McHugh, B. J. J. Slagmolen, C. Messenger, S. Saraf, P. J. Veitch, J. Bogenstahl, L. Ribichini, Roberto Conte, E. Maros, P. Shawhan, W. G. Anderson, E. Innerhofer, Walter Winkler, Harald Lück, P. Charlton, L. Sancho De La Jordana, I. Wilmut, S. C. McGuire, Michael E Zucker, Massimo Tinto, A. Di Credico, L. Matone, R. L. Ward, Laura Cadonati, J. S. Kissel, B. P. Abbott, C. Aulbert, Ping Koy Lam, Shantanu Desai, Kip S. Thorne, Keisuke Goda, I. A. Bilenko, V. Dergachev, David J. Ottaway, Roger Jones, V. Leonhardt, J. C. Dumas, E. Chin, K. Rawlins, M. Guenther, M. Degree, A. Moylan, J. H. Romie, A. Sibley, S. Vass, Albert Lazzarini, K. Bayer, Erik Katsavounidis, Susan M. Scott, Teviet Creighton, M. J. Lubinski, D. Jackrel, Chad Hanna, F. J. Raab, B. Bland, K. Kawabe, Marco Aurelio Diaz, S. M. Aston, W. Kells, M. R. Smith, S. Wen, D. Busby, X. Siemens, V. P. Mitrofanov, John G. Dwyer, R. Gustafson, B. Rivera, Pablo Barriga, Daniel C. Woods, Vladimir B. Braginsky, H. Vahlbruch, K. Riles, M. A. Arain, T. Etzel, M. Mageswaran, S. Giampanis, John Worden, Boris Hage, S. H. Huttner, Gregory M. Harry, M. C. Araya, M. Lei, E. Espinoza, M. Weinert, David H. Shoemaker, C. Torres, A. Rodriguez, C. Barker, Andreas Freise, Vincenzo Pierro, K. Kokeyama, P. G. Murray, Holger J. Pletsch, C. Wilkinson, C. Zhao, Alicia M. Sintes, M. Ramsunder, E. Hirose, Juri Agresti, A. Dietz, Badri Krishnan, E. Chalkey, Matthew Pitkin, M. Varvella, R. Wooley, J. Heefner, R. Grosso, Stephen Fairhurst, J. Zweizig, Antony C. Searle, R. P. Croce, D. J. Hosken, C. M. Mow-Lowry, J. G. Rollins, Yousuke Itoh, Marco G. Tarallo, I. W. Martin, B. Johnson, J. H. Hough, D. Kasprzyk, Frank Seifert, D. Hoyland, Virginio Sannibale, David E. McClelland, M. Samidi, T. Hayler, Peter Fritschel, J. Dickson, C. I. Torrie, Jan Harms, A. S. Sengupta, A. J. Weinstein, W. Wu, P. T. Beyersdorf, V. Boschi, K. C. Cannon, J. Slutsky, C. Van Den Broeck, Kris Ryan, D. Webber, J. Greenhalgh, S. Wise, I. Yakushin, Helge Müller-Ebhardt, Michele Vallisneri, S. E. Whitcomb, S. Grunewald, K. Mailand, Maurizio Longo, Krzysztof Belczynski, Douglas R. Cook, R. Mittleman, Ravi Kumar Kopparapu, Soumya D. Mohanty, Rana X. Adhikari, C. Gray, M. Ito, A. M. Cruise, Ik Siong Heng, R.L. Coldwell, Evan Goetz, Gareth Jones, Nelson Christensen, N. Zotov, P. Cochrane, Emma L. Robinson, V. Quetschke, Bangalore Suryanarayana Sathyaprakash, E. Black, Martin M. Fejer, J. R. Smith, R. Bork, G. Traylor, Kentaro Somiya, Michele Zanolin, P. Kwee, A. Grant, B. Machenschalk, C. A. Cantley, K. Mason, Eric Howell, T. Nash, Michael Landry, Sanjeev Dhurandhar, Kenji Numata, L. Zhang, J. Zhang, Vuk Mandic, Thomas Corbitt, S. Sakata, Miquel Trias, Richard O'Shaughnessy, B. Barr, P. Patel, Malik Rakhmanov, S. B. Anderson, Kenneth G. Libbrecht, C. Robinson, Benjamin William Allen, S. Ray-Majumder, Karsten Danzmann, Kirk McKenzie, S. Meshkov, L. Williams, R. L. Savage, H. Ward, Peter King, A. Heptonstall, R. Riesen, Slawomir Gras, Roland Schilling, Stefano Marano, G. Billingsley, C. N. Colacino, M. Malec, H. Rehbein, K. Watts, Oliver Burmeister, Vincenzo Galdi, Francesco Chiadini, D. M. Whitbeck, D. R. Ingram, Phil Willems, Morag M. Casey, M. Heurs, Yi Chen, N. Fotopoulos, R. Rahkola, A. Franzen, A. E. Villar, Alberto Vecchio, Graham Woan, David B. Tanner, D. M. Strom, A. C. Melissinos, V. V. Frolov, Robert L. Byer, V. Parameshwaraiah, Nergis Mavalvala, Stuart Reid, Jerome Degallaix, H. Yamamoto, John Veitch, R. J. Dupuis, Jong H. Chow, B. C. Barish, David Crooks, T. T. Fricke, Lisa M. Goggin, D. Chin, Supriyo Sinha, Stanislav Babak, Bernard F. Schutz, Li Ju, Sascha Schediwy, M. MacInnis, R. S. Amin, A. Cumming, Eugeniy E. Mikhailov, J. Hanson, Duncan A. Brown, Guido Mueller, A. M. Gretarsson, M. Sung, E. Messaritaki, G. Mendell, Sheila Rowan, A. Brooks, P. Ehrens, H. zur Mühlen, N. A. Lockerbie, B. Lantz, Carlos Cepeda, Robert J. McCarthy, J. A. Giaime, K. Wette, Timothy Evans, Karel E. Urbanek, Gianpietro Cagnoli, D. Sigg, S. W. Ballmer, R. M. S. Schofield, G. Moreno, M. Fyffe, Gabriela Gonzalez, Benjamin J. Owen, Shuichi Sato, P. Savov, James Whelan, P. Ajith, M. Pedraza, J. Myers, E. Myers, Christopher Wipf, K. V. Tokmakov, Shourov Chatterji, D. Fazi, S. J. Waldman, Suvadeep Bose, Martin Hewitson, Junwei Cao, Maria Alessandra Papa, Malcolm B. Gray, Joseph D. Romano, Jared Markowitz, Vincenzo Fiumara, Fumiko Kawazoe, Kasem Mossavi, Kent Blackburn, J. Thacker, Soma Mukherjee, Drew Keppel, Zewu Yan, R. Taylor, N. A. Robertson, G. Diederichs, Helena Armandula, Andre Thüring, Ke-Xun Sun, D. Hammer, Michael C. B. Ashley, Peter Kalmus, Carlo Ungarelli, Jason S. Pelc, I. Leonor, John K. Cannizzo, K. D. Giardina, J. W C McNabb, Jordan Camp, T. Meier, J. Dalrymple, G. Newton, B. Lee, Matthew Evans, L. Cardenas, M. V. Plissi, Hartmut Grote, S. Klimenko, D. Barker, P. E. Lindquist, Peter Aufmuth, M. Lormand, S. Roddy, B. Bhawal, J. N. Marx, A. Bullington, Rahul Biswas, Lee Samuel Finn, L. Bogue, Sean T. McWilliams, J. Garofoli, Shuhei Yoshida, B. F. Whiting, H. Overmier, L. Wallace, R. Frey, D. Sellers, Simon Chelkowski, A. G. Wiseman, D. C. Coyne, D. Hoak, Patrick Brady, T. Z. Summerscales, Hirotaka Takahashi, Gavin Davies, B. Sears, Guenakh Mitselmakher, Vicky Kalogera, A. Bunkowski, Jonathan C. Leiner, S. Márka, V. Re, Yaohui Fan, Kenneth A. Strain, A. Weidner, Innocenzo M. Pinto, Thomas Cokelaer, Rainer Weiss, R. W. P. Drever, Seiji Kawamura, Reinhard Prix, Elizabeth Harstad, W. W. Johnson, Osamu Miyakawa, David H. Reitze, B. O'Reilly, N. Rainer, David Blair, Yi Pan, Jolien D. E. Creighton, Lindy Blackburn, Chunglee Kim, V. Sandberg, D. S. Rabeling, R. A. Mercer, Jesper Munch, A. Ivanov, H. Radkins, Damien Mudge, S. P. Vyachanin, M. Brinkmann, W. Tyler, David Coward, S. Penn, LSC Collaboration, The, Castaldi, G., Galdi, V., Pierro, V., and Pinto, I. M.

Subjects
Physics, Physics and Astronomy (miscellaneous), Gravitational wave, Monte Carlo method, FOS: Physical sciences, Astrophysics, General Relativity and Quantum Cosmology (gr-qc), LIGO, General Relativity and Quantum Cosmology, Black hole, QC350, Amplitude, Binary black hole, NAUTILUS, EXPLORER, Waveform, Noise (radio), QC
Abstract

The fourth science run of the LIGO and GEO 600 gravitational-wave detectors, carried out in early 2005, collected data with significantly lower noise than previous science runs. We report on a search for short-duration gravitational-wave bursts with arbitrary waveform in the 64-1600 Hz frequency range appearing in all three LIGO interferometers. Signal consistency tests, data quality cuts, and auxiliary-channel vetoes are applied to reduce the rate of spurious triggers. No gravitational-wave signals are detected in 15.5 days of live observation time; we set a frequentist upper limit of 0.15 per day (at 90% confidence level) on the rate of bursts with large enough amplitudes to be detected reliably. The amplitude sensitivity of the search, characterized using Monte Carlo simulations, is several times better than that of previous searches. We also provide rough estimates of the distances at which representative supernova and binary black hole merger signals could be detected with 50% efficiency by this analysis., Comment: Corrected amplitude sensitivities (7% change on average); 30 pages, submitted to Classical and Quantum Gravity

Published
2007
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12. High-precision spectroscopy of ultracold molecules in an optical lattice

Author

Tanya Zelevinsky, Andrew T. Grier, Marco G. Tarallo, F. Apfelbeck, Bart H. McGuyer, Geoffrey Z. Iwata, and Mickey McDonald

Subjects
Chemical Physics (physics.chem-ph), Physics, Optical lattice, Quantum Physics, Atomic Physics (physics.atom-ph), Binding energy, FOS: Physical sciences, General Physics and Astronomy, Molecular physics, 3. Good health, Physics - Atomic Physics, Quantum state, Coherent control, Lattice (order), Physics - Chemical Physics, Ultracold neutrons, Molecule, Quantum Physics (quant-ph), Spectroscopy
Abstract

The study of ultracold molecules tightly trapped in an optical lattice can expand the frontier of precision measurement and spectroscopy, and provide a deeper insight into molecular and fundamental physics. Here we create, probe, and image microkelvin $^{88}$Sr$_2$ molecules in a lattice, and demonstrate precise measurements of molecular parameters as well as coherent control of molecular quantum states using optical fields. We discuss the sensitivity of the system to dimensional effects, a new bound-to-continuum spectroscopy technique for highly accurate binding energy measurements, and prospects for new physics with this rich experimental system., 12 pages, 4 figures

Published
2015

13. Precise study of asymptotic physics with subradiant ultracold molecules

Author

Bart H. McGuyer, Robert Moszynski, Wojciech Skomorowski, Tanya Zelevinsky, Marco G. Tarallo, Mickey McDonald, and Geoffrey Z. Iwata

Subjects
Physics, Quantum Physics, Atomic Physics (physics.atom-ph), General Physics and Astronomy, FOS: Physical sciences, Weak interaction, Quantum chemistry, Homonuclear molecule, Physics - Atomic Physics, Bond length, Excited state, Molecule, Atomic physics, Spectroscopy, Quantum Physics (quant-ph), Quantum
Abstract

Weakly bound molecules have physical properties without atomic analogues, even as the bond length approaches dissociation. In particular, the internal symmetries of homonuclear diatomic molecules result in formation of two-body superradiant and subradiant excited states. While superradiance has been demonstrated in a variety of systems, subradiance is more elusive due to the inherently weak interaction with the environment. Here we characterize the properties of deeply subradiant molecular states with intrinsic quality factors exceeding $10^{13}$ via precise optical spectroscopy with the longest molecule-light coherent interaction times to date. We find that two competing effects limit the lifetimes of the subradiant molecules, with different asymptotic behaviors. The first is radiative decay via weak magnetic-dipole and electric-quadrupole interactions. We prove that its rate increases quadratically with the bond length, confirming quantum mechanical predictions. The second is nonradiative decay through weak gyroscopic predissociation, with a rate proportional to the vibrational mode spacing and sensitive to short-range physics. This work bridges the gap between atomic and molecular metrology based on lattice-clock techniques, yielding new understanding of long-range interatomic interactions and placing ultracold molecules at the forefront of precision measurements., 12 pages, 6 figures

Published
2014

14. Test of Einstein Equivalence Principle for 0-spin and half-integer-spin atoms: Search for spin-gravity coupling effects

Author

Marco G. Tarallo, D. V. Sutyrin, X. Zhang, Tommaso Mazzoni, Nicola Poli, and Guglielmo M. Tino

Subjects
Physics, Optical lattice, Atomic Physics (physics.atom-ph), General Physics and Astronomy, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Coupling (probability), 7. Clean energy, General Relativity and Quantum Cosmology, Physics - Atomic Physics, symbols.namesake, Gravitational field, Quantum mechanics, symbols, Half-integer, Matter wave, Physics::Atomic Physics, Einstein, Equivalence principle, Spin (physics)
Abstract

We report on a conceptually new test of the equivalence principle performed by measuring the acceleration in Earth's gravity field of two isotopes of strontium atoms, namely, the bosonic $^{88}$Sr isotope which has no spin vs the fermionic $^{87}$Sr isotope which has a half-integer spin. The effect of gravity upon the two atomic species has been probed by means of a precision differential measurement of the Bloch frequency for the two atomic matter waves in a vertical optical lattice. We obtain the values $\eta = (0.2\pm 1.6)\times10^{-7}$ for the E\"otv\"os parameter and $k=(0.5\pm1.1)\times10^{-7}$ for the coupling between nuclear spin and gravity. This is the first reported experimental test of the equivalence principle for bosonic and fermionic particles and opens a new way to the search for the predicted spin-gravity coupling effects., Comment: 5 pages, 4 figures. New spin-gravtity coupling analysis on the data added to the manuscript

Published
2014
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15. Virgo: a laser interferometer to detect gravitational waves

Author

Tjeerd Ketel, Antonio Eleuteri, M. Parisi, R. Passaquieti, L. Di Fiore, B. Mours, A. Królak, M. Blom, F. Beauville, K. G. Arun, G. A. Prodi, R. DeSalvo, M. Barsuglia, Gianpietro Cagnoli, Gianluca Persichetti, V. Granata, Julien Moreau, B. Mansoux, D. Verkindt, G. Losurdo, Anna Dari, M. Doets, B. Canuel, F. Piergiovanni, G. Ballardin, T Maiani, L. Giacobone, Y. Minenkov, M. Pietka, Patrice Hello, E. Turri, X Grave, R. Morand, L. Bonelli, M. Davier, G. Pagliaroli, I. Maksimovic, J. Marque, R. L. Ward, R. Hermel, G. Hemming, A. Masserot, Marco G. Tarallo, F. Vetrano, M. A. Mazzoni, L. Journet, O Lodygensky, J. P. Zendri, F. Nocera, G. Vedovato, V. Loriette, G. Barrand, P. N. Y. David, István Rácz, D. Boget, Ludovico Carbone, P. Popolizio, C Drezen, D. Passuello, C. Palomba, V Reita, Piotr Jaranowski, J.-M. Mackowski, Antoine Heidmann, Lisa Barsotti, Riccardo Sturani, Shourov Chatterji, Sofiane Aoudia, C. Arnault, Fausto Acernese, Andreas Freise, A. Di Virgilio, A. Giazotto, F. Mul, Alessandra Toncelli, G. Parguez, L. Brocco, Claude Boccara, J-Y. Vinet, I. Ferrante, S. Hamdani, R. Sottile, F. Cleva, M. Mantovani, Samuele Cortese, C Garnier, M. Lorenzini, V. Dattilo, S. D'Antonio, T. Bouedo, F. Travasso, R. Gouaty, Michał Bejger, Alessandra Corsi, L. Giordano, Mauro Tonelli, L. A. Forte, A. Dietz, M. Alshourbagy, M. Granata, L. Derome, L. Fabbroni, E. Genin, G. Cella, R. Bilhaut, L. Taffarello, A. Grado, J. L. Beney, B Dujardin, V. Fafone, R. Del Fabbro, M. Punturo, Andrea Chincarini, G. Gemme, M. Drago, P. Amico, P. Ganau, M. Galimberti, P. La Penna, F. Raffaelli, Eric Hennes, A. Pasqualetti, M. G. Beker, S. Petit, M. Pichot, Enrico Calloni, N. Liguori, L. Salconi, O. Veziant, V. Re, Guido Russo, Mirko Prato, C. Bradaschia, M. Dehamme, G. De Carolis, P. Dominici, L Matone, L. Holloway, F. Antonucci, Saverio Avino, O. Francois, A. Chiummo, Luca Gammaitoni, A. Paoli, F. Moreau, N. Leroy, B. L. Swinkels, F. Marion, F. Ricci, B. Dulach, D. Sentenac, G. Debreczeni, B. Lagrange, P. Puppo, Maurizio Ripepe, R. Paoletti, M. Loupias, F. Fidecaro, G. M. Guidi, E. Chassande-Mottin, S. Kreckelbergh, M. E. Gáspár, B. Lieunard, V. Moscatelli, K. Yamamoto, A. Brillet, M. Del Prete, Igor Neri, N. Letendre, L. Bosi, B. Bouhou, L. Pinard, C. Girard, T. Accadia, L. Naticchioni, Salvatore Vitale, M Laval, H Voet, F. Richard, P. Astone, M. Perciballi, Tania Regimbau, S. Frasca, M. Branchesi, R. Cavalieri, H. J. Bulten, L. Massonnet, L. Palladino, R. De Rosa, V. Malvezzi, A. Colla, A. Morgia, F. Frasconi, A. Basti, J. F. J. van den Brand, R. Flaminio, S. Birindelli, Tenglin Li, Archana Pai, F. Paoletti, P. Ruggi, S. Mancini, M. Iannarelli, S. Braccini, M. Tacca, D. Babusci, J.-P. Coulon, D. Jehanno, B. Sassolas, J. C. Lacotte, A Dominjon, L. Sperandio, A. C. Clapson, G. Conforto, F. Garufi, A. Viceré, H Groenstege, Andrea Gaddi, J.-D. Fournier, L. Rolland, Fabrizio Barone, C. Buy, I. Kowalska, Marie-Anne Bizouard, M. Bebronne, J. Franc, C. Michel, N. Morgado, J. C. Le Marec, V Sannibale, J. Colas, Ettore Majorana, G. Gennaro, P. Marin, M. Yvert, A. Rocchi, C. Eder, E. Campagna, P. Roudier, Fabio Marchesoni, R. Taddei, N. Arnaud, G. Daguin, J. L. Montorio, I. Fiori, R Pignard, R. Day, V. Boschi, Luisa Bracci, Roberto Cecchi, Tristan Briant, P. Rapagnani, M. Mohan, N. Man, S. Hebri, Nelson Christensen, A Remilleux, E. Tournefier, F. Cavalier, Matthew Evans, Stefano Bigotta, Ketevan Qipiani, C. Magazzù, Silvio Pardi, O. Torre, O. Rabaste, Leopoldo Milano, C. Tremola, M. Bitossi, A. Di Lieto, A. Reboux, E. Cuoco, S. Rapisarda, T. Pradier, D. Rosińska, M. Vasúth, Salvatore Solimeno, D. Enard, Elena Cesarini, B. Lopez, J. F. Hayau, E. Coccia, F. Robinet, G. Calamai, C. N. Colacino, Joseph M. Kovalik, V. Brisson, G. Matone, C. Van Den Broeck, B. Perniola, M. Was, Ruggero Stanga, S Tissot, Maria Grazia Bernardini, Ph Heusse, D. Buskulic, Zhenyu Zhang, C. Greverie, Rosa Poggiani, R. Chiche, H. Vocca, S. Karkar, A. Gennai, P. Mugnier, Simona Mosca, M. Vavoulidis, S. Vilalte, S. Van Der Putten, Tomasz Bulik, L. Fournier, Th. S. Bauer, François Bondu, G. Giordano, M. Colombini, Francesco Cottone, F. Bellachia, G. Vajente, D. Forest, A. Belletoile, W. Del Pozzo, P. F. Cohadon, H. Heitmann, D. S. Rabeling, Rocco Romano, M. Dialinas, F. Menzinger, Iolanda Ricciardi, F. Carbognani, M. Di Paolo Emilio, A. Bozzi, D. Huet, H Fang, R. Bonnand, E Pacaud, F. Martelli, S Mitra, Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), APC - Cosmologie, Physique Corpusculaire et Cosmologie - Collège de France ( PCC ), Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Observatoire de Paris-Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Institut de Physique de Rennes ( IPR ), Université de Rennes 1 ( UR1 ), Université de Rennes ( UNIV-RENNES ) -Université de Rennes ( UNIV-RENNES ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire des matériaux avancés ( LMA ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), APC - Gravitation ( APC-Gravitation ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Max-Planck-Institut-Max-Planck-Institut, T., Accadia, F., Acernese, M., Alshourbagy, P., Amico, F., Antonucci, S., Aoudia, N., Arnaud, C., Arnault, K. G., Arun, P., Astone, S., Avino, D., Babusci, G., Ballardin, F., Barone, G., Barrand, L., Barsotti, M., Barsuglia, A., Basti, Th S., Bauer, F., Beauville, M., Bebronne, M., Bejger, M. G., Beker, F., Bellachia, A., Belletoile, J. L., Beney, M., Bernardini, S., Bigotta, R., Bilhaut, S., Birindelli, M., Bitossi, M. A., Bizouard, M., Blom, C., Boccara, D., Boget, F., Bondu, L., Bonelli, R., Bonnand, V., Boschi, L., Bosi, T., Bouedo, B., Bouhou, A., Bozzi, L., Bracci, S., Braccini, C., Bradaschia, M., Branchesi, T., Briant, A., Brillet, V., Brisson, L., Brocco, T., Bulik, H. J., Bulten, D., Buskulic, C., Buy, G., Cagnoli, G., Calamai, Calloni, Enrico, E., Campagna, B., Canuel, F., Carbognani, L., Carbone, F., Cavalier, R., Cavalieri, R., Cecchi, G., Cella, E., Cesarini, E., Chassande Mottin, S., Chatterji, R., Chiche, A., Chincarini, A., Chiummo, N., Christensen, A. C., Clapson, F., Cleva, E., Coccia, P. F., Cohadon, C. N., Colacino, J., Cola, A., Colla, M., Colombini, G., Conforto, A., Corsi, S., Cortese, F., Cottone, J. P., Coulon, E., Cuoco, S., D'Antonio, G., Daguin, A., Dari, V., Dattilo, P. Y., David, M., Davier, R., Day, G., Debreczeni, G., De Caroli, M., Dehamme, R., Del Fabbro, W., Del Pozzo, M., del Prete, L., Derome, DE ROSA, Rosario, R., Desalvo, M., Dialina, L., Di Fiore, A., Di Lieto, M., Di Paolo Emilio, A., Di Virgilio, A., Dietz, M., Doet, P., Dominici, A., Dominjon, M., Drago, C., Drezen, B., Dujardin, B., Dulach, C., Eder, A., Eleuteri, D., Enard, M., Evan, L., Fabbroni, V., Fafone, H., Fang, I., Ferrante, F., Fidecaro, I., Fiori, R., Flaminio, D., Forest, Forte, LUCA ANTONIO, J. D., Fournier, L., Fournier, J., Franc, O., Francoi, S., Frasca, F., Frasconi, A., Freise, A., Gaddi, M., Galimberti, L., Gammaitoni, P., Ganau, C., Garnier, Garufi, Fabio, M. E., Gáspár, G., Gemme, E., Genin, A., Gennai, G., Gennaro, L., Giacobone, A., Giazotto, G., Giordano, L., Giordano, C., Girard, R., Gouaty, A., Grado, M., Granata, V., Granata, X., Grave, C., Greverie, H., Groenstege, G. M., Guidi, S., Hamdani, J. F., Hayau, S., Hebri, A., Heidmann, H., Heitmann, P., Hello, G., Hemming, E., Henne, R., Hermel, P., Heusse, L., Holloway, D., Huet, M., Iannarelli, P., Jaranowski, D., Jehanno, L., Journet, S., Karkar, T., Ketel, H., Voet, J., Kovalik, I., Kowalska, S., Kreckelbergh, A., Krolak, J. C., Lacotte, B., Lagrange, P., La Penna, M., Laval, J. C., Le Marec, N., Leroy, N., Letendre, T. G. F., Li, B., Lieunard, N., Liguori, O., Lodygensky, B., Lopez, M., Lorenzini, V., Loriette, G., Losurdo, M., Loupia, J. M., Mackowski, T., Maiani, E., Majorana, C., Magazzù, I., Maksimovic, V., Malvezzi, N., Man, S., Mancini, B., Mansoux, M., Mantovani, F., Marchesoni, F., Marion, P., Marin, J., Marque, F., Martelli, A., Masserot, L., Massonnet, G., Matone, L., Matone, M., Mazzoni, F., Menzinger, C., Michel, Milano, Leopoldo, Y., Minenkov, S., Mitra, M., Mohan, J. L., Montorio, R., Morand, F., Moreau, J., Moreau, N., Morgado, A., Morgia, S., Mosca, V., Moscatelli, B., Mour, P., Mugnier, F. A., Mul, L., Naticchioni, I., Neri, F., Nocera, E., Pacaud, G., Pagliaroli, A., Pai, L., Palladino, C., Palomba, F., Paoletti, R., Paoletti, A., Paoli, S., Pardi, G., Parguez, M., Parisi, A., Pasqualetti, R., Passaquieti, D., Passuello, M., Perciballi, B., Perniola, G., Persichetti, S., Petit, M., Pichot, F., Piergiovanni, M., Pietka, R., Pignard, L., Pinard, R., Poggiani, P., Popolizio, T., Pradier, M., Prato, G. A., Prodi, M., Punturo, P., Puppo, K., Qipiani, O., Rabaste, D. S., Rabeling, I., Rácz, F., Raffaelli, P., Rapagnani, S., Rapisarda, V., Re, A., Reboux, T., Regimbau, V., Reita, A., Remilleux, F., Ricci, I., Ricciardi, F., Richard, M., Ripepe, F., Robinet, A., Rocchi, L., Rolland, R., Romano, D., Rosińska, P., Roudier, P., Ruggi, Russo, Guido, L., Salconi, V., Sannibale, B., Sassola, D., Sentenac, S., Solimeno, R., Sottile, L., Sperandio, R., Stanga, R., Sturani, B., Swinkel, M., Tacca, R., Taddei, L., Taffarello, M., Tarallo, S., Tissot, A., Toncelli, M., Tonelli, O., Torre, E., Tournefier, F., Travasso, C., Tremola, E., Turri, G., Vajente, J. F. J., van den Brand, C., Van Den Broeck, S., van der Putten, M., Vasuth, M., Vavoulidi, G., Vedovato, D., Verkindt, F., Vetrano, O., Véziant, A., Viceré, J. Y., Vinet, S., Vilalte, S., Vitale, H., Vocca, R. L., Ward, M., Wa, K., Yamamoto, M., Yvert, J. P., Zendri, Z., Zhang, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut de Physique de Rennes (IPR), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS), Laboratoire des matériaux avancés (LMA), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), (Astro)-Particles Physics, Mathematical Analysis, Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), APC - Gravitation (APC-Gravitation), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), and Max-Planck-Gesellschaft-Max-Planck-Gesellschaft

Subjects
Gravitational-wave observatory, PROTOTYPE, 01 natural sciences, SCATTERED-LIGHT NOISE, law.invention, Detection of gravitational wave, interferometers, law, Instrumentation, gravitational wave, Mathematical Physics, ComputingMilieux_MISCELLANEOUS, Physics, SEISMIC NOISE, Detector, SUPER ATTENUATOR, Settore FIS/01 - Fisica Sperimentale, [ SDU.ASTR.IM ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Interferometry, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], 1ST, SUSPENSION, Gravitational waves, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Optics, Suspensions, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, Detection theory, Gravitational Waves, Interferometric Detector, Electronics, 010306 general physics, 010308 nuclear & particles physics, business.industry, Gravitational wave, Lasers, Michelson interferometer, PERFORMANCE, Antennas, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [ PHYS.ASTR.IM ] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], business, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Sensitivity (electronics), SHOT-NOISE, SYSTEM, PENDULUM
Abstract

This paper presents a complete description of Virgo, the French-Italian gravitational wave detector. The detector, built at Cascina, near Pisa (Italy), is a very large Michelson interferometer, with 3 km-long arms. In this paper, following a presentation of the physics requirements, leading to the specifications for the construction of the detector, a detailed description of all its different elements is given. These include civil engineering infrastructures, a huge ultra-high vacuum (UHV) chamber (about 6000 cubic metres), all of the optical components, including high quality mirrors and their seismic isolating suspensions, all of the electronics required to control the interferometer and for signal detection. The expected performances of these different elements are given, leading to an overall sensitivity curve as a function of the incoming gravitational wave frequency. This description represents the detector as built and used in the first data-taking runs. Improvements in different parts have been and continue to be performed, leading to better sensitivities. These will be detailed in a forthcoming paper. © 2012 IOP Publishing Ltd and Sissa Medialab srl.

Published
2012
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16. Precision Measurement of Gravity with Cold Atoms in an Optical Lattice and Comparison with a Classical Gravimeter

Author

Nicola Poli, Guglielmo M. Tino, Marco Prevedelli, F.-Y. Wang, Andrea Alberti, Marco G. Tarallo, N. Poli, F.Y. Wang, M.G. Tarallo, A. Alberti, M. Prevedelli, and G.M. Tino

Subjects
Physics, Optical lattice, Condensed matter physics, Atomic Physics (physics.atom-ph), Gravimeter, FOS: Physical sciences, General Physics and Astronomy, Gravitational acceleration, Physics - Atomic Physics, Particle in a one-dimensional lattice, precision measurements, gravity, strontium, optical lattice, bloch oscillation, Lattice (order), Quantum system, Bloch oscillations, Physics::Atomic Physics, Atomic physics, ATOMIC INTERFEROMETRY, Gravitational redshift
Abstract

We report on a high precision measurement of gravitational acceleration using ultracold strontium atoms trapped in a vertical optical lattice. Using amplitude modulation of the lattice intensity, an uncertainty $\Delta g /g \approx 10^{-7}$ was reached by measuring at the 5$^{th}$ harmonic of the Bloch oscillation frequency. After a careful analysis of systematic effects, the value obtained with this microscopic quantum system is consistent with the one we measured with a classical absolute gravimeter at the same location. This result is of relevance for the recent interpretation of related experiments as tests of gravitational redshift and opens the way to new tests of gravity at micrometer scale., Comment: 4 pages, 4 figures

Published
2011
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17. Absolute frequency measurement of unstable lasers with optical frequency combs

Author

Nicolo' Beverini, F.-Y. Wang, D. V. Sutyrin, Marco G. Tarallo, Guglielmo M. Tino, Marco Schioppo, and Nicola Poli

Subjects
Physics, Time delay and integration, business.industry, Nonlinear optics, Physics::Optics, Gravitational acceleration, Laser, optical frequency measurements, Optical frequency Combs (OFCs), law.invention, Frequency comb, Chemical species, Optics, law, Calibration, business, Jitter
Abstract

Here we report on absolute frequency measurements of a commercial high power CW diode-pumped solid-state laser (Coherent Verdi-V5). This kind of lasers usually presents large frequency jitter (up to 50 MHz) both in the short term (1 ms time scale) and in the long term (>10 s time scale). A precise measurement of absolute frequency deviations in both temporal scales should require a set of different devices (optical cavities, optical wave-meters), each suited for measurements only at a specific integration time. Here we demonstrate how a frequency comb can be used to overcome this difficulty, allowing in a single step a full characterization of both short ( 103 s) absolute frequency jitter with a resolution better than 1 MHz. We demonstrate in this way the flexibility of optical frequency combs for absolute frequency measurements not only of ultra-stable lasers but also of relatively unstable lasers. The absolute frequency calibration of the Verdi laser that we have obtained have been used in order to improve the accuracy of the measurements of the local gravitational acceleration value with 88Sr atoms trapped in 1D vertical lattices.

Published
2011

18. Optical lattice clock on bosonic Strontium atoms

Author

Nicolo' Beverini, D. V. Sutyrin, Nicola Poli, Marco G. Tarallo, Marco Schioppo, Guglielmo M. Tino, and Christopher W. Oates

Subjects
Physics, Optical lattice, business.industry, Physics::Optics, Laser, Atomic clock, optical lattice clock, strontium, Semiconductor laser theory, law.invention, Optics, law, Optical cavity, Atom optics, business, Spectroscopy, Quantum clock
Abstract

We report on recent realization of an optical lattice clock operating on the 1S 0 -3P 0 transition in 88Sr, at LENS laboratories. The clock transition is excited with the technique of magnetic field-induced spectroscopy. New experimental techniques has also been developed in order to simplifies the clock spectroscopy in Sr atoms. The first new method helps in the first search of the clock transition without the use of extensive frequency metrology hardware and in particular optical frequency combs. This technique exploits a near coincidence in the atomic wavelengths of the 1S 0 -3P 0 clock and 1S 0 -3P 1 second stage cooling transitions in Sr, which are only 5 THz far apart. This coincidence enables the use of an optical (transfer) cavity to reference the frequency of the clock transition relative to that of the much stronger cooling transition. Secondly we reduce the complexity of the experimental setup by using only semiconductor laser sources in the apparatus. With this setup, about 104 88Sr atoms are trapped in a 1D lattice formed by 200 mW of radiation tuned near the magic wavelength at 813 nm.

Published
2009

19. An optical lattice clock based on bosonic Sr

Author

Marco G. Tarallo, Nicola Poli, Christopher W. Oates, Marco Schioppo, and Guglielmo M. Tino

Subjects
Physics, Optical lattice, strontium, optical lattice clock, business.industry, Laser, Atomic clock, law.invention, Wavelength, Optics, law, Optical cavity, Lattice (order), Atom optics, Spectroscopy, business
Abstract

We present experimental results for an optical lattice clock operating on the 1S 0 ↔ 3P 0 transition in 88Sr, which is excited with the technique of magentic field-induced spectroscopy To reduce the complexity of the setup we have developed a set of new experimental techniques that greatly simplifies the clock spectroscopy in Sr atoms. First, we developed a method for finding the clock transition that removes the need for extensive frequency metrology hardware and optical frequency combs. This technique exploits a near coincidence in the atomic wavelengths of the 1S 0 ↔ 3P 0 clock and 1S 0 ↔ 3P 1 second stage cooling transitions in Sr, which are only 5 THz far apart. This coincidence enables the use of an optical (transfer) cavity to reference the frequency of the clock transition relative to that of the much stronger coolign transition Second, all laser sources in the experimental setup are based on semiconductor technology, which greatly reduces the complexity of the apparatus. With this setup, about 104 88Sr atoms are trapped in a 1D lattice formed by 200 mW of radiation tuned near the magic wavelength at 813 nm. Preliminar uncertainty budget for our optical lattice clock is also presented, with particular attention to density dependent collisions, which led to an unexpectedly high signal contrast for long interaction times.

Published
2009

20. VIRGO COMMISSIONING PROGRESS

Author

Antonio Eleuteri, A. Spallicci, Luca Gammaitoni, P. Puppo, Julien Moreau, C. Palomba, A. Di Virgilio, D. Buskulic, M. Del Prete, F. Frasconi, S. Frasca, R. Flaminio, F. Menzinger, F. Travasso, M. Lorenzini, A. Masserot, Lisa Barsotti, F. Paoletti, P. Ruggi, P. Amico, P. La Penna, Alessandra Toncelli, F. Garufi, V. Brisson, F. Martelli, Guido Russo, F. Cavalier, Leopoldo Milano, D. Verkindt, S. Kreckelbergh, F. Vetrano, Iolanda Ricciardi, B. Mours, G. Losurdo, F. Carbognani, D. Babusci, M. Punturo, Alessandra Corsi, Francesco Cottone, L. Pinard, G. Vajente, E. Cesarini, François Bondu, V. Loriette, D. Grosjean, Saverio Avino, Fabio Marchesoni, P. Hello, R. Passaquieti, Fausto Acernese, N. Morgado, Claude Boccara, Anna Dari, Stefano Bigotta, M. Mantovani, F. Piergiovanni, M. Alshourbagy, F. Ricci, H. Heitmann, Salvatore Solimeno, M. Davier, F. Antonucci, G. Giordano, E. Campagna, G. Cella, S. Birindelli, V. Reita, N. Letendre, Fabrizio Barone, L. Giordano, S. Hebri, R. Cavalieri, M. Tonelli, E. Tournefier, R. Gouaty, J.-P. Coulon, A. Gennai, L. Bosi, J.-D. Fournier, I. Fiori, D. Passuello, S. Braccini, C. Tremola, F. Marion, N. Leroy, H. Vocca, M. A. Bizouard, Nelson Christensen, V. Dattilo, A. Brillet, A. Remillieux, R. De Rosa, F. Cleva, J. Marque, M. Laval, B. Dujardin, Enrico Calloni, Sofiane Aoudia, Marco G. Tarallo, J.-M. Mackowski, C. Moins, P. Rapagnani, M. Yvert, Christian Corda, L. Di Fiore, M. Barsuglia, Rosa Poggiani, Ettore Majorana, A.-C. Clapson, F. Nocera, S. Karkar, G. Ballardin, E. Genin, C. Bradaschia, E. Chassande-Mottin, M. A. Mazzoni, C. N. Man, F. Fidecaro, G. M. Guidi, A. Giazotto, P. Astone, F. Beauville, I. Ferrante, Ketevan Qipiani, A. Viceré, Silvio Pardi, E. Cuoco, B. Lopez, J-Y. Vinet, and A. Pasqualetti

Published
2008
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21. THE STATUS OF THE VIRGO GRAVITATIONAL WAVE DETECTOR

Author

Iolanda Ricciardi, N. Letendre, R. Cavalieri, F. Carbognani, Marco G. Tarallo, M. Lorenzini, A. Masserot, E. Tournefier, C. Tremola, J.-M. Mackowski, J.-P. Coulon, J.-D. Fournier, M. Yvert, Ettore Majorana, A.-C. Clapson, H. Vocca, L. Giordano, S. Hebri, A. Di Virgilio, F. Ricci, I. Fiori, F. Paoletti, P. Ruggi, S. Kreckelbergh, M. Tonelli, R. Gouaty, F. Frasconi, R. Flaminio, A. Spallicci, D. Grosjean, G. Cella, M. Laval, N. Morgado, Sofiane Aoudia, F. Nocera, F. Vetrano, A. Pasqualetti, M. Alshourbagy, V. Dattilo, Fausto Acernese, Fabrizio Barone, M. Mantovani, Claude Boccara, Antonio Eleuteri, C. Bradaschia, P. Astone, S. Birindelli, F. Martelli, A. Brillet, A. Gennai, C. Moins, F. Antonucci, Luca Gammaitoni, Julien Moreau, V. Brisson, Ruggero Stanga, Christian Corda, F. Travasso, A. Remillieux, V. Reita, M. Del Prete, P. Amico, P. La Penna, R. De Rosa, Francesco Cottone, S. Frasca, Anna Dari, F. Cleva, D. Verkindt, L. Brocco, Rosa Poggiani, P. Puppo, Nelson Christensen, L. Pinard, S. Karkar, G. Vajente, S. Braccini, B. Dujardin, D. Buskulic, F. Garufi, V. Loriette, Enrico Calloni, D. Passuello, F. Menzinger, G. Losurdo, R. Passaquieti, F. Cavalier, L. Di Fiore, M. A. Mazzoni, M. A. Bizouard, J. Marque, B. Perniola, A. Giazotto, E. Cesarini, I. Ferrante, François Bondu, L. Milano, F. Marion, G.V. Russo, H. Heitmann, Fabio Marchesoni, P. Hello, N. Leroy, M. Barsuglia, F. Piergiovanni, G. Giordano, Alessandra Corsi, M. Davier, C. Palomba, Saverio Avino, B. Mours, M. Punturo, G. Ballardin, C. N. Man, J. Y. Vinet, F. Fidecaro, G. M. Guidi, Lisa Barsotti, Alessandra Toncelli, Ketevan Qipiani, Silvio Pardi, E. Cuoco, B. Lopez, E. Genin, E. Chassande-Mottin, F. Beauville, A. Viceré, L. Bosi, Stefano Bigotta, Salvatore Solimeno, P. Rapagnani, E. Campagna, D. Babusci, H. Kleinert, R.T. Jantzen, R. Ruffini, Acernese, F, Amico, P, Alshourbagy, M, Antonucci, F, Aoudia, S, Avino, S, Babusci, D, Ballardin, G, Barone, F, Barsotti, L, Barsuglia, M, Beauville, F, Bigotta, S, Birindelli, S, BIZOUARD M., A, Boccara, C, Bondu, F, Bosi, L, Bradaschia, C, Braccini, S, Brillet, A, Brisson, V, Brocco, L, Buskulic, D, Calloni, Enrico, Campagna, E, Cavalier, F, Cavalieri, R, Cella, G, Cesarini, E, CHASSANDE MOTTIN, E, Christensen, N, Corda, C, Cottone, F, CLAPSON A., C, Cleva, F, COULON J., P, Cuoco, E, Dari, A, Dattilo, V, Davier, M, DEL PRETE, M, DE ROSA, Rosario, DI FIORE, L, DI VIRGILIO, A, Dujardin, B, Eleuteri, A, Enard, D, Ferrante, I, Fidecaro, F, Fiori, I, Flaminio, R, FOURNIER J., D, Francois, O, Frasca, S, Frasconi, F, Freise, A, Gammaitoni, L, Garufi, Fabio, Gennai, A, Giazotto, A, Giordano, G, Giordano, L, Gouaty, R, Grosjean, D, Guidi, G, Hebri, S, Heitmann, H, Hello, P, Karkar, S, Kreckelbergh, S, LA PENNA, P, Laval, M, Leroy, N, Letendre, N, Lorenzini, M, Loriette, V, Loupias, M, Losurdo, G, Majorana, E, MAN C., N, Mantovani, M, Marchesoni, F, Marco, T, Marion, F, Marque, J, Martelli, F, Masserot, A, Mazzoni, M, Milano, L, Moins, C, Moreau, J, Morgado, N, Mours, B, Nocera, F, Pai, A, Palomba, C, Paoletti, F, Pardi, S, Pasqualetti, A, Passaquieti, R, Passuello, D, Perniola, B, Piergiovanni, F, Pinard, L, Poggiani, R, Punturo, M, Puppo, P, Qipiani, K, Rapagnani, P, Reita, V, Remillieux, A, Ricci, F, Ricciardi, I, Ruggi, P, Russo, Guido, Solimeno, S, Spallicci, A, Stanga, R, Tonelli, M, Toncelli, A, Tournefier, E, Travasso, F, Tremola, C, Vajente, G, Verkindt, D, Vetrano, F, Vicere', A, VINET J., Y, Vocca, H, and Yvert, M.

Subjects
Physics, Gravitational-wave observatory, Einstein Telescope, Tests of general relativity, Gravitational wave, Gravity Probe A, Astronomy, Astrophysics, Equivalence principle, Shapiro delay, Gravitational redshift
Published
2008
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22. Search for gravitational waves from binary inspirals in S3 and S4 LIGO data

Author

S. Márka, Kenneth A. Strain, B. O'Reilly, Yi Pan, B. Lee, D. Hoak, J. N. Marx, M. Fyffe, M. V. Plissi, Hartmut Grote, P. E. Lindquist, B. Bhawal, R. Bork, Benno Willke, J. Clark, L. Ruet, Soumya D. Mohanty, N. Zotov, Jordan Camp, Alessandra Buonanno, Rana X. Adhikari, J. Zhang, S. H. Huttner, V. Leonhardt, David Jones, Ravi Kumar Kopparapu, J. Bogenstahl, Michael E Zucker, Nicolás Yunes, E. Innerhofer, S. Giampanis, A. Dietz, K. Mason, A. J. Weinstein, I. Gholami, W. Wu, P. T. Beyersdorf, B. Machenschalk, V. Boschi, S. Ray-Majumder, T. Meier, J. Dalrymple, G. Newton, A. M. Cruise, R.L. Coldwell, C. N. Colacino, P. J. Sutton, Chunnong Zhao, David H. Shoemaker, P. Cochrane, M. Degree, N. A. Robertson, S. Chelkowski, R. Grosso, L. Zhang, Peter R. Saulson, O. Burmeister, C. Vorvick, Yi Chen, Roman Schnabel, Vuk Mandic, R. P. Croce, J. Heefner, M. Ito, Subhasish Mitra, D. Hammer, Matthew Evans, F. Seifert, A. Grant, S. Sakata, R. L. Ward, Michael C. B. Ashley, E. Chin, Walter Winkler, Harald Lück, B. Johnson, L. Cardenas, D. Kasprzyk, F. Ya. Khalili, Atsushi J. Nishizawa, A. Weidner, D. Meyers, C. Gray, Miquel Trias, P. Schwinberg, S. C. McGuire, M. Samidi, B. Lantz, Michele Vallisneri, Ik Siong Heng, Richard O'Shaughnessy, B. Barr, A. L. Stuver, Giuseppe Castaldi, P. Patel, Malik Rakhmanov, J. Worden, L. Williams, A. Rüdiger, Emma L. Robinson, A. Ivanov, Peter Kalmus, Marco Aurelio Diaz, J. H. Romie, K. Bayer, H. Zur Mühlen, W. G. Anderson, S. Grunewald, A. M. Rogan, Carlo Ungarelli, H. Yamamoto, N. Fotopoulos, R. Rahkola, Vincenzo Matta, H. Radkins, Damien Mudge, Keisuke Goda, S. Saraf, Gavin Davies, R. Riesen, S. P. Vyachanin, F. J. Raab, P. Shawhan, Andreas Freise, Vincenzo Pierro, Stefano Marano, S. Penn, Pamela J. Russell, Roberto Conte, C. Aulbert, Erik Katsavounidis, B. P. Abbott, Roland Schilling, P. Charlton, M. Brinkmann, W. Tyler, B. Sears, Roger K. Route, Vicky Kalogera, C. A. Cantley, Matthew Pitkin, C. Messenger, M. Mageswaran, A. Bullington, Rahul Biswas, K. A. Thorne, C. Robinson, M. Lormand, L. Matone, S. Wen, D. Jackrel, John G. Dwyer, A. Di Credico, L. Bogue, Sean T. McWilliams, K. S. Ganezer, I. Yakushin, K. Watts, David Coward, Laura Cadonati, K. Kawabe, D. Ugolini, Hirotaka Takahashi, M. Varvella, R. Wooley, Benjamin William Allen, Stefan Hild, V. Parameshwaraiah, Vladimir B. Braginsky, Karsten Danzmann, W. Kells, S. Dhurandhar, L. Ribichini, H. Vahlbruch, K. Riles, E. Espinoza, R. J. Dupuis, R. Gustafson, T. Hayler, S. Vass, H. Bantilan, Yaohui Fan, N. A. Lockerbie, M. Weinert, D. Chin, Supriyo Sinha, A. Sibley, E. Myers, V. Fiumara, Kentaro Somiya, I. A. Bilenko, V. Dergachev, David J. Ottaway, Stanislav Babak, J. C. Dumas, Richard J. Abbott, A. E. Villar, A. Moylan, G. T. Jones, Teviet Creighton, Ping Koy Lam, M. A. Barton, Badri Krishnan, Slawomir Gras, T. Evans, Yousuke Itoh, Duncan A. Brown, R. Desalvo, Chad Hanna, X. Siemens, E. Chalkey, Antony C. Searle, C. M. Mow-Lowry, Erika D'Ambrosio, D. Busby, Kenji Numata, C. Wilkinson, P. Savov, H. Overmier, James Whelan, Guenakh Mitselmakher, Nergis Mavalvala, Jerome Degallaix, K. Kokeyama, John K. Cannizzo, Jonathan C. Leiner, V. Re, P. Ajith, B. C. Barish, V. Kondrashov, B. F. Whiting, D. Coyne, A. M. Gretarsson, K. Y. Franzen, D. Hoyland, J. Zweizig, F. Nocera, Rainer Weiss, D. J. Hosken, Karel E. Urbanek, C. Parameswariah, E. E. Doomes, J. G. Rollins, M. A. Arain, Gregory M. Harry, P. G. Murray, D. Cook, J. A. Sidles, Fabio Postiglione, C. Van Den Broeck, I. Wilmut, S. E. Whitcomb, S. Gossler, Sandra E. Wiley, Gabriela Gonzalez, M. Lei, J. A. Giaime, T. Regimbau, P. Kwee, J. H. Hough, Lindy Blackburn, P. Ehrens, F. Kawazoe, J. Garofoli, J. S. Kissel, M. Malec, L. Sancho De La Jordana, Shantanu Desai, Kip S. Thorne, Chunglee Kim, V. Sandberg, D. R. Ingram, Phil Willems, J. Hanson, R. W.P. Drever, D. Sellers, M. Guenther, P. J. Veitch, D. S. Rabeling, Michele Zanolin, Roger Jones, I. W. Martin, Marco G. Tarallo, D. M. Strom, David Blair, Virginio Sannibale, David E. McClelland, J. Slutsky, D. Webber, R. A. Mercer, K. D. Giardina, Patrick Brady, V. P. Mitrofanov, M. C. Araya, Lisa M. Goggin, Innocenzo M. Pinto, D. Debra, Maurizio Longo, Boris Hage, S. M. Aston, V. Quetschke, Bangalore Suryanarayana Sathyaprakash, E. Black, Martin M. Fejer, J. R. Smith, S. Klimenko, T. Nash, B. Rivera, Pablo Barriga, S. Wise, T. Demma, Thomas Cokelaer, Krzysztof Belczynski, R. Mittleman, Nelson Christensen, A. Sazonov, S. M. Scott, Seiji Kawamura, Jesper Munch, B. Bland, Reinhard Prix, Elizabeth Harstad, Daniel C. Woods, J. W C McNabb, Malcolm B. Gray, Peter Fritschel, K. C. Cannon, M. Lubinski, A. Heptonstall, S. Mukherjee, Jong H. Chow, H. Ward, K. Mailand, Osamu Miyakawa, David H. Reitze, David Crooks, L. Wallace, S. Meshkov, R. Frey, H. J. Pletsch, G. Traylor, D. Kozak, Thomas Corbitt, J. Thacker, Kenneth G. Libbrecht, Kevin M. Carter, Drew Keppel, Zewu Yan, P. J. King, I. Leonor, A. G. Wiseman, H. Rehbein, Pankaj Sarin, S. B. Anderson, Stephen Fairhurst, John Veitch, David B. Tanner, G. Mendell, Sascha Schediwy, William E. Butler, M. Sung, V. V. Frolov, M. MacInnis, Martin P McHugh, B. J. J. Slagmolen, M. Pedraza, M. H. P. M. van Putten, Maria Alessandra Papa, Carlos Cepeda, Kent Blackburn, Shuichi Sato, D. Barker, K. Rawlins, M. Hewitson, T. Etzel, S. Roddy, Joseph D. Romano, Jared Markowitz, Kasem Mossavi, A. M. Sintes, P. Aufmuth, Lee Samuel Finn, Kirk McKenzie, C. Torres, A. Rodriguez, C. Barker, Kevin M. Ryan, Morag M. Casey, M. Heurs, J. Betzwieser, Francesco Chiadini, A. Franzen, A. Thüring, A. C. Melissinos, J. E. Brau, T. Z. Summerscales, R. Taylor, A. Brooks, G. Diederichs, K. Wette, Helena Armandula, D. Sigg, W. W. Johnson, N. Rainer, S. W. Ballmer, E. Hirose, Juri Agresti, H. Müller-Ebhardt, Eric Howell, Michael Landry, R. McCarthy, G. Billingsley, J. D. E. Creighton, R. Amin, R. M. S. Schofield, Benjamin J. Owen, Christopher Wipf, K. V. Tokmakov, Junwei Cao, Sanichiro Yoshida, Graham Woan, Robert L. Byer, E. Maros, Stuart Reid, Ke Sun, Bernard F. Schutz, Li Ju, Guido Mueller, A. Cumming, E. Messaritaki, Sheila Rowan, J. Dickson, C. I. Torrie, Jan Harms, A. S. Sengupta, J. Greenhalgh, G. Moreno, Evan Goetz, Vincenzo Galdi, R. L. Savage, D. M. Whitbeck, T. T. Fricke, Eugeniy E. Mikhailov, A. Bunkowski, M. R. Smith, G. H. Sanders, Alberto Vecchio, A. Lazzarini, Gianpietro Cagnoli, J. Myers, Shourov Chatterji, D. Fazi, S. J. Waldman, Suvadeep Bose, and The LIGO Scientific Collaboration

Subjects
Nuclear and High Energy Physics, Population, FOS: Physical sciences, Primordial black hole, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, General Relativity and Quantum Cosmology (gr-qc), General Relativity and Quantum Cosmology, laser-interferometer, QC350, Binary black hole, Binary star, Astrophysics::Solar and Stellar Astrophysics, ddc:530, education, QC, QB, Physics, LASER-INTERFEROMETER, education.field_of_study, Gravitational wave, Astronomy, sensitivity, LIGO, Black hole, radiation, Neutron star, RADIATION, Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik, Astrophysics::Earth and Planetary Astrophysics, SENSITIVITY
Abstract

We report on a search for gravitational waves from the coalescence of compact binaries during the third and fourth LIGO science runs. The search focused on gravitational waves generated during the inspiral phase of the binary evolution. In our analysis, we considered three categories of compact binary systems, ordered by mass: (i) primordial black hole binaries with masses in the range 0.35 M(sun) < m1, m2 < 1.0 M(sun), (ii) binary neutron stars with masses in the range 1.0 M(sun) < m1, m2 < 3.0 M(sun), and (iii) binary black holes with masses in the range 3.0 M(sun)< m1, m2 < m_(max) with the additional constraint m1+ m2 < m_(max), where m_(max) was set to 40.0 M(sun) and 80.0 M(sun) in the third and fourth science runs, respectively. Although the detectors could probe to distances as far as tens of Mpc, no gravitational-wave signals were identified in the 1364 hours of data we analyzed. Assuming a binary population with a Gaussian distribution around 0.75-0.75 M(sun), 1.4-1.4 M(sun), and 5.0-5.0 M(sun), we derived 90%-confidence upper limit rates of 4.9 yr^(-1) L10^(-1) for primordial black hole binaries, 1.2 yr^(-1) L10^(-1) for binary neutron stars, and 0.5 yr^(-1) L10^(-1) for stellar mass binary black holes, where L10 is 10^(10) times the blue light luminosity of the Sun., 12 pages, 11 figures

Published
2008

23. All-sky search for periodic gravitational waves in LIGO S4 data

Author

D. Hammer, F. Seifert, Michael C. B. Ashley, Peter Kalmus, Carlo Ungarelli, I. Leonor, H. Rehbein, K. D. Giardina, S. B. Anderson, David B. Tanner, E. Hirose, M. Sung, Juri Agresti, J. W C McNabb, M. Pedraza, Maria Alessandra Papa, Kent Blackburn, Benno Willke, J. Clark, H. Müller-Ebhardt, H. Ward, A. L. Stuver, Eric Howell, Michael Landry, E. Chalkley, L. Ruet, Alessandra Buonanno, G. Billingsley, John Veitch, Sanichiro Yoshida, Graham Woan, Rana X. Adhikari, Sascha Schediwy, B. Machenschalk, Soumya D. Mohanty, Robert L. Byer, Stuart Reid, P. Shawhan, K. Rawlins, P. Charlton, Ke Sun, Bernard F. Schutz, M. MacInnis, R. S. Amin, Andreas Freise, Vincenzo Pierro, A. Di Credico, N. Zotov, E. Innerhofer, S. Giampanis, Matthew Pitkin, K. Mason, M. Varvella, R. Wooley, Sanjeev Dhurandhar, S. Ray-Majumder, Li Ju, I. A. Bilenko, J. Hanson, V. Dergachev, Guido Mueller, David J. Ottaway, T. Hayler, C. N. Colacino, Vincenzo Galdi, Yi Chen, B. Lantz, R. P. Croce, R. L. Ward, M. Degree, J. H. Romie, K. Bayer, F. J. Raab, R. M. S. Schofield, Benjamin J. Owen, Badri Krishnan, Antony C. Searle, R. Gustafson, C. Torres, A. Rodriguez, C. Barker, I. Wilmut, F. Kawazoe, J. Garofoli, Christopher Wipf, C. M. Mow-Lowry, J. Cannizzo, A. Bunkowski, D. Hoyland, Pankaj Sarin, J. S. Kissel, David Jones, C. A. Cantley, K. V. Tokmakov, Martin Hewitson, Junwei Cao, C. Robinson, Benjamin William Allen, Karsten Danzmann, J. Zweizig, Roger Jones, C. Van Den Broeck, J. Bogenstahl, Michael E Zucker, Stefano Marano, Seiji Kawamura, Reinhard Prix, Elizabeth Harstad, Peter R. Saulson, K. Kawabe, S. M. Aston, Slawomir Gras, B. Rivera, Pablo Barriga, S. H. Huttner, M. Mageswaran, Jong H. Chow, David Crooks, Osamu Miyakawa, David H. Reitze, Erika D'Ambrosio, J. Dickson, C. I. Torrie, Jan Harms, A. S. Sengupta, V. V. Frolov, Martin P McHugh, V. Parameshwaraiah, A. Dietz, B. J. J. Slagmolen, J. E. Brau, P. G. Murray, E. Chin, J. Greenhalgh, J. H. Hough, M. A. Arain, Evan Goetz, S. Sakata, Miquel Trias, Gregory M. Harry, D. Chin, Supriyo Sinha, Stanislav Babak, E. Maros, R. Taylor, M. Lei, Duncan A. Brown, Douglas R. Cook, B. F. Whiting, Shantanu Desai, R. L. McCarthy, Kip S. Thorne, Marco Aurelio Diaz, G. Diederichs, Michele Zanolin, Richard O'Shaughnessy, B. Barr, P. Patel, Malik Rakhmanov, P. Kwee, V. Kalogera, H. Overmier, N. Fotopoulos, S. Meshkov, A. Cumming, R. Rahkola, J. Worden, L. Williams, A. Rüdiger, D. Sellers, V. P. Mitrofanov, I. W. Martin, Helena Armandula, G. Mendell, M. C. Araya, M. Guenther, Virginio Sannibale, David E. McClelland, Kirk McKenzie, B. Lee, N. Rainer, D. Hoak, R. Riesen, Boris Hage, A. M. Gretarsson, Karel E. Urbanek, Morag M. Casey, M. Heurs, Roland Schilling, Patrick Brady, M. V. Plissi, M. Fyffe, Gabriela Gonzalez, Sheila Rowan, M. Ito, F. Ya. Khalili, Atsushi J. Nishizawa, Kevin M. Ryan, A. Thüring, K. Mailand, Malcolm B. Gray, Gavin Davies, Hartmut Grote, A. C. Melissinos, B. Sears, Gianpietro Cagnoli, Maurizio Longo, T. Z. Summerscales, T. Etzel, J. Betzwieser, Richard J. Abbott, Krzysztof Belczynski, P. E. Lindquist, R. Mittleman, Francesco Chiadini, A. Franzen, A. M. Rogan, A. Brooks, Marco G. Tarallo, P. Ehrens, J. N. Marx, R. J. Dupuis, J. Slutsky, Yaohui Fan, Nelson Christensen, D. Webber, B. Bland, Carlos Cepeda, J. Thacker, Soma Mukherjee, Drew Keppel, J. C. Dumas, V. Quetschke, Bangalore Suryanarayana Sathyaprakash, E. Black, Martin M. Fejer, J. R. Smith, B. Bhawal, S. Saraf, Roberto Conte, C. Aulbert, L. Matone, Zewu Yan, T. Nash, K. Wette, Timothy Evans, Albert Lazzarini, Shuichi Sato, J. Myers, D. Sigg, Shourov Chatterji, H. Yamamoto, Joseph D. Romano, Jared Markowitz, R. Bork, L. Wallace, Kasem Mossavi, S. W. Ballmer, A. Sibley, G. Moreno, K. Kokeyama, R. Frey, D. Fazi, S. J. Waldman, Suvadeep Bose, N. A. Lockerbie, P. J. King, D. J. Hosken, A. G. Wiseman, J. G. Rollins, Jolien D. E. Creighton, Chonghoon Kim, Lindy Blackburn, D. C. Coyne, P. Savov, James Whelan, P. Ajith, L. Zhang, V. Sandberg, D. S. Rabeling, M. R. Smith, Hirotaka Takahashi, S. Márka, Ravi Kumar Kopparapu, R. A. Mercer, Guenakh Mitselmakher, Stephen Fairhurst, Kenneth A. Strain, Vincenzo Matta, A. M. Cruise, Jesper Munch, B. O'Reilly, Innocenzo M. Pinto, Vuk Mandic, D. M. Strom, C. Messenger, A. Ivanov, H. Radkins, Damien Mudge, S. P. Vyachanin, M. Brinkmann, W. Tyler, J. A. Giaime, David Coward, Thomas Cokelaer, D. Barker, S. Roddy, I. Yakushin, S. E. Whitcomb, S. Gossler, A. M. Sintes, Alberto Vecchio, P. Aufmuth, Lee Samuel Finn, Ping Koy Lam, V. Leonhardt, A. J. Weinstein, I. Gholami, W. Wu, P. T. Beyersdorf, V. Boschi, R.L. Coldwell, Giuseppe Castaldi, A. Grant, S. Chelkowski, D. B. Kozak, C. Vorvick, Roman Schnabel, A. Weidner, D. Meyers, P. Schwinberg, K. Watts, H. Zur Mühlen, W. G. Anderson, B. P. Abbott, S. Vass, Jian Zhang, W. Kells, D. Busby, Y. Pan, Subhasish Mitra, A. E. Villar, S. Wen, S. Wise, S. Grunewald, Kenneth G. Libbrecht, R. L. Savage, D. M. Whitbeck, Keisuke Goda, T. T. Fricke, Eugeniy E. Mikhailov, Nergis Mavalvala, Jerome Degallaix, Erik Katsavounidis, Laura Cadonati, B. C. Barish, V. Kondrashov, A. Moylan, Susan M. Scott, Teviet Creighton, Chunnong Zhao, Chad Hanna, M. J. Lubinski, R. DeSalvo, X. Siemens, C. Wilkinson, D. Jackrel, John G. Dwyer, E. E. Doomes, David H. Shoemaker, P. Cochrane, M. Ramsunder, Vladimir B. Braginsky, H. Vahlbruch, T. Demma, L. Sancho De La Jordana, K. Riles, Peter Fritschel, K. C. Cannon, E. Espinoza, M. Weinert, H. J. Pletsch, G. Traylor, Thomas Corbitt, O. Burmeister, A. Heptonstall, M. Malec, D. R. Ingram, Phil Willems, Daniel C. Woods, Yousuke Itoh, J. Heefner, R. Grosso, D. Ugolini, Lisa M. Goggin, M. Lormand, A. Bullington, Rahul Biswas, B. Johnson, D. Kasprzyk, L. Bogue, Sean T. McWilliams, Michele Vallisneri, Ik Siong Heng, Emma L. Robinson, M. Samidi, L. Ribichini, C. Gray, E. Myers, V. Fiumara, Jonathan C. Leiner, V. Re, Kentaro Somiya, Kenji Numata, Rainer Weiss, R. W. P. Drever, W. W. Johnson, David Blair, Jordan Camp, H. Bantilan, M. A. Barton, Walter Winkler, T. Meier, J. Dalrymple, D.B. DeBra, K. Y. Franzen, G. Newton, Fabio Postiglione, Harald Lück, S. C. McGuire, P. J. Veitch, Matthew Evans, L. Cardenas, S. Klimenko, Nicolás Yunes, P. J. Sutton, S. Penn, Pamela J. Russell, Roger K. Route, K. A. Thorne, Stefan Hild, G. T. Jones, N. A. Robertson, LSC Collaboration, The, Castaldi, G., Galdi, V., Pierro, V., and Pinto, I. M.

Subjects
Nuclear and High Energy Physics, Population, FOS: Physical sciences, Astrophysics, General Relativity and Quantum Cosmology (gr-qc), 01 natural sciences, Noise (electronics), General Relativity and Quantum Cosmology, Particle detector, QC350, Signal-to-noise ratio, 0103 physical sciences, ddc:530, 010306 general physics, education, QC, QB, Physics, education.field_of_study, 010308 nuclear & particles physics, Gravitational wave, Astrophysics (astro-ph), LIGO, Computational physics, Neutron star, StackSlide, Amplitude, Graviational waves, LIGO S4, PowerFlux, Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik, Hough
Abstract

We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50-1000 Hz and with the frequency's time derivative in the range -1.0E-8 Hz/s to zero. Data from the fourth LIGO science run (S4) have been used in this search. Three different semi-coherent methods of transforming and summing strain power from Short Fourier Transforms (SFTs) of the calibrated data have been used. The first, known as "StackSlide", averages normalized power from each SFT. A "weighted Hough" scheme is also developed and used, and which also allows for a multi-interferometer search. The third method, known as "PowerFlux", is a variant of the StackSlide method in which the power is weighted before summing. In both the weighted Hough and PowerFlux methods, the weights are chosen according to the noise and detector antenna-pattern to maximize the signal-to-noise ratio. The respective advantages and disadvantages of these methods are discussed. Observing no evidence of periodic gravitational radiation, we report upper limits; we interpret these as limits on this radiation from isolated rotating neutron stars. The best population-based upper limit with 95% confidence on the gravitational-wave strain amplitude, found for simulated sources distributed isotropically across the sky and with isotropically distributed spin-axes, is 4.28E-24 (near 140 Hz). Strict upper limits are also obtained for small patches on the sky for best-case and worst-case inclinations of the spin axes., Comment: 39 pages, 41 figures An error was found in the computation of the C parameter defined in equation 44 which led to its overestimate by 2^(1/4). The correct values for the multi-interferometer, H1 and L1 analyses are 9.2, 9.7, and 9.3, respectively. Figure 32 has been updated accordingly. None of the upper limits presented in the paper were affected

Published
2008

24. VIRGO: a large interferometer for gravitational wave detection started its first scientific run

Author

F. Garufi, A. Giazotto, Rocco Romano, I. Ferrante, F. Nocera, C. Tremola, F. Vetrano, D. Passuello, A. Di Lieto, Leopoldo Milano, H. Vocca, G. Pagliaroli, D. Buskulic, T. Regimbau, F. Menzinger, Francesco Cottone, Rosa Poggiani, L. Pinard, V. Dattilo, Frédérique Marion, B. Mours, E. Coccia, S. Kreckelbergh, Silvio Pardi, A. Brillet, E. Cuoco, E. Campagna, Th S. Bauer, Anna Dari, S. Van Der Putten, Guido Russo, V. Fafone, F. Martelli, C. Greverie, A. Remillieux, R. De Rosa, R. Cavalieri, F. Cleva, V. Granata, G. Vajente, Marie-Anne Bizouard, Christian Corda, Matthew Evans, N. Morgado, B. Lopez, D. Grosjean, S. Birindelli, L. Giordano, S. Hamdani, F. Frasconi, A. C. Clapson, A. Masserot, C. Palomba, Iolanda Ricciardi, A. Di Virgilio, M. Yvert, R. Terenzi, R. Flaminio, G. Cella, A. Rocchi, H. Heitmann, Stefano Bigotta, P. Puppo, Julien Moreau, M. Alshourbagy, L. Baggio, J.-P. Coulon, Enrico Calloni, Salvatore Solimeno, Sabrina D'Antonio, Sofiane Aoudia, A. Gennai, L. Di Fiore, Marco G. Tarallo, Lisa Barsotti, F. Travasso, F. Ricci, B. Dujardin, Alessandra Toncelli, D. Huet, C. Bradaschia, Y. Minenkov, M. Laval, Alessandro D. A. M. Spallicci, M. Lorenzini, P. Amico, M. Barsuglia, S. Braccini, P. La Penna, E. Genin, N. Leroy, P. Astone, Igor Neri, J.-D. Fournier, Simona Mosca, R. Passaquieti, N. Letendre, V. Brisson, L. Bosi, I. Fiori, E. Tournefier, F. Antonucci, C. N. Man, F. Piergiovanni, Alessandra Corsi, J. F. J. van der Brand, M. Punturo, M. Davier, E. C-Mottin, J.-M. Mackowski, P. Rapagnani, D. Verkindt, A. Viceré, Saverio Avino, F. Cavalier, J. Marque, Claude Boccara, Mauro Tonelli, F. Fidecaro, G. M. Guidi, C. Moins, G. Losurdo, G. Cagnoli, L. Rolland, Fabrizio Barone, S. Hebri, E. Cesarini, Fausto Acernese, M. Mantovani, Fabio Marchesoni, François Bondu, F. Paoletti, P. Ruggi, V. Loriette, Luca Gammaitoni, M. Del Prete, S. Frasca, Ettore Majorana, A. Pasqualetti, Patrice Hello, J-Y. Vinet, F., Acernese, M., Alshourbagy, P., Amico, F., Antonucci, S., Aoudia, P., Astone, S., Avino, L., Baggio, F., Barone, L., Barsotti, M., Barsuglia, T. S., Bauer, S., Bigotta, S., Birindelli, M., Bizouard, C., Boccara, F., Bondu, L., Bosi, S., Braccini, C., Bradaschia, A., Brillet, V., Brisson, D., Buskulic, G., Cagnoli, Calloni, Enrico, E., Campagna, F., Cavalier, R., Cavalieri, G., Cella, E., Cesarini, E. C., Mottin, A. C., Clapson, F., Cleva, E., Coccia, C., Corda, A., Corsi, F., Cottone, J. P., Coulon, E., Cuoco, S., D'Antonio, A., Dari, V., Dattilo, M., Davier, DE ROSA, Rosario, M., Del Prete, L., Di Fiore, A., Di Lieto, A., Di Virgilio, B., Dujardin, M., Evan, V., Fafone, I., Ferrante, F., Fidecaro, I., Fiori, R., Flaminio, J. D., Fournier, S., Frasca, F., Frasconi, L., Gammaitoni, Garufi, Fabio, E., Genin, A., Gennai, A., Giazotto, L., Giordano, V., Granata, C., Greverie, D., Grosjean, G., Guidi, S., Hamdani, S., Hebri, H., Heitmann, P., Hello, D., Huet, S., Kreckelbergh, P., La Penna, M., Laval, N., Leroy, N., Letendre, B., Lopez, M., Lorenzini, V., Loriette, G., Losurdo, J. M., Mackowski, E., Majorana, M., Mantovani, F., Marchesoni, F., Marion, J., Marque, F., Martelli, A., Masserot, F., Menzinger, Milano, Leopoldo, Y., Minenkov, C., Moin, J., Moreau, N., Morgado, S., Mosca, B., Mour, C. N., Man, I., Neri, F., Nocera, G., Pagliaroli, C., Palomba, F., Paoletti, S., Pardi, A., Pasqualetti, R., Passaquieti, D., Passuello, F., Piergiovanni, L., Pinard, R., Poggiani, M., Punturo, P., Puppo, P., Rapagnani, T., Regimbau, A., Remillieux, F., Ricci, I., Ricciardi, A., Rocchi, L., Rolland, R., Romano, P., Ruggi, Russo, Guido, Solimeno, Salvatore, A., Spallicci, M., Tarallo, R., Terenzi, A., Toncelli, M., Tonelli, E., Tournefier, F., Travasso, C., Tremola, G., Vajente, J. F. J., van der Brand, S., van der Putten, D., Verkindt, F., Vetrano, A., Vicerè, J. Y., Vinet, H., Vocca, M., Yvert, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), APC - Gravitation (APC-Gravitation), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Laboratoire des matériaux avancés (LMA), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Virgo, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), VIRGO, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ESPCI ParisTech, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), and Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)

Subjects
Physics, History, Gravitational-wave observatory, 010308 nuclear & particles physics, Gravitational wave, Detector, Settore FIS/01 - Fisica Sperimentale, Astronomy, Virgo interferometer, 01 natural sciences, Particle detector, LIGO, Computer Science Applications, Education, Interferometry, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, Astronomical interferometer, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics
Abstract

International audience; The VIRGO interferometer is the largest ground based European gravitational wave detector operating at the EGO Laboratory in the Pisa, Italy; countryside. During the last commissioning period relevant progress have been done in approaching its design sensitivity all over the detection bandwidth. Thanks to the effort of the whole Collaboration a long scientific run has been done collecting data for more than 4 months in conjunction with the LIGO detectors. The results obtained from the detector point of view are: a very good stability and a duty-cycle as high as 81% in science mode. In this paper we present the status of the VIRGO interferometer giving an overview of the experimental apparatus together with its most relevant features.

Published
2008
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25. Searches for periodic gravitational waves from unknown isolated sources and Scorpius X-1: Results from the second LIGO science run

Author

T. Demma, H. Ward, Rana X. Adhikari, Peter Fritschel, B. F. Whiting, L. Wallace, B. Machenschalk, J. Zhang, J. S. Kissell, S. Chelkowski, D. B. Kozak, A. Weidner, S. Nagano, D. M. Whitbeck, K. C. Cannon, D. Meyers, P. Schwinberg, D. Sigg, G. Moreno, T. T. Fricke, Eugeniy E. Mikhailov, H. Zur Mühlen, W. G. Anderson, D. Barker, John Veitch, B. P. Abbott, J. Betzwieser, Sascha Schediwy, M. Coles, M. Guenther, S. Mukherjee, S. Roddy, H. J. Pletsch, Thomas Corbitt, M. MacInnis, Francesco Chiadini, A. Franzen, D. Busby, M. A. Arain, Gerhard Heinzel, Benno Willke, J. Clark, J. Logan, L. Ruet, Akiteru Takamori, A. M. Rogan, G. Mitselmakher, R. S. Amin, Andreas Freise, N. Fotopoulos, R. Rahkola, Gregory M. Harry, M. C. Díaz, A. Libson, Matthew Pitkin, Malcolm B. Gray, Patrick Brady, M. R. Smith, R. Taylor, J. G. Rollins, G. Mendell, M. Varvella, R. Wooley, V. Sannibale, P. Aufmuth, Lee Samuel Finn, S. Sakata, S. Wise, Erika D'Ambrosio, Jong H. Chow, David Crooks, M. Lei, B. O'Reilly, Seiji Kawamura, Reinhard Prix, Elizabeth Harstad, D. R. Ingram, S. Reid, Alberto Vecchio, Kenneth G. Libbrecht, Miquel Trias, Pankaj Sarin, T. Hayler, T. Regimbau, G. Traylor, Kevin M. Carter, Alessandra Buonanno, K. A. Thorne, Stefano Marano, R. Gustafson, S. M. Aston, K. Bayer, Jesper Munch, Vincenzo Fiumara, P. Shawhan, Roman Schnabel, Osamu Miyakawa, David H. Reitze, M. Fyffe, Badri Krishnan, K. Watts, H. Rehbein, Richard O'Shaughnessy, B. Barr, P. Patel, Malik Rakhmanov, E. Chalkey, D. J. Hosken, D. S. Rabeling, S. B. Anderson, B. Lee, J. Worden, M. Zanolin, R. J. Dupuis, Christian J. Killow, I. Yakushin, Hirotaka Takahashi, Antony C. Searle, C. M. Mow-Lowry, E. Innerhofer, S. Giampanis, Phil Willems, A. E. Villar, David B. Tanner, L. Williams, A. Rüdiger, N. E. Strand, S. Vass, J. H. Romie, A. Bullington, Rahul Biswas, C. I. Torrie, J. Thacker, D. Hoak, Subhasish Mitra, Ravi Kumar Kopparapu, A. M. Sintes, William E. Butler, Drew Keppel, L. Bogue, Sean T. McWilliams, T. Evans, P. Csatorday, S. Penn, David Jones, Nergis Mavalvala, M. Sung, S. Dhurandhar, V. Parameshwaraiah, M. Brinkmann, Jerome Degallaix, Linqing Wen, D. M. Strom, B. Blair, A. F. Brooks, A. J. Weinstein, Zewu Yan, A. M. Cruise, B. C. Barish, M. Weinert, Shantanu Desai, D. Hoyland, W. W. Johnson, Kip S. Thorne, K. D. Zaleski, G. S. Davies, R. DeSalvo, I. W. Martin, Shuichi Sato, M. Degree, R. Riesen, E. Goetz, H. Yamamoto, Jordan Camp, V. Kondrashov, Maria Alessandra Papa, E. Maros, Martin P McHugh, Harald Lück, M. V. Plissi, David E. McClelland, E. E. Doomes, R. A. Mercer, B. Sears, B. J. J. Slagmolen, M. H. P. M. van Putten, C. Van Den Broeck, D. Chin, Supriyo Sinha, Stanislav Babak, B. Lantz, F. J. Raab, T. Meier, J. Dalrymple, Kent Blackburn, Lisa M. Goggin, L. Sancho De La Jordana, G. Newton, Vuk Mandic, Vicky Kalogera, J. Zweizig, Peter R. Saulson, Duncan A. Brown, I. Leonor, John K. Cannizzo, V. P. Mitrofanov, J. Bogenstahl, Hartmut Grote, Joseph D. Romano, Jared Markowitz, Michael E Zucker, D. Cook, C. Vorvick, Laura Cadonati, Innocenzo M. Pinto, E. L. Robison, Yaohui Fan, H. Ding, Thomas Cokelaer, I. Wilmut, F. Kawazoe, M. C. Araya, J. Garofoli, S. Márka, S. H. Huttner, P. Ehrens, Kasem Mossavi, A. Lazzarini, S. C. McGuire, Daniel C. Woods, S. Klimenko, K. D. Giardina, Richard S. Savage, V. Pierro, J. Hanson, C. Cepeda, Julien Sylvestre, K. Rawlins, A. Moylan, Susan M. Scott, Teviet Creighton, A. L. Stuver, E. J. Daw, Boris Hage, K. Mailand, P. E. Lindquist, J. E. Brau, Maurizio Longo, J. Heefner, R. Grosso, Chad Hanna, K. Wette, J. C. Dumas, Curt Cutler, J. A. Giaime, Gianpietro Cagnoli, N. A. Lockerbie, Matthew Evans, L. Cardenas, R. Frey, Soumya D. Mohanty, X. Siemens, Richard J. Abbott, C. Wilkinson, W. R. Johnston, E. Chin, J. N. Marx, R. P. Croce, Krzysztof Belczynski, R. Mittleman, Nelson Christensen, Karel E. Urbanek, P. J. King, C. Parameswariah, P. Savov, James Whelan, P. G. Murray, N. Zotov, Roger Jones, Philip Nutzman, M. Heurs, K. Ryan, S. W. Ballmer, J. W C McNabb, Ik Siong Heng, F. Nocera, M. Pedraza, K. Kokeyama, D. Ugolini, A. G. Wiseman, P. Ajith, L. Zhang, B. Bhawal, K. Mason, M. Ramsunder, T. Z. Summerscales, S. Grunewald, V. Leonhardt, B. Bland, N. A. Robertson, R. L. Ward, G. Diederichs, I. Gholami, W. Wu, Gabriela Gonzalez, S. Ray-Majumder, R. Bork, J. Myers, Jonathan C. Leiner, V. Re, D. Hammer, M. Vallisneri, F. Seifert, Michael C. B. Ashley, P. T. Beyersdorf, V. Boschi, K. S. Ganezer, J. H. Hough, K. Kawabe, P. Charlton, C. N. Colacino, A. Rodriguez, M. Malec, Shourov Chatterji, D. Fazi, Helena Armandula, Rainer Weiss, Peter Kalmus, C. A. Cantley, N. Rainer, T. Delker, A. Di Credico, S. J. Waldman, Suvadeep Bose, C. Robinson, Massimo Tinto, C. Barker, Benjamin William Allen, Karsten Danzmann, P. Kwee, R. W. P. Drever, Yi Chen, R.L. Coldwell, Carlo Ungarelli, B. Rivera, Pablo Barriga, C. Gray, M. Mageswaran, I. A. Bilenko, V. Dergachev, Slawomir Gras, David J. Ottaway, K. Riles, Kenneth A. Strain, Marco G. Tarallo, J. Slutsky, Nicolás Yunes, A. Grant, Jolien D. E. Creighton, Vincenzo Matta, D. Webber, A. W. Heptonstall, Lindy Blackburn, V. Quetschke, Bangalore Suryanarayana Sathyaprakash, E. Black, Keisuke Goda, Yi Pan, Chunglee Kim, Martin M. Fejer, J. R. Smith, T. Nash, W. Kells, Erik Katsavounidis, C. Messenger, S. Wiley, A. Sazonov, M. J. Lubinski, R. M S Schofield, D. Jackrel, John G. Dwyer, Haisheng Rong, Vladimir B. Braginsky, H. Vahlbruch, L. Ribichini, G. H. Sanders, A. Ivanov, V. V. Frolov, E. Espinoza, E. Myers, Damien Mudge, S. P. Vyachanin, Kentaro Somiya, W. Tyler, D. C. Coyne, Stephen Fairhurst, Yousuke Itoh, Ping Koy Lam, Kenji Numata, David Coward, A. M. Gretarsson, Pamela J. Russell, S. Richman, Chunnong Zhao, David H. Shoemaker, P. Cochrane, Oliver Jennrich, Roger K. Route, O. Burmeister, Stefan Hild, B. Johnson, W. Winkler, D. Kasprzyk, M. Samidi, G. T. Jones, Giuseppe Castaldi, S. E. Whitcomb, S. Gossler, C. V. Torres, S. Wen, R. McCarthy, H. Bantilan, M. A. Barton, D.B. DeBra, K. Y. Franzen, J. A. Sidles, Fabio Postiglione, D. Sellers, P. J. Veitch, H. Radkins, A. Cumming, A. Dietz, M. Ito, F. Ya. Khalili, Atsushi J. Nishizawa, T. Etzel, S. Saraf, Roberto Conte, C. Aulbert, L. Matone, A. Sibley, E. Messaritaki, M. Lormand, Sanichiro Yoshida, Sheila Rowan, Graham Woan, Robert L. Byer, P. J. Sutton, Ke Sun, J. Dickson, Bernard F. Schutz, Li Ju, Jan Harms, A. S. Sengupta, S. J. Berukoff, J. Greenhalgh, Guido Mueller, H. Overmier, S. Meshkov, Vincenzo Galdi, Benjamin J. Owen, Christopher Wipf, A. Bunkowski, K. V. Tokmakov, R. Schilling, Martin Hewitson, Junwei Cao, E. Hirose, Juri Agresti, H. Müller-Ebhardt, Eric Howell, Michael Landry, G. Billingsley, V. Sandberg, Kirk McKenzie, Morag M. Casey, A. Thüring, A. C. Melissinos, The LIGO Scientific Collaboration, LSC Collaboration, The, Castaldi, G., Galdi, V., Pierro, V., and Pinto, I. M.

Subjects
Nuclear and High Energy Physics, Physics and Astronomy (miscellaneous), NEUTRON-STARS, Frequency band, FOS: Physical sciences, PARALLAX, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, Parameter space, 01 natural sciences, General Relativity and Quantum Cosmology, Radio spectrum, Pulsar, 0103 physical sciences, QC176, ddc:530, 010303 astronomy & astrophysics, Nuclear and High Energy Physic, QB, pulsar, Physics, parallax, 010308 nuclear & particles physics, Gravitational wave, PULSAR, neutron-stars, LIGO, radiation, Neutron star, Amplitude, RADIATION, Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik
Abstract

We carry out two searches for periodic gravitational waves using the most sensitive few hours of data from the second LIGO science run. The first search is targeted at isolated, previously unknown neutron stars and covers the entire sky in the frequency band 160-728.8 Hz. The second search targets the accreting neutron star in the low-mass X-ray binary Scorpius X-1, covers the frequency bands 464-484 Hz and 604-624 Hz, and two binary orbit parameters. Both searches look for coincidences between the Livingston and Hanford 4-km interferometers. For isolated neutron stars our 95% confidence upper limits on the gravitational wave strain amplitude range from 6.6E-23 to 1E-21 across the frequency band; For Scorpius X-1 they range from 1.7E-22 to 1.3E-21 across the two 20-Hz frequency bands. The upper limits presented in this paper are the first broad-band wide parameter space upper limits on periodic gravitational waves using coherent search techniques. The methods developed here lay the foundations for upcoming hierarchical searches of more sensitive data which may detect astrophysical signals., 35 pages, 30 figures

Published
2007
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26. Search for gravitational wave radiation associated with the pulsating tail of the SGR1806−20hyperflare of 27 December 2004 using LIGO

Author

M. R. Smith, I. Leonor, John K. Cannizzo, Alberto Vecchio, B. Lantz, Gianpietro Cagnoli, J. Myers, Shourov Chatterji, D. Fazi, S. J. Waldman, Suvadeep Bose, J. D. E. Creighton, H. Yamamoto, J. C. Dumas, R. P. Croce, Jong H. Chow, R. M. S. Schofield, B. Lee, Jonathan C. Leiner, R. Taylor, V. Re, Benno Willke, Albert Lazzarini, D. Hoak, J. Clark, G. Mendell, L. Ruet, Benjamin J. Owen, Christopher Wipf, K. V. Tokmakov, Rainer Weiss, D. Barker, G. Diederichs, R. W. P. Drever, K. D. Giardina, K. Kokeyama, W. W. Johnson, David Crooks, B. Bland, F. Ya. Khalili, A. Cumming, Martin Hewitson, Atsushi J. Nishizawa, Junwei Cao, Giuseppe Castaldi, M. V. Plissi, Soumya D. Mohanty, R. L. Savage, S. Roddy, N. Zotov, Alessandra Buonanno, D. J. Hosken, J. G. Rollins, Karel E. Urbanek, J. W C McNabb, David Blair, V. Leonhardt, A. J. Weinstein, K. Mason, Hartmut Grote, A. M. Sintes, Helena Armandula, Ke-Xun Sun, C. A. Cantley, A. M. Rogan, I. Gholami, W. Wu, C. Robinson, Benjamin William Allen, E. Innerhofer, S. Giampanis, Sanichiro Yoshida, A. M. Gretarsson, N. Rainer, G. P. Newton, M. Fyffe, Sanjeev Dhurandhar, S. Saraf, S. Ray-Majumder, Lee Samuel Finn, Karsten Danzmann, Roberto Conte, N. A. Lockerbie, N. Fotopoulos, R. Rahkola, Graham Woan, L. Matone, Robert L. Byer, Stuart Reid, Gabriela Gonzalez, P. T. Beyersdorf, Carlos Cepeda, P. E. Lindquist, Slawomir Gras, Peter Aufmuth, E. Messaritaki, Sheila Rowan, H. Rehbein, H. Bantilan, Jesper Munch, Robert J. McCarthy, C. N. Colacino, Stefano Marano, S. B. Anderson, L. Wallace, D. M. Whitbeck, R. Frey, Shuichi Sato, J. N. Marx, A. Sibley, Erika D'Ambrosio, M. Degree, M. Lormand, David B. Tanner, Stephen Fairhurst, R. J. Dupuis, Ravi Kumar Kopparapu, Bernard F. Schutz, Li Ju, J. Hanson, Yi Chen, B. Bhawal, M. Landry, S. H. Huttner, Vincenzo Galdi, M. A. Barton, R. L. Ward, M. Sung, A. M. Cruise, Guido Mueller, V. Boschi, Joseph D. Romano, Jared Markowitz, A. G. Wiseman, Kasem Mossavi, S. Sakata, S. Wen, A. Dietz, Shantanu Desai, M. Pedraza, Vuk Mandic, A. Bullington, Rahul Biswas, L. Bogue, Sean T. McWilliams, V. V. Frolov, J. H. Romie, Miquel Trias, K. Bayer, Rana X. Adhikari, Gareth Jones, J. A. Giaime, D. C. Coyne, Kip S. Thorne, F. J. Raab, Maria Alessandra Papa, R.L. Coldwell, V. Parameshwaraiah, P. Savov, B. Machenschalk, L. Ribichini, T. T. Fricke, Kevin M. Ryan, I. Yakushin, Hirotaka Takahashi, James Whelan, R. Gustafson, P. Ajith, D.B. DeBra, Kent Blackburn, V. P. Mitrofanov, S. Márka, Jordan Camp, E. Hirose, Juri Agresti, A. Bunkowski, J. Zhang, D. Chin, Supriyo Sinha, Stanislav Babak, M. Ito, N. A. Robertson, T. Meier, Guenakh Mitselmakher, Francesco Chiadini, A. Franzen, Kirk McKenzie, M. C. Araya, Richard O'Shaughnessy, B. Barr, P. Patel, Malik Rakhmanov, Kenneth A. Strain, Boris Hage, J. Dalrymple, C. Gray, J. Worden, L. Williams, H. Müller-Ebhardt, E. Myers, Duncan A. Brown, K. Y. Franzen, A. Rüdiger, B. O'Reilly, Morag M. Casey, M. Heurs, D. Hammer, F. Seifert, Yi Pan, Eric Howell, Eugeniy E. Mikhailov, S. Chelkowski, J. Dickson, C. I. Torrie, Jan Harms, A. S. Sengupta, J. Zweizig, Michael C. B. Ashley, J. A. Sidles, Matthew Evans, L. Cardenas, Kentaro Somiya, G. Billingsley, A. Grant, D. B. Kozak, C. Vorvick, Kenji Numata, Peter Kalmus, J. Greenhalgh, Innocenzo M. Pinto, R. Riesen, Evan Goetz, A. Thüring, S. Klimenko, A. C. Melissinos, Fabio Postiglione, T. Etzel, Carlo Ungarelli, Roland Schilling, Thomas Cokelaer, T. Z. Summerscales, P. Kwee, Marco G. Tarallo, L. Zhang, J. Slutsky, S. Meshkov, D. Webber, A. Weidner, D. Meyers, P. Schwinberg, V. Quetschke, Bangalore Suryanarayana Sathyaprakash, E. Black, Martin M. Fejer, J. R. Smith, Malcolm B. Gray, R. Bork, T. Nash, A. Brooks, P. Ehrens, Richard J. Abbott, P. J. Veitch, K. Wette, H. Zur Mühlen, W. G. Anderson, S. E. Whitcomb, S. Gossler, Timothy Evans, B. P. Abbott, D. Sigg, S. W. Ballmer, C. Aulbert, Chunnong Zhao, David H. Shoemaker, P. Cochrane, Roman Schnabel, Vincenzo Fiumara, J. E. Brau, G. Moreno, S. Vass, Subhasish Mitra, O. Burmeister, J. Thacker, W. Kells, D. Busby, H. Ward, Soma Mukherjee, Peter King, Drew Keppel, Zewu Yan, B. Johnson, D. Kasprzyk, P. G. Murray, M. Samidi, J. H. Hough, S. Wise, S. Grunewald, Douglas R. Cook, Michele Zanolin, Keisuke Goda, Erik Katsavounidis, Kenneth G. Libbrecht, M. J. Lubinski, D. Jackrel, K. Mailand, Maurizio Longo, John G. Dwyer, Krzysztof Belczynski, Vladimir B. Braginsky, H. Vahlbruch, R. Mittleman, K. Riles, Nelson Christensen, John Veitch, E. Espinoza, M. Weinert, Yousuke Itoh, Sascha Schediwy, M. MacInnis, Vincenzo Matta, R. S. Amin, Andreas Freise, Vincenzo Pierro, Matthew Pitkin, C. Messenger, M. Varvella, R. Wooley, T. Hayler, Ping Koy Lam, S. Kamat, J. Heefner, R. Grosso, M. A. Arain, Gregory M. Harry, I. Wilmut, F. Kawazoe, J. Garofoli, J. S. Kissel, M. Lei, Roger Jones, K. Kawabe, S. M. Aston, B. Rivera, Pablo Barriga, M. Mageswaran, I. W. Martin, Virginio Sannibale, David E. McClelland, Michele Vallisneri, Ik Siong Heng, Emma L. Robinson, V. Kondrashov, R. DeSalvo, E. E. Doomes, L. Sancho De La Jordana, K. Rawlins, C. Torres, A. Rodriguez, C. Barker, Daniel C. Woods, Pankaj Sarin, A. L. Stuver, Martin P McHugh, B. J. J. Slagmolen, K. Watts, E. Maros, P. Shawhan, P. Charlton, A. Di Credico, A. E. Villar, I. A. Bilenko, V. Dergachev, Nergis Mavalvala, Jerome Degallaix, David J. Ottaway, B. C. Barish, David Jones, A. Ivanov, H. Radkins, Damien Mudge, S. P. Vyachanin, Peter R. Saulson, M. Brinkmann, W. Tyler, Walter Winkler, David Coward, Harald Lück, D. S. Rabeling, R. A. Mercer, S. C. McGuire, Lindy Blackburn, Chunglee Kim, V. Sandberg, Massimo Tinto, Nicolás Yunes, Badri Krishnan, E. Chalkey, Antony C. Searle, C. M. Mow-Lowry, D. Hoyland, B. F. Whiting, C. Van Den Broeck, P. J. Sutton, J. Bogenstahl, Michael E Zucker, E. Chin, Marco Aurelio Diaz, S. Penn, Pamela J. Russell, Roger K. Route, K. A. Thorne, J. Betzwieser, D. Ugolini, Stefan Hild, H. Overmier, D. Sellers, M. Guenther, Patrick Brady, Seiji Kawamura, Reinhard Prix, Elizabeth Harstad, Osamu Miyakawa, David H. Reitze, Gavin Davies, B. Sears, Vicky Kalogera, Yaohui Fan, Laura Cadonati, A. Moylan, Susan M. Scott, Teviet Creighton, Chad Hanna, X. Siemens, C. Wilkinson, T. Demma, Peter Fritschel, K. C. Cannon, H. J. Pletsch, G. Traylor, Thomas Corbitt, A. Heptonstall, M. Malec, D. R. Ingram, Phil Willems, D. M. Strom, and Lisa M. Goggin

Subjects
Physics, Nuclear and High Energy Physics, 010308 nuclear & particles physics, Gravitational wave, Astrophysics::High Energy Astrophysical Phenomena, Astronomy, Astrophysics, Light curve, 01 natural sciences, Electromagnetic radiation, Asteroseismology, LIGO, law.invention, Neutron star, Amplitude, law, 0103 physical sciences, 010303 astronomy & astrophysics, Flare
Abstract

We have searched for gravitational waves (GWs) associated with the SGR 1806−20 hyperflare of 27 December 2004. This event, originating from a Galactic neutron star, displayed exceptional energetics. Recent investigations of the x-ray light curve’s pulsating tail revealed the presence of quasiperiodic oscillations (QPOs) in the 30–2000 Hz frequency range, most of which coincides with the bandwidth of the LIGO detectors. These QPOs, with well-characterized frequencies, can plausibly be attributed to seismic modes of the neutron star which could emit GWs. Our search targeted potential quasimonochromatic GWs lasting for tens of seconds and emitted at the QPO frequencies. We have observed no candidate signals above a predetermined threshold, and our lowest upper limit was set by the 92.5 Hz QPO observed in the interval from 150 s to 260 s after the start of the flare. This bound corresponds to a (90% confidence) root-sum-squared amplitude h^(90%)_(rss-det) =4.5×10^(−22) strain Hz^(−1/2) on the GW waveform strength in the detectable polarization state reaching our Hanford (WA) 4 km detector. We illustrate the astrophysical significance of the result via an estimated characteristic energy in GW emission that we would expect to be able to detect. The above result corresponds to 7.7×10^(46) erg (=4.3×10^(−8) M_⊙c^2), which is of the same order as the total (isotropic) energy emitted in the electromagnetic spectrum. This result provides a means to probe the energy reservoir of the source with the best upper limit on the GW waveform strength published and represents the first broadband asteroseismology measurement using a GW detector.

Published
2007
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27. Generation of a flat-top laser beam for gravitational wave detectors by means of a nonspherical Fabry-Perot resonator

Author

Erika D'Ambrosio, L. Pinard, D. Forest, Marco G. Tarallo, Phil Willems, Juri Agresti, B. Simoni, C. Michel, N. Morgado, John W. Miller, B. Lagrange, A. Remilleux, J. M. Mackowsky, J.-L. Montorio, and R. DeSalvo

Subjects
Physics, business.industry, Materials Science (miscellaneous), Curved mirror, Physics::Optics, Industrial and Manufacturing Engineering, law.invention, Resonator, Optics, Tilt (optics), law, Beam tilt, Optical cavity, Light beam, Physics::Accelerator Physics, Business and International Management, business, Adaptive optics, Beam (structure), Caltech Library Services
Abstract

We have tested a new kind of Fabry-Perot long-baseline optical resonator proposed to reduce the thermal noise sensitivity of gravitational wave interferometric detectors--the "mesa beam" cavity--whose flat top beam shape is achieved by means of an aspherical end mirror. We present the fundamental mode intensity pattern for this cavity and its distortion due to surface imperfections and tilt misalignments, and contrast the higher order mode patterns to the Gauss-Laguerre modes of a spherical mirror cavity. We discuss the effects of mirror tilts on cavity alignment and locking and present measurements of the mesa beam tilt sensitivity.

Published
2007

28. Status of Virgo detector

Author

F. Cleva, Francesco Cottone, R. De Rosa, L. Pinard, F. Martelli, Fausto Acernese, F. Garufi, G. Vajente, P. Ruggi, Fabio Marchesoni, R. Flaminio, D. Buskulic, Giorgio Ivan Russo, Leopoldo Milano, L. Di Fiore, B. Mours, M. Mantovani, Enrico Calloni, V. Brisson, Lisa Barsotti, D. Passuello, M. Barsuglia, F. Vetrano, C. Palomba, Alessandra Toncelli, Anna Dari, M. Alshourbagy, E. Campagna, H. Heitmann, N. Morgado, Marco G. Tarallo, A. Pasqualetti, M. Laval, M. Lorenzini, V. Reita, K. Qipiani, P. Rapagnani, S. Birindelli, Luca Gammaitoni, P. Puppo, C. N. Man, F. Cavalier, B. Dujardin, F. Nocera, F. Paoletti, J.-M. Mackowski, E. Chassande-Mottin, J.-Y. Vinet, C. Bradaschia, F. Ricci, S. Kreckelbergh, F. Travasso, M. Del Prete, S. Frasca, Alban Remillieux, Rosa Poggiani, A. C. Clapson, Silvio Pardi, F. Fidecaro, E. Cuoco, B. Lopez, S. Karkar, P. Amico, P. La Penna, V. Dattilo, G. Losurdo, M. Punturo, G. Ballardin, M. Tonelli, E. Genin, A. Brillet, François Bondu, V. Loriette, F. Beauville, F. Marion, D. Babusci, M. Yvert, P. Astone, D. Verkindt, Fabrizio Barone, Alessandra Corsi, Julien Moreau, C. Moins, S. Hebri, Marina Mazzoni, Patrice Hello, A. Di Virgilio, F. Frasconi, J. Marque, S. Bigotta, A. Giazotto, Saverio Avino, I. Ferrante, A. Masserot, Ettore Majorana, F. Antonucci, Iolanda Ricciardi, Salvatore Solimeno, F. Carbognani, Nelson Christensen, E. Tournefier, G. Giordano, Sofiane Aoudia, Elena Cesarini, D. Grosjean, R. Passaquieti, F. Piergiovanni, A. Gennai, M. Davier, Marie-Anne Bizouard, Christian Corda, F. Menzinger, L. Bosi, R. Gouaty, N. Letendre, A. Viceré, G. Cella, Claude Boccara, L. Giordano, S. Braccini, G. Guidi, R. Cavalieri, J.-P. Coulon, A. Eleuteri, Alessandro D. A. M. Spallicci, J.-D. Fournier, C. Tremola, I. Fiori, H. Vocca, N. Leroy, DE ROSA, Rosario, Milano, Leopoldo, Garufi, Fabio, F., Acernese, Calloni, Enrico, L., Di Fiore, Giordano, Lara, Solimeno, Salvatore, Avino, Saverio, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux ( ARTEMIS ), Université Nice Sophia Antipolis ( UNS ), Université Côte d'Azur ( UCA ) -Université Côte d'Azur ( UCA ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de la Côte d'Azur, Université Côte d'Azur ( UCA ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), ESPCI ParisTech, APC - Gravitation ( APC-Gravitation ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Max-Planck-Institut-Max-Planck-Institut, Laboratoire des matériaux avancés ( LMA ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Virgo, Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), VIRGO, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), APC - Gravitation (APC-Gravitation), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Laboratoire des matériaux avancés (LMA), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), and Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS)

Subjects
Physics, Gravitational-wave observatory, Physics and Astronomy (miscellaneous), 010308 nuclear & particles physics, Detector, Real-time computing, Astronomy, Limiting, 01 natural sciences, Continuous data, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], 0103 physical sciences, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Sensitivity (control systems), 010303 astronomy & astrophysics
Abstract

International audience; The commissioning of the Virgo gravitational wave detector has restarted after several major hardware upgrades carried out during winter 2005. Now Virgo is fully operative and its sensitivity greatly improved and continually improving. A program of short scientific data taking has already started and Virgo is moving towards a period of continuous data taking, which should start at the end of May 2007. The actual status of the Virgo detector is reported, describing the actual detector sensitivity as well as the limiting noises and the mid-term plans.

Published
2007
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29. Upper limit map of a background of gravitational waves

Author

K. Bayer, P. Shawhan, Ravi Kumar Kopparapu, A. M. Sintes, A. M. Cruise, J. Zweizig, Stefano Marano, S. M. Aston, Badri Krishnan, E. Chalkey, Antony C. Searle, K. Rawlins, S. Sakata, Miquel Trias, C. M. Mow-Lowry, E. Hirose, S. Vass, J. H. Romie, Juri Agresti, Vuk Mandic, G. Mitselmakher, V. Parameshwaraiah, D. Hoyland, S. Chelkowski, D. B. Kozak, H. Overmier, Richard O'Shaughnessy, B. Barr, P. Patel, Malik Rakhmanov, D. Barker, Vincenzo Galdi, J. Worden, L. Williams, A. Rüdiger, L. Ribichini, H. Müller-Ebhardt, C. Van Den Broeck, S. Roddy, Eric Howell, Michael Landry, M. R. Smith, V. Leonhardt, I. Gholami, W. Wu, D. Chin, Supriyo Sinha, Stanislav Babak, P. T. Beyersdorf, P. Aufmuth, Lee Samuel Finn, Duncan A. Brown, R. Riesen, B. O'Reilly, Seiji Kawamura, Reinhard Prix, Elizabeth Harstad, G. Billingsley, J. C. Dumas, V. Boschi, E. Myers, A. Weidner, Soumya D. Mohanty, R. Frey, T. Demma, P. J. King, J. Cannizzo, M. Heurs, A. Bullington, A. G. Wiseman, Osamu Miyakawa, David H. Reitze, V. Sandberg, A. Rodriguez, Rahul Biswas, L. Bogue, S. Klimenko, C. Barker, Kentaro Somiya, D. C. Coyne, I. Yakushin, P. G. Murray, N. Zotov, Hirotaka Takahashi, C. I. Torrie, A. Dietz, D. Meyers, A. Bunkowski, R.L. Coldwell, J. A. Giaime, P. Schwinberg, Sanichiro Yoshida, Richard J. Abbott, Innocenzo M. Pinto, Thomas Cokelaer, Sean T. McWilliams, S. Penn, K. Mason, Nicolás Yunes, K. Kokeyama, T. Evans, H. Zur Mühlen, W. G. Anderson, Maurizio Longo, Krzysztof Belczynski, R. Mittleman, M. C. Díaz, Kenji Numata, R. P. Croce, A. Grant, Graham Woan, Robert L. Byer, R. Schilling, M. Weinert, A. Cumming, S. Ray-Majumder, Peter Fritschel, V. Kondrashov, B. Sears, Pankaj Sarin, Karel E. Urbanek, Benno Willke, J. Clark, L. Ruet, J. N. Marx, J. Bogenstahl, Michael E Zucker, P. J. Sutton, Bernard F. Schutz, Li Ju, B. P. Abbott, T. Etzel, Nelson Christensen, B. Bland, C. N. Colacino, Jordan Camp, Malcolm B. Gray, D. Cook, D. Ugolini, Yaohui Fan, T. Meier, J. Dalrymple, Gabriela Gonzalez, G. Traylor, Guido Mueller, P. Charlton, Kirk McKenzie, Keisuke Goda, A. Di Credico, Yi Chen, J. Betzwieser, Francesco Chiadini, E. Messaritaki, M. Lormand, D. R. Ingram, A. Franzen, G. Newton, Richard S. Savage, V. Pierro, Alessandra Buonanno, K. A. Thorne, Sheila Rowan, C. Vorvick, S. Mukherjee, B. Bhawal, G. Moreno, M. Ito, Vincenzo Fiumara, Rana X. Adhikari, Gareth Jones, D. Busby, C. A. Cantley, H. Rehbein, S. Meshkov, I. A. Bilenko, V. Dergachev, K. Watts, S. B. Anderson, M. J. Lubinski, B. F. Whiting, B. Machenschalk, Martin P McHugh, B. J. J. Slagmolen, E. Chin, D. S. Rabeling, Stephen Fairhurst, M. Zanolin, J. Hanson, C. Cepeda, J. E. Brau, Gianpietro Cagnoli, J. Zhang, David J. Ottaway, J. Dickson, Jan Harms, A. S. Sengupta, K. Mailand, David B. Tanner, Matthew Evans, E. Innerhofer, S. Giampanis, R. M S Schofield, D. Jackrel, J. Greenhalgh, H. J. Pletsch, Thomas Corbitt, K. D. Giardina, R. Bork, M. Pedraza, C. Robinson, Benjamin William Allen, Karsten Danzmann, C. Gray, Slawomir Gras, L. Cardenas, J. Thacker, A. E. Villar, N. Fotopoulos, R. Rahkola, S. E. Whitcomb, S. Gossler, R. Taylor, Marco G. Tarallo, R. A. Mercer, Giuseppe Castaldi, F. Ya. Khalili, Atsushi J. Nishizawa, Benjamin J. Owen, Harald Lück, G. Diederichs, Drew Keppel, Zewu Yan, M. Sung, S. Dhurandhar, A. F. Brooks, A. J. Weinstein, Christopher Wipf, K. V. Tokmakov, J. Myers, M. Guenther, Patrick Brady, S. C. McGuire, A. M. Rogan, Erika D'Ambrosio, B. Lee, S. Saraf, John G. Dwyer, Vladimir B. Braginsky, Martin Hewitson, Junwei Cao, J. Slutsky, D. Webber, Maria Alessandra Papa, Laura Cadonati, W. W. Johnson, M. Degree, Shourov Chatterji, D. Hoak, D. Fazi, S. J. Waldman, Suvadeep Bose, Roberto Conte, David Jones, Nergis Mavalvala, Jerome Degallaix, C. Aulbert, E. Goetz, Jesper Munch, Kent Blackburn, M. V. Plissi, I. Leonor, T. Z. Summerscales, L. Matone, B. C. Barish, Alberto Vecchio, A. Moylan, Susan M. Scott, G. S. Davies, Teviet Creighton, R. DeSalvo, H. Vahlbruch, E. Espinoza, J. H. Hough, S. Wise, K. Ryan, V. Quetschke, K. Kawabe, Peter R. Saulson, Bangalore Suryanarayana Sathyaprakash, E. Black, Shantanu Desai, Kip S. Thorne, E. E. Doomes, R. L. Ward, A. Sibley, Martin M. Fejer, Helena Armandula, J. R. Smith, Ke-Xun Sun, A. L. Stuver, Hartmut Grote, N. Rainer, R. J. Dupuis, R. Gustafson, L. Sancho De La Jordana, P. Kwee, S. Reid, Kenneth G. Libbrecht, Jonathan C. Leiner, Chad Hanna, V. Kalogera, D. M. Strom, X. Siemens, C. Wilkinson, V. Re, V. P. Mitrofanov, Yousuke Itoh, P. E. Lindquist, M. C. Araya, W. Kells, D. J. Hosken, Boris Hage, E. Katsavounidis, Vincenzo Matta, D. M. Whitbeck, A. W. Heptonstall, A. Ivanov, J. W C McNabb, S. Márka, K. C. Cannon, S. H. Huttner, Daniel C. Woods, N. A. Robertson, Damien Mudge, Rainer Weiss, Roman Schnabel, T. T. Fricke, S. P. Vyachanin, D. Hammer, M. Vallisneri, F. Seifert, Michael C. B. Ashley, Subhasish Mitra, W. Tyler, J. Heefner, R. Grosso, Kenneth A. Strain, Shuichi Sato, Eugeniy E. Mikhailov, A. M. Gretarsson, David Coward, C. Messenger, Peter Kalmus, C. V. Torres, Carlo Ungarelli, Y. Pan, N. A. Lockerbie, E. Maros, R. W. P. Drever, P. Savov, James Whelan, P. Ajith, Ik Siong Heng, L. Zhang, Emma L. Robinson, Pamela J. Russell, S. Grunewald, Roger K. Route, Joseph D. Romano, Jared Markowitz, S. Wen, Kasem Mossavi, A. Lazzarini, David Blair, K. Riles, Stefan Hild, Chunnong Zhao, Jolien D. E. Creighton, M. Malec, Phil Willems, Lindy Blackburn, David H. Shoemaker, P. Cochrane, Chunglee Kim, O. Burmeister, H. Yamamoto, B. Lantz, F. J. Raab, Lisa M. Goggin, B. Johnson, W. Winkler, D. Kasprzyk, M. Samidi, H. Radkins, R. McCarthy, H. Bantilan, M. A. Barton, D.B. DeBra, K. Y. Franzen, J. A. Sidles, Fabio Postiglione, D. Sellers, P. J. Veitch, Andreas Freise, Matthew Pitkin, J. G. Rollins, G. Mendell, M. Varvella, R. Wooley, V. Sannibale, T. Hayler, H. Ward, L. Wallace, John Veitch, Sascha Schediwy, M. MacInnis, R. S. Amin, I. Wilmut, F. Kawazoe, J. Garofoli, J. S. Kissel, Roger Jones, B. Rivera, Pablo Barriga, M. Mageswaran, V. V. Frolov, Ping Koy Lam, D. Sigg, M. A. Arain, Gregory M. Harry, M. Lei, M. Fyffe, Morag M. Casey, A. Thüring, A. C. Melissinos, I. W. Martin, David E. McClelland, P. Ehrens, K. Wette, S. W. Ballmer, Jong H. Chow, David Crooks, M. Brinkmann, The LIGO Scientific Collaboration, LSC Collaboration, The, Castaldi, G., Galdi, V., Pierro, V., and Pinto, I. M.

Subjects
Nuclear and High Energy Physics, Physics and Astronomy (miscellaneous), FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, 01 natural sciences, Power law, General Relativity and Quantum Cosmology, Gravitational wave background, QC350, 0103 physical sciences, ddc:530, Limit (mathematics), 010306 general physics, QC, QB, Nuclear and High Energy Physic, Physics, 010308 nuclear & particles physics, Gravitational wave, Astrophysics (astro-ph), Isotropy, Spectral density, LIGO, radiation, Amplitude, RADIATION, Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik
Abstract

We searched for an anisotropic background of gravitational waves using data from the LIGO S4 science run and a method that is optimized for point sources. This is appropriate if, for example, the gravitational wave background is dominated by a small number of distinct astrophysical sources. No signal was seen. Upper limit maps were produced assuming two different power laws for the source strain power spectrum. For an f^-3 power law and using the 50 Hz to 1.8 kHz band the upper limits on the source strain power spectrum vary between 1.2e-48 Hz^-1 (100 Hz/f)^3 and 1.2e-47 Hz^-1 (100 Hz /f)^3, depending on the position in the sky. Similarly, in the case of constant strain power spectrum, the upper limits vary between 8.5e-49 Hz^-1 and 6.1e-48 Hz^-1. As a side product a limit on an isotropic background of gravitational waves was also obtained. All limits are at the 90% confidence level. Finally, as an application, we focused on the direction of Sco-X1, the closest low-mass X-ray binary. We compare the upper limit on strain amplitude obtained by this method to expectations based on the X-ray luminosity of Sco-X1., Comment: 11 pages, 9 figures, 2 tables

Published
2007

30. The real-time distributed control of the Virgo Interferometric Detector for Gravitational Waves

Author

R. De Rosa, S. Bigotta, M. Alshourbagy, F.P.D. Passuello, C. N. Man, J. Y. Vinet, F. Fidecaro, C. Tremola, G. Ballardin, E. Campagna, F. Martelli, Fausto Acernese, M. Lorenzini, C. Mottin, C. Palomba, M. Mantovani, D. Passuello, M. Barsuglia, M. Tonelli, V. Reita, P. Ruggi, E. Genin, H. Vocca, N. Morgado, A. Giazotto, A. Pasqualetti, A. Gennai, F. Cleva, Francesco Cottone, L. Pinard, I. Ferrante, G. Vajente, G. Guidi, Fabio Marchesoni, P. Hello, Alban Remillieux, F. Ricci, D. Verkindt, Salvatore Solimeno, L. Giordano, Th. Bauer, F. Travasso, L. Milano, B. Dujardin, V. Loriette, H. Heitmann, Claude Boccara, P. Amico, F. Marion, R. Flaminio, S. Hamdani, P. La Penna, A. Spallicci, Lisa Barsotti, N. Leroy, François Bondu, F. Cavalier, G. Cella, A. Masserot, Enrico Calloni, Alessandra Toncelli, C. Moins, D. Grosjean, B. Mours, G. Losurdo, Alessandra Corsi, F. Frasconi, Anna Dari, M. Punturo, F. Paoletti, S. Braccini, M. A. Bizouard, Matthew Evans, Fabrizio Barone, L. Bosi, M. Del Prete, S. Frasca, Nelson Christensen, L. Gamaitoni, A. Di Virgilio, A. Viceré, S. Hebri, N. Letendre, Saverio Avino, Ketevan Qipiani, D. Buskulic, Silvio Pardi, L. Di Fiori, Antonio Eleuteri, S. Kreckelbergh, R. Cavalieri, M. Yvert, E. Cuoco, B. Lopez, S. Birindelli, F. Antonucci, V. Brisson, J. F. J. van den Brand, Elena Cesarini, D. Babusci, G.V. Russo, E. Tournefier, P. Puppo, Julien Moreau, R. Passaquieti, R. Gouaty, F. Beauville, F. Nocera, J.-P. Coulon, F. Piergiovanni, J.-D. Fournier, G. Giordano, M. Davier, P. Rapagnani, Ettore Majorana, A.-C. Clapson, M. Laval, I. Fiori, Rosa Poggiani, S. Van Der Putten, Christian Corda, Marco G. Tarallo, J.-M. Mackowski, C. Bradaschia, P. Astone, Sofiane Aoudia, Marina Mazzoni, Iolanda Ricciardi, F. Carbognani, D. Huet, F. Menzinger, F. Vetrano, S. Karkar, V. Dattilo, A. Brillet, F. Garuli, J. Marque, Garufi, Fabio, Avino, Saverio, Calloni, Enrico, DE ROSA, Rosario, Giordano, Lara, Milano, Leopoldo, Pardi, Silvio, Russo, Guido, Solimeno, Salvatore, THE VIRGO, Collaboration, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux ( ARTEMIS ), Université Nice Sophia Antipolis ( UNS ), Université Côte d'Azur ( UCA ) -Université Côte d'Azur ( UCA ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de la Côte d'Azur, Université Côte d'Azur ( UCA ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), ESPCI ParisTech, APC - Gravitation ( APC-Gravitation ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Max-Planck-Institut-Max-Planck-Institut, Laboratoire des matériaux avancés ( LMA ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Virgo, Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), VIRGO, Amico, P., Alshourbagy, M., Antonucci, F., Aoudia, S., Astone, P., Babusci, D., Barillé, R., Ballardin, G., Barone, F., Barsotti, L., Barsuglia, M., Bauer, T. S., Beauville, F., Bigotta, S., Bizouard, M. A., Boccara, C., Bondu, F., Bosi, L., Bradaschia, C., Birindelli, S., Braccini, S., van den Brand, J. F. J., Brillet, A., Brisson, V., Buskulic, D., Campagna, E., Carbognani, F., Cavalier, F., Cavalieri, R., Cella, G., Cesarini, E., Chassande Mottin, E., Christensen, N., Clapson, A. C., Cleva, F., Corda, C., Corsi, A., Cottone, F., Coulon, J. P., Cuoco, E., Dari, A., Dattilo, V., Davier, M., del Prete, M., Di Fiore, L., Di Virgilio, A., Dujardin, B., Eleuteri, A., Evans, M., Ferrante, I., Fidecaro, F., Fiori, I., Flaminio, R., Fournier, J. D., Frasca, S., Frasconi, F., Freise, A., Gammaitoni, L., Genin, E., Gennai, A., Giazotto, A., Giordano, G., Gouaty, R., Grosjean, D., Guidi, G., Hamdani, S., Hebri, S., Heitmann, H., Hello, P., Huet, D., Karkar, S., Kreckelbergh, S., La Penna, P., Laval, M., Leroy, N., Letendre, N., Lopez, B., Lorenzini, M., Loriette, V., Losurdo, G., Mackowski, J. M., Majorana, E., Man, C. N., Mantovani, M., Marchesoni, F., Marion, F., Marque, J., Martelli, F., Masserot, A., Mazzoni, M., Menzinger, F., Moins, C., Moreau, J., Morgado, N., Mours, B., Nocera, F., Palomba, C., Paoletti, F., Pasqualetti, A., Passaquieti, R., Passuello, D., Piergiovanni, F., Pinard, L., Poggiani, R., Punturo, M., Puppo, P., van der Putten, S., Qipiani, K., Rapagnani, P., Reita, V., Remillieux, A., Ricci, F., Ricciardi, I., Ruggi, P., Solimeno, S., Spallicci, A., Tarallo, M., Tonelli, M., Toncelli, A., Tournefier, E., Travasso, F., Tremola, C., Vajente, G., Verkindt, D., Vetrano, F., Vicere, A., Vinet, J. Y., Vocca, H., Yvert, M., (Astro)-Particles Physics, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), APC - Gravitation (APC-Gravitation), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Laboratoire des matériaux avancés (LMA), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), and Geometry

Subjects
Nuclear and High Energy Physics, LOCKING, Computer science, data acquisition, 01 natural sciences, Gravitational waves, Optics, Data acquisition, 0103 physical sciences, Electronic engineering, Digital control, Sensitivity (control systems), [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Electrical and Electronic Engineering, 010306 general physics, Innovation, [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Physics, business.industry, 010308 nuclear & particles physics, Gravitational wave, Detector, Real time systems, SENSOR, interferometry, Interferometry, Nuclear Energy and Engineering, gravitational waves, real time systems, Control system, and Infrastructure, SDG 9 - Industry, Innovation, and Infrastructure, business, Distributed control system, SDG 9 - Industry, SYSTEM
Abstract

The VIRGO experiment for the detection of gravitational waves is a big challenge both for physics and for technology. In particular, to satisfy the stringent requirements on the alignment and position of its suspended optical components to keep the detector at its point, a very complex distributed and supervised control system has been implemented. The current constraints are about 10(-10) m RMS for the longitudinal control ("Locking") and 10(-9) rad RMS for the angular degrees of freedom ("Alignment"). These requirements are satisfied by means of a specially designed hierarchical architecture for the local control system. It is necessary for managing the hard task of filtering all the environmental noises that limit the sensitivity of the interferometer. On the other end, the interferometer is supervised by a distributed global control system to maintain the detector fully operational. In this paper we describe the status of the real-time distributed control system of the Virgo interferometric detector of Gravitational waves, its performances and planned improvements.

Published
2007
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31. Strontium optical lattice clock with all semiconductor sources

Author

Marco G. Tarallo, Nicola Poli, Marco Prevedelli, R. E. Drullinger, and Guglielmo M. Tino

Subjects
Optical lattice, Materials science, business.industry, Physics::Optics, Semiconductor device, Laser, Atomic clock, law.invention, Wavelength, Finesse, Semiconductor, Ultracold atom, law, Optoelectronics, Strontium, optical lattice clock, semiconductor lasers, Physics::Atomic Physics, Atomic physics, business
Abstract

We report on our progress toward the realization of an optical frequency standard referenced to strontium intercombination lines. Our current setup allows the production of ultracold Sr atoms in hundreds of ms. For high resolution spectroscopy of 1S0-3P0 doubly forbidden transition we have also prepared a 698 nm clock laser stabilized on high finesse symmetrically suspended cavity and a high power 813 nm light source for the optical lattice trap at the magic wavelength. All the laser source employed are based on semiconductor device. This opens the way to the realization of compact, reliable and eventually transportable optical frequency standards.

Published
2007

32. Measurement of the optical parameters of the Virgo interferometer

Author

Vicenzo Datillo, Christophe Moins, L. Giordano, E. Cuoco, Laurent Pinard, G. Giordano, F. Martelli, Gianluca Guidi, M. Punturo, Leopoldo Milano, F. Marion, Luciano Di Fiore, B. Mours, A. Masserot, F. Garufi, Olivier Francois, Luca Gammaitoni, Bénédicte Dujardin, F. Frasconi, Francesco Cottone, G. Vajente, L. Bosi, M. Mazzoni, M. Del Prete, S. Frasca, R. Flaminio, D. Passuello, Nicolas Leroy, M. Barsuglia, Nelson Christensen, Laura Brocco, R. Passaquieti, Archana Pai, F. Paoletti, F. Cavalier, H. Heitmann, P. Ruggi, Sonia Karkar, A. Viceré, Salem Hebri, Elena Cesarini, F. Menzinger, D. Babusci, Iolanda Ricciardi, Fabrice Beauville, F. Carbognani, A. Pasqualetti, E. Genin, Alessandra Corsi, Mohamed Alshourbagy, Mikael Laval, F. Fidecaro, B. Perniola, P. Rapagnani, M. Davier, Matteo Lorenzini, C. Tremola, Angela Di Virgilio, V. Brisson, Rosario De Rosa, C. Palomba, Rosa Poggiani, Enrico Campagna, Fabrizio Barone, Jean Yves Vinet, G. Ballardin, A. Gennai, Saverio Avino, Paolo La Penna, Stephane Kreckelbergh, Salvatore Solimeno, Irene Fiori, Federica Antonucci, Daniel Grosjean, N. Morgado, F. Ricci, V. Loriette, Guido Russo, P. Puppo, H. Vocca, R. Gouaty, A. Giazotto, I. Ferrante, Cleva Frédéric, Catherine Nary-Man, N. Letendre, Fausto Acernese, Stefano Bigotta, Giancarlo Cella, Antonio Eleuteri, M. Mantovani, R. Cavalieri, Jean Daniel Fourier, M. Yvert, Ruggero Stanga, Albert-Claude Boccara, Alban Remillieux, D. Verkindt, Lisa Barsotti, Marco G. Tarallo, Alessandra Toncelli, Julien Moreau, J.-P. Coulon, F. Piergiovanni, François Bondu, Edwige Tournefier, Alessandro D. A. M. Spallicci, F. Travasso, Ketevan Qipiani, P. Amico, D. Buskulic, Silvio Pardi, B. Lopez, Fabio Marchesoni, Mauro Tonelli, Flavia Vetrano, V. Reita, G. Losurdo, C. Bradaschia, P. Astone, Jean-Marie Mackowski, Sofiane Aoudia, Eric Chassande-Motin, Marie-Anne Bizouard, Christian Corda, Enrico Calloni, J. Marque, F. Nocera, S. Braccini, Simona Birindelli, Ettore Majorana, Patrice Hello, Andre-Claude Clapson, A. Brillet, Anna Dari, Acernese, F, Alshourbagy, M, Amico, P, Aoudia, S, Antonucci, F, Astone, P, Avino, S, Babusci, D, Ballardin, G, Barone, F, Barsuglia, M, Barsotti, L, Beauville, F, Bigotta, S, Birindelli, S, Bizouard, Ma, Boccara, Ac, Bondu, F, Bosi, L, Braccini, S, Bradaschia, C, Brillet, A, Brisson, V, Brocco, L, Buskulic, D, Calloni, Enrico, Campagna, E, Cavalier, F, Carbognani, F, Cavalieri, R, Cella, G, Cesarini, E, Chassande Motin, E, Christensen, N, Clapson, Ac, Frédéric, C, Corda, C, Corsi, A, Cottone, F, Coulon, Jp, Cuoco, E, Dari, A, Datillo, V, Davier, M, del Prete, M, DE ROSA, Rosario, Di Fiore, L, Di Virgilio, A, Dujardin, B, Eleuteri, A, Ferrante, I, Fidecaro, F, Fiori, I, Flaminio, R, Fourier, Jd, Frasca, S, Frasconi, F, Francois, O, Gammaitoni, L, Garufi, Fabio, Genin, E, Gennai, A, Giazotto, A, Giordano, G, Giordano, L, Gouaty, R, Grosjean, D, Guidi, Gm, Hebri, S, Heitmann, H, Hello, P, Karkar, S, Kreckelbergh, S, La Penna, P, Laval, M, Leroy, N, Letendre, N, Lopez, B, Lorenzini, M, Loriette, V, Losurdo, G, Mackowski, Jm, Majorana, E, Mantovani, M, Marchesoni, F, Marion, F, Marque, J, Martelli, F, Masserot, A, Mazzoni, M, Menzinger, F, Moreau, J, Milano, Leopoldo, Moins, C, Morgado, N, Mours, B, Nary Man, C, Nocera, F, Pai, A, Palomba, C, Paoletti, F, Pardi, S, Pasqualetti, A, Passaquieti, R, Passuello, D, Perniola, B, Piergiovanni, F, Pinard, L, Poggiani, R, Punturo, M, Puppo, P, Qipiani, K, Rapagnani, P, Ricci, F, Reita, V, Remillieux, A, Ricciardi, I, Ruggi, P, Russo, Guido, Solimeno, Salvatore, Spallicci, A, Stanga, R, Tarallo, M, Toncelli, A, Tonelli, M, Tournefier, E, Travasso, F, Tremola, C, Vajente, G, Verkindt, D, Vetrano, F, Viceré, A, Vinet, Jy, Vocca, H, and Yvert, M.

Subjects
Physics, Gravitational wave, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Materials Science (miscellaneous), Astrophysics::Instrumentation and Methods for Astrophysics, Phase (waves), Virgo interferometer, Astrophysics::Cosmology and Extragalactic Astrophysics, Industrial and Manufacturing Engineering, parametri ottici, General Relativity and Quantum Cosmology, Optics, Onde gravitazionali, interferometri, Business and International Management, business, Astrophysics::Galaxy Astrophysics
Abstract

The Virgo interferometer, aimed at detecting gravitational waves, is now in a commissioning phase. Measurements of its optical properties are needed for the understanding of the instrument. We present the techniques developed for the measurement of the optical parameters of Virgo. These parameters are compared with the Virgo specifications.

Published
2007

33. Gravitational waves by gamma-ray bursts and the virgo detector: the case of GRB 050915a

Author

G. Ballardin, D. Grosjean, Frédérique Marion, C. Tremola, N. Letendre, K. Qipiani, P. Puppo, A. Gennai, M. Punturo, G. Losurdo, A. Di Virgilio, Luca Gammaitoni, S. Kreckelbergh, Matthew Evans, H. Vocca, F. Paoletti, Francesco Cottone, L. Pinard, F. Garufi, M. Yvert, R. Cavalieri, S. Hamdani, M. A. Bizouard, F. Frasconi, M. Del Prete, G. Vajente, S. Frasca, C. Palomba, R. Flaminio, L. Bosi, Anna Dari, F. Menzinger, Iolanda Ricciardi, Leopoldo Milano, J.-P. Coulon, A. Eleuteri, G. Cella, H. Heitmann, Alessandro D. A. M. Spallicci, F. Carbognani, Nelson Christensen, F. Ricci, Fabio Marchesoni, E. Tournefier, J.-D. Fournier, A. Viceré, P. Ruggi, Alban Remillieux, Elena Cesarini, I. Fiori, Giorgio Ivan Russo, V. Brisson, S. Birindelli, M. Alshourbagy, V. Dattilo, D. Huet, Julien Moreau, D. Babusci, L. Giordano, R. Passaquieti, F. Cavalier, J.-Y. Vinet, Claude Boccara, Marina Mazzoni, F. Piergiovanni, M. Davier, V. Reita, François Bondu, M. Tonelli, R. De Rosa, F. Martelli, E. Campagna, V. Loriette, Fausto Acernese, M. Mantovani, G. Giordano, N. Leroy, C. Bradaschia, Salvatore Solimeno, A. Brillet, Th S. Bauer, Alessandra Corsi, N. Morgado, Fabrizio Barone, S. Hebri, Saverio Avino, F. Antonucci, F. Travasso, F. Cleva, P. Amico, P. La Penna, F. J. van den Brand, D. Buskulic, C. Moins, S. Braccini, B. Mours, Enrico Calloni, D. Verkindt, Sofiane Aoudia, M. Laval, S. Bigotta, P. Rapagnani, F. Beauville, F. Fidecaro, L. Di Fiore, D. Passuello, M. Barsuglia, E. Chassande-Mottin, Ettore Majorana, J. Marque, F. Nocera, Rosa Poggiani, S. Karkar, Christian Corda, S. Van Der Putten, B. Dujardin, F. Vetrano, Patrice Hello, A. Masserot, Marco G. Tarallo, G. Guidi, C. N. Man, J.-M. Mackowski, A. Giazotto, I. Ferrante, A. Pasqualetti, Lisa Barsotti, Alessandra Toncelli, M. Lorenzini, E. Genin, P. Astone, Silvio Pardi, E. Cuoco, B. Lopez, A. C. Clapson, R. Gouaty, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux ( ARTEMIS ), Université Nice Sophia Antipolis ( UNS ), Université Côte d'Azur ( UCA ) -Université Côte d'Azur ( UCA ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de la Côte d'Azur, Université Côte d'Azur ( UCA ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), ESPCI ParisTech, APC - Gravitation ( APC-Gravitation ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Max-Planck-Institut-Max-Planck-Institut, Laboratoire des matériaux avancés ( LMA ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Virgo, Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), VIRGO, Milano, Leopoldo, Calloni, Enrico, DE ROSA, Rosario, Garufi, Fabio, Avino, Saverio, I., Ricciardi, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), APC - Gravitation (APC-Gravitation), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Laboratoire des matériaux avancés (LMA), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), and Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)

Subjects
Swift Gamma-Ray Burst Mission, Gravitational-wave observatory, Physics and Astronomy (miscellaneous), NEUTRON-STARS, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics, 01 natural sciences, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], BINARIES, General Relativity and Quantum Cosmology, 0103 physical sciences, 010303 astronomy & astrophysics, BLACK-HOLES, SUPERNOVA, Physics, PROGENITORS, 010308 nuclear & particles physics, Gravitational wave, Detector, Astronomy, 28 FEBRUARY 1997, ERROR BOX, Supernova, Neutron star, Amplitude, AFTERGLOWS, GRBS, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], RADIATION, Gamma-ray burst
Abstract

International audience; In the framework of the expected association between gamma-ray bursts and gravitational wave signals, we present the preliminary results of an analysis aimed to search for bursts of gravitational waves associated with the long GRB 050915a. GRB 050915a was detected by the Swift satellite in 2005, when the Virgo detector was engaged in one of its science runs, namely the C7 run, during which the best sensitivity attained in 2005 was exhibited. This offered the opportunity for the first coincident analysis between a gamma-ray burst and the Virgo gravitational wave detector. Here we give an overview of this ongoing analysis, which at the end will play the role of a prototype, crucial in defining a methodology for gamma-ray burst triggered searches with Virgo. The final results of our analysis will also allow us to evaluate up to which level Virgo will be able to constrain the amplitude of the gravitational wave signal from a typical long gamma-ray burst.

Published
2007
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34. Searching for a stochastic background of gravitational waves with the laser interferometer gravitational-wave observatory

Author

R. Grosso, Seiji Kawamura, Reinhard Prix, Elizabeth Harstad, O. Miyakawa, Walter Winkler, B. Sears, M. R. Smith, Harald Lück, R. Riesen, Michele Vallisneri, Ik Siong Heng, S. C. McGuire, A. Dietz, P. Hoang, C. Barker, David H. Reitze, C. Aulbert, G. Billingsley, B. Lee, W. Kells, A. Heptonstall, S. H. Huttner, R. Bork, E. D'Ambrosio, D. Cook, V. Leonhardt, D. I. Jones, S. Meshkov, R. Wooley, S. Sakata, L. Wallace, A. M. Cruise, S. Penn, Marco G. Tarallo, J. Slutsky, V. Quetschke, Bangalore Suryanarayana Sathyaprakash, Martin M. Fejer, J. R. Smith, K. Mailand, J. Thacker, D. Chin, Stanislav Babak, Roger K. Route, Duncan A. Brown, K. Rawlins, C. Messenger, D. M. Strom, P. Willems, M. Lubinski, Michael E Zucker, J. Garofoli, W. G. Anderson, I. Leonor, John K. Cannizzo, Jolien D. E. Creighton, Gavin Davies, M. Samidi, Lee Samuel Finn, K. Blackburn, Miquel Trias, M. Pedraza, K. A. Thorne, E. Myers, J. Hanson, Soumya D. Mohanty, D. Ugolini, B. Abbott, S. B. Anderson, Albrecht Rüdiger, Stefan Hild, Gabriela Gonzalez, Lindy Blackburn, D. Sellers, H. Overmier, R. J. Dupuis, P. G. Murray, J. Worden, D. Meyers, G. Diederichs, M. Lormand, N. Zotov, G. Mendell, W. Hua, Martin P McHugh, Vicky Kalogera, Chunglee Kim, M. Fyffe, M. Ito, J. H. Hough, Richard O'Shaughnessy, B. Barr, Malik Rakhmanov, Nergis Mavalvala, Jerome Degallaix, A. Sibley, Sarah J. Vigeland, K. Mason, A. Brooks, Guenakh Mitselmakher, S. Wen, Ping Koy Lam, B. J. J. Slagmolen, S. Márka, A. Villar, H. Yamamoto, C. Vorvick, J. A. Giaime, R. Savage, Peter Fritschel, P. Kwee, E. E. Doomes, K. C. Cannon, J. Romie, F. Ya. Khalili, S. Ray-Majumder, Roland Schilling, J. Myers, Kenneth A. Strain, Yaohui Fan, A. Weidner, Chunnong Zhao, A. Bunkowski, P. Russell, J. Heefner, Andre Thüring, E. J. Elliffe, Helge Müller-Ebhardt, David H. Shoemaker, H. Armandula, M. A. Barton, L. Sancho De La Jordana, S. Gossler, D. Kozak, Rana X. Adhikari, Gareth Jones, I. Yakushin, B. Machenschalk, A. M. Rogan, Nicolás Yunes, C. N. Colacino, C. Wilkinson, Peter R. Saulson, P. Schwinberg, G. Traylor, F. J. Raab, V. V. Frolov, J. Betzwieser, Thomas Corbitt, D.B. DeBra, J. C. Dumas, M. Guenther, D. Ingram, K. Y. Franzen, M. Malec, Yi Chen, Scott Koranda, Daniel C. Woods, L. Matone, G. Moreno, D. I. Robertson, Gregory M. Harry, N. Hindman, D. Busby, Thomas Cokelaer, K. Wette, J. N. Marx, S. Wise, Matthew Pitkin, D. Kasprzyk, I. Gholami, Laura Cadonati, S. Grunewald, D. Hoak, K. Kokeyama, A. Khan, M. Zanolin, D. B. Tanner, B. Bhawal, A. Moylan, Susan M. Scott, Benjamin Sheard, I. W. Martin, Malcolm B. Gray, Chad Hanna, Curt Cutler, X. Siemens, M. Mageswaran, K. Bayer, Clive C. Speake, P. J. Veitch, Marco Aurelio Diaz, S. Chatterji, David E. McClelland, A. L. Stuver, M. Lei, R. Frey, C. Torrie, Kenneth G. Libbrecht, Damien Mudge, V. Re, S. P. Vyachanin, S. Roddy, D. J. Hosken, V. Sandberg, J. G. Rollins, B. Bland, R. Abbott, R. Gustafson, A. G. Wiseman, Alicia M. Sintes, V. Kondrashov, T. Hayler, P. Ehrens, H. Rehbein, Fumiko Kawazoe, David Coward, A. Lazzarini, Krzysztof Belczynski, R. DeSalvo, C. Torres, A. Rodriguez, Kentaro Somiya, B. F. Whiting, S. Giampanis, R. Mittleman, Nelson Christensen, K. Watts, D. M. Whitbeck, P. Charlton, E. Chin, Soma Mukherjee, A. Di Credico, D. S. Rabeling, S. E. Seader, Kenji Numata, S. Dhurandar, J. Zweizig, A. Franzen, R. Rahkola, P. Sarin, I. A. Bilenko, V. Dergachev, Rainer Weiss, David J. Ottaway, P. Lindquist, K. Ryan, W. Tyler, R. W. P. Drever, R. A. Mercer, V. Sannibale, W. W. Johnson, Stephen Fairhurst, T. T. Fricke, Z. Yan, C. Gray, J. Dickson, Jan Harms, A. S. Sengupta, E. Hirose, Juri Agresti, Jesper Munch, J. W C McNabb, Eric D. Black, Badri Krishnan, Eugeniy E. Mikhailov, H. zur Mühlen, David Blair, Jordan Camp, Antony C. Searle, C. M. Mow-Lowry, S. Ballmer, James Whelan, P. Ajith, Frank Seifert, D. Hoyland, M. Araya, O. Spjeld, D. Coyne, T. Meier, J. Dalrymple, G. Newton, Shuichi Sato, Kirk McKenzie, Simon Chelkowski, T. Summerscales, L. Bogue, Joseph D. Romano, Morag M. Casey, M. Heurs, Kasem Mossavi, Patrick Brady, J. Greenhalgh, M. V. Plissi, Matthew Evans, Yi Pan, M. Varvella, A. C. Melissinos, Eric Howell, S. Saraf, M. Sung, Jong H. Chow, Hartmut Grote, T. D. Creighton, David Crooks, H. Ward, Peter King, S. Klimenko, N. Fotopoulos, Michael Landry, Maria Alessandra Papa, Evan Goetz, V. Mandic, N. A. Robertson, A. Bullington, K. Kawabe, Michael C. B. Ashley, John Veitch, Sascha Schediwy, Shuhei Yoshida, Peter Kalmus, M. MacInnis, R. S. Amin, Carlo Ungarelli, Peter H. Sneddon, B. Lantz, I. Wilmut, R. McCarthy, S. Vass, A. Ivanov, Daniel Sigg, Roger Jones, S. M. Aston, R. M. S. Schofield, Pablo Barriga, Benjamin J. Owen, N. A. Lockerbie, L. Zhang, Christopher Wipf, S. J. Waldman, Gianpietro Cagnoli, K. V. Tokmakov, A. Cumming, L. Goggin, C. A. Cantley, C. Robinson, Benjamin William Allen, Karsten Danzmann, Slawomir Gras, G. de Vine, A. M. Gretarsson, Martin Hewitson, Junwei Cao, E. Maros, R. Taylor, L. Ribichini, Brian O'Reilly, E. Messaritaki, Shantanu Desai, D. Grimmett, Sheila Rowan, Kip S. Thorne, V. P. Mitrofanov, Graham Woan, Robert L. Byer, Boris Hage, C. Cepeda, Stuart Reid, R. Ward, B. Rivera, P. J. Sutton, Ke Sun, Bernard F. Schutz, Li Ju, A. Weinstein, C. Hardham, Benno Willke, P. Shawhan, Suvadeep Bose, L. Ruet, Keisuke Goda, D. Webber, Alessandra Buonanno, Guido Mueller, H. Radkins, R. Burman, Erik Katsavounidis, Alberto Vecchio, D. Jackrel, T. Etzel, V. Parameshwaraiah, Vladimir B. Braginsky, H. Vahlbruch, K. Riles, B. C. Barish, Yousuke Itoh, D. Barker, Roman Schnabel, J. E. Brau, T. Evans, L. Cardenas, Subhasish Mitra, J. Markowitz, W. Wu, P. T. Beyersdorf, R.L. Coldwell, A. Grant, S. E. Whitcomb, B. Johnson, and The LIGO Scientific Collaboration

Subjects
Physics, Gravitational-wave observatory, 010308 nuclear & particles physics, Gravitational wave, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Astrophysics, 01 natural sciences, Gravitational-wave astronomy, LIGO, Cosmic string, Interferometry, General Relativity and Quantum Cosmology, Space and Planetary Science, Observatory, 0103 physical sciences, Astronomical interferometer, 010306 general physics, QC, QB
Abstract

The Laser Interferometer Gravitational-Wave Observatory (LIGO) has performed the fourth science run, S4, with significantly improved interferometer sensitivities with respect to previous runs. Using data acquired during this science run, we place a limit on the amplitude of a stochastic background of gravitational waves. For a frequency independent spectrum, the new Bayesian 90% upper limit is Ω_(GW) × [H_0/(72 km s^(−1) Mpc^(−1))]^2 < 6.5 × 10^(-5). This is currently the most sensitive result in the frequency range 51-150 Hz, with a factor of 13 improvement over the previous LIGO result. We discuss the complementarity of the new result with other constraints on a stochastic background of gravitational waves, and we investigate implications of the new result for different models of this background.

Published
2007

35. Search for gravitational waves from binary black hole inspirals in LIGO data

Author

Linqing Wen, T. Etzel, Joseph D. Romano, C. King, Kasem Mossavi, J. E. Brau, W. R. Johnston, Laura Cadonati, K. Kawabe, P. Csatorday, A. Chandler, Kevin M. Ryan, J. Betzwieser, D. Debra, W. Kells, Lindon J. Robison, A. Wilson, A. L. Stuver, J. S. Noel, M. Fyffe, O. Matherny, B. Lantz, Susan M. Scott, Teviet Creighton, Herbert Walther, Y. Hefetz, Gerhard Heinzel, C. Hardham, Helena Armandula, E. J. Elliffe, M. V. Plissi, Roman Schnabel, S. Penn, Karsten Kötter, Pamela J. Russell, S. Richman, B. Barr, H. Ward, Chad Hanna, A. Heptonstall, J. Worden, A. Rüdiger, K. Rawlins, Benno Willke, K. D. Zaleski, Oliver Jennrich, Subhasish Mitra, Marco G. Tarallo, X. Siemens, C. Wilkinson, J. Castiglione, D. Barker, K. A. Thorne, Adrian C. Ottewill, P. Charlton, Michael E Zucker, A. Di Credico, D. Churches, L. Ruet, Hartmut Grote, R. Riesen, D. Webber, B. F. Whiting, John Veitch, S. Roddy, Roland Schilling, M. Fine, E. J. Daw, S. Dhurandhar, Krzysztof Belczynski, R. Mittleman, Nelson Christensen, A. Hartunian, V. Quetschke, Bangalore Suryanarayana Sathyaprakash, D. Ugolini, Carsten Fallnich, Stefan Hild, M. A. Barton, I. A. Bilenko, V. Dergachev, Ian Taylor, David J. Ottaway, Alessandra Buonanno, E. Black, Martin M. Fejer, J. R. Smith, S. Klimenko, T. Nash, V. V. Frolov, M. MacInnis, S. Mukherjee, Sanichiro Yoshida, D. Sellers, A. M. Sintes, P. Aufmuth, Jeffrey A. Edlund, F. Nocera, Lee Samuel Finn, J. W C McNabb, D. Jungwirth, A. Sazonov, Manuel Luna, K. Reithmaier, A. Gillespie, Andreas Freise, A. Libson, Matthew Pitkin, A. Ivanov, M. Mageswaran, R. Wooley, R. Burgess, Daniel C. Woods, N. A. Robertson, Richard J. Abbott, I. Yakushin, P. E. Lindquist, H. Radkins, S. P. Vyachanin, M. Coles, M. Guenther, D. I. Robertson, C. Torres, Graham Woan, A. Rodriguez, Robert L. Byer, K. Y. Franzen, E. Maros, Stuart Reid, Curt Cutler, C. Gray, C. A. Cantley, T. Regimbau, Roy Williams, K. Wette, R. Coldwell, W. Tyler, T. Evans, Carlo Ungarelli, Michael D. Smith, Keisuke Goda, David Jones, Guenakh Mitselmakher, C. I. Torrie, C. Barker, V. Parameshwaraiah, K. S. Ganezer, Patrick Brady, Pankaj Sarin, D. Farnham, Raymond G. Beausoleil, A. Ageev, M. Hammond, C. Messenger, M. Lormand, O. Spjeld, R. Zhu, W. Hua, C. Robinson, Benjamin William Allen, K. Watts, B. Bland, V. Chickarmane, I. Zawischa, D. Sigg, W. W. Johnson, S. W. Ballmer, Stefan Goßler, R. Gustafson, Karsten Danzmann, M. C. Sumner, R. Balasubramanian, M. Rakhmanov, V. Schmidt, D. Chin, Stanislav Babak, Walid A. Majid, Erik Katsavounidis, Phil Willems, Gavin Davies, Duncan A. Brown, Walter Winkler, J. Kern, P. G. Murray, D. Steussy, B. Sears, Kevin M. Carter, J. A. Giaime, S. B. Anderson, Jan Harms, William E. Butler, Peter R. Saulson, M. Ito, Martin P McHugh, B. J. Cusack, Brent Ware, Bernard F. Schutz, Eileen S. Rotthoff, Vladimir B. Braginsky, Kevin C. Schlaufman, J. H. Hough, S. E. Seader, B. Bhawal, David B. Tanner, H. Ding, G. Mendell, M. W. Regehr, Marco Aurelio Diaz, M. Sung, S. Grunewald, K. Riles, M. H. P. M. van Putten, S. Tilav, L. Jones, Rana X. Adhikari, Gareth Jones, L. Sievers, Robert Bennett, Thomas Cokelaer, Peter H. Sneddon, G. Stapfer, Gregory M. Harry, Erika D'Ambrosio, Michele Zanolin, C. A. Shapiro, M. Pedraza, Vicky Kalogera, Robert Spero, Soumya D. Mohanty, Harald Lück, U. Weiland, S. R. Rao, M. Lei, T. Olson, M. Barnes, Julien Sylvestre, D. M. Strom, L. Wallace, S. J. Berukoff, R. Bork, N. Zotov, S. Seel, Lisa M. Goggin, K. Mason, R. Frey, A. Marin, C. Aulbert, Scott Koranda, C. Parameswariah, J. Langdale, Sandra E. Wiley, Gabriela Gonzalez, P. J. King, D. Grimmett, I. Leonor, Philip Nutzman, L. Matone, M. Ashley, D. Coyne, A. M. Gretarsson, D. Cook, A. Khan, J. Mason, Virginio Sannibale, David E. McClelland, G. Moreno, Guido Mueller, Yousuke Itoh, B. Bochner, Maria Alessandra Papa, Kent Blackburn, Herbert Welling, Massimo Tinto, Nergis Mavalvala, B. C. Barish, H. Yamamoto, A. Grant, J. Garofoli, Stephen Fairhurst, A. G. Wiseman, S. Wen, Lindy Blackburn, P. Ehrens, Chunglee Kim, V. Sandberg, Michele Vallisneri, A. Sibley, B. Machenschalk, S. Ray-Majumder, Seiji Kawamura, S. Márka, B. Rivera, Philippe Grandclément, K. T. Reilly, David H. Shoemaker, Shantanu Desai, Ik Siong Heng, F. Asiri, Kip S. Thorne, A. J. Weinstein, W. Wu, R. W.P. Drever, F. Mann, Peter Fritschel, Shinji Miyoki, Kenneth A. Strain, A. Weidner, R. A. Mercer, J. Heefner, B. O'Reilly, Reinhard Prix, V. P. Mitrofanov, P. J. Sutton, Haisheng Rong, K. C. Cannon, M. Lubinski, S. E. Whitcomb, M. C. Araya, B. Johnson, W. O. Hamilton, C. N. Colacino, K. Mailand, J. Chapsky, J. Hanson, Osamu Miyakawa, David H. Reitze, S. Killbourn, H. Overmier, James Whelan, Juri Agresti, A. Rizzi, G. Traylor, P. Ajith, L. Zhang, Thomas Corbitt, Christian J. Killow, Akiteru Takamori, Badri Krishnan, Antony C. Searle, T. Findley, S. Liu, D. Ouimette, Yi Chen, J. Cannizzo, J. Allen, D. Kozak, N. Hepler, M. Hennessy, Q. Z. Shu, R. L. Ward, M. Hrynevych, A. Bunkowski, T. Summerscales, Frank Seifert, Joseph M. Kovalik, S. Wise, E. Messaritaki, Sheila Rowan, J. H. Romie, K. Bayer, Michael Landry, S. Meshkov, Kenneth G. Libbrecht, F. J. Raab, S. Chelkowski, R. McCarthy, G. Billingsley, C. Vorvick, P. Schwinberg, J. D. E. Creighton, I. Salzman, R. Amin, W. G. Anderson, Peter Shawhan, M. Tibbits, B. P. Abbott, R. M. S. Schofield, S. Vass, J. Zweizig, Benjamin J. Owen, E. Myers, K. V. Tokmakov, D. Busby, Junwei Cao, R. L. Savage, S. Nagano, D. Redding, M. Malec, P. Hoang, Eugeniy E. Mikhailov, Alberto Vecchio, A. Lazzarini, Richard J. K. Taylor, Gianpietro Cagnoli, J. Myers, Shourov Chatterji, Suvadeep Bose, M. R. Smith, G. H. Sanders, R. Lawrence, M. Hewitson, Morag M. Casey, M. Heurs, B. J. Winjum, A. C. Melissinos, David Crooks, A. Bullington, L. Bogue, D. Rose, R. Desalvo, V. Re, Rainer Weiss, N. Hindman, J. G. Rollins, Jordan Camp, T. Delker, P. R. Williams, J. Dalrymple, A. S. Sengupta, H. Tariq, G. Newton, Matthew Evans, L. Cardenas, Vuk Mandic, Yi Pan, Eric K. Gustafson, T. T. Lyons, J. Logan, R. K. Nayak, R. Rahkola, R. J. Dupuis, and The LIGO Scientific Collaboration

Subjects
Physics, Nuclear and High Energy Physics, Gravitational-wave observatory, 010308 nuclear & particles physics, Gravitational wave, FOS: Physical sciences, Binary number, Astronomy, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, 01 natural sciences, Cosmology, LIGO, General Relativity and Quantum Cosmology, filters, Interferometry, Binary black hole, 0103 physical sciences, Astronomical interferometer, ddc:530, Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik, FILTERS, 010303 astronomy & astrophysics, QC
Abstract

We report on a search for gravitational waves from binary black hole inspirals in the data from the second science run of the LIGO interferometers. The search focused on binary systems with component masses between 3 and 20 solar masses. Optimally oriented binaries with distances up to 1 Mpc could be detected with efficiency of at least 90%. We found no events that could be identified as gravitational waves in the 385.6 hours of data that we searched., 18 pages, 8 figures

Published
2006

36. Design and construction of a prototype of a flat top beam interferometer and initial tests

Author

R. DeSalvo, Juri Agresti, N. Morgado, Erika D'Ambrosio, L. Pinard, B. Lagrange, D. Forest, Phil Willems, J M Mackowski, C. Michel, J.-L. Montorio, Marco G. Tarallo, B. Simoni, A. Remillieux, Laboratoire des matériaux avancés (LMA), Université Claude Bernard Lyon 1 (UCBL), and Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)

Subjects
Physics, History, 010308 nuclear & particles physics, business.industry, Curved mirror, 01 natural sciences, LIGO, Computer Science Applications, Education, law.invention, Interferometry, Optics, law, Optical cavity, 0103 physical sciences, Astronomical interferometer, Physics::Accelerator Physics, Laser beam quality, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, business, Beam (structure), Caltech Library Services, Gaussian beam
Abstract

A non-Gaussian, flat-top laser beam profile, also called Mesa Beam Profile, supported by non spherical mirrors known as Mexican Hat (MH) mirrors, has been proposed as a way to depress the mirror thermal noise and thus improve the sensitivity of future interferometric Gravitational Wave detectors, including Advanced LIGO [1]. Non-Gaussian beam configurations have never been tested before [2] hence the main motivation of this project is to demonstrate the feasibility of this new concept. A 7m rigid suspended Fabry-Perot (FP) cavity which can support a scaled version of a Mesa beam applicable to the LIGO interferometers has been developed. The FP cavity prototype is being designed to prove the feasibility of actual MH mirror profiles, determine whether a MH mirror cavity is capable of transforming an incoming Gaussian beam into a flat top beam profile, study the effects of unavoidable mirror imperfections on the resulting beam profile and gauge the difficulties associated with locking and maintaining the alignment of such an optical cavity. We present the design of the experimental apparatus and simulations comparing Gaussian and Mesa beams performed both with ideal and current (measured) mirror profiles. An overview of the technique used to manufacture this kind of mirror and initial results showing Mesa beam properties are presented.

Published
2006
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37. Joint LIGO and TAMA300 Search for Gravitational Waves from Inspiralling Neutron Star Binaries

Author

J. E. Brau, Subhasish Mitra, D. Churches, A. J. Weinstein, W. Wu, P. T. Beyersdorf, A. Grant, S. Liu, L. Zhang, Keisuke Goda, Erik Katsavounidis, Daisuke Tatsumi, A. Wilson, M. J. Lubinski, Vladimir B. Braginsky, K. Riles, Yousuke Itoh, Ken-ichi Nakao, A. Ageev, M. Lormand, M. Fine, K. Rawlins, A. Bunkowski, Kazuyuki Miura, J. Logan, R. K. Nayak, Rebecca Abbott, J. Heefner, Mayu Katsuki, David H. Shoemaker, R. Rahkola, Y. Hefetz, Shigemi Otsuka, Peter Fritschel, Gerhard Heinzel, C. Hardham, Hideki Ishitsuka, Hideki Asada, Jan Harms, Alberto Vecchio, Juri Agresti, A. Rizzi, S. Penn, Benno Willke, L. Ruet, Kazuaki Kuroda, Robert J. McCarthy, Linqing Wen, Pamela J. Russell, S. Richman, K. C. Cannon, A. Bullington, F. Mann, Shuichi Sato, Masaru Shibata, A. Gillespie, Oliver Jennrich, Akitoshi Ueda, L. Bogue, R. L. Savage, V. V. Frolov, Curt Cutler, Alessandra Buonanno, V. Parameshwaraiah, I. Leonor, John K. Cannizzo, T. Summerscales, S. Nagano, Yusaku Hamuro, Darby Kozak, K. A. Thorne, J. Betzwieser, M. C. Araya, D. Ugolini, Mitsuru Musha, Y. Saito, Carsten Fallnich, Yoshikazu Karasawa, R. J. Dupuis, Kiminori Kondo, C. Torres, A. Rodriguez, C. Barker, B. Johnson, Naoki Seto, D. Redding, Youhei Sato, Joseph D. Romano, C. King, Stefan Hild, N. Sato, C. A. Cantley, C. Robinson, Benjamin William Allen, Karsten Danzmann, M. C. Sumner, Shoken M. Miyama, D. Chin, Stanislav Babak, Kasem Mossavi, Walid A. Majid, Duncan A. Brown, P. Hoang, G. Traylor, Thomas Corbitt, Michael Landry, G. Billingsley, Michele Vallisneri, Ik Siong Heng, Fumiko Kawazoe, H. Tariq, Shigenori Moriwaki, J. Chapsky, S. Meshkov, Akiteru Takamori, Pankaj Sarin, D. Farnham, Akito Araya, E. J. Daw, Brent Ware, Y. Ogawa, Norikatsu Mio, G. Mendell, Soma Mukherjee, Sanichiro Yoshida, M. R. Smith, Shinji Miyoki, Graham Woan, Zong Hong Zhu, Robert L. Byer, Stuart Reid, Shihori Sakata, A. M. Gretarsson, D. Rose, C. A. Shapiro, V. Schmidt, Toru Tanji, T. Nakamura, E. Rotthoff, P. Csatorday, William E. Butler, Eugeniy E. Mikhailov, T. Findley, E. Messaritaki, Morag M. Casey, M. Heurs, D. Ouimette, C. Gray, Erika D'Ambrosio, A. Chandler, B. J. Winjum, C. Parameswariah, M. Rakhmanov, Vuk Mandic, Bernard F. Schutz, H. Yamamoto, Takaharu Kaneyama, J. W C McNabb, Laura Cadonati, Walter Winkler, Sheila Rowan, Harald Lück, G. Stapfer, Kevin M. Ryan, J. Hanson, Yoshitaka Nagayama, J. Langdale, G. P. Newton, M. Fyffe, N. A. Robertson, Ken-ichi Ueda, Sandra E. Wiley, Gabriela Gonzalez, Ken'ichi Nakagawa, Martin P McHugh, V. Re, Susan M. Scott, G. H. Sanders, R. Lawrence, M. H. P. M. van Putten, Koichi Waseda, C. Aulbert, S. Tilav, Guido Mueller, Rana X. Adhikari, Gareth Jones, H. Overmier, Roy Williams, J. A. Giaime, Katsuaki Kasahara, Eric K. Gustafson, Hideo Iguchi, Kentaro Somiya, Kenji Soida, B. Machenschalk, P. R. Williams, Takashi Kuwabara, Richard J. K. Taylor, S. Wise, D. Sellers, Teviet Creighton, S. Grunewald, Herbert Walther, Chad Hanna, K. Kötter, C. Wilkinson, Gianpietro Cagnoli, Toshikazu Suzuki, Rainer Weiss, T. Etzel, A. C. Melissinos, K. Oohara, T. T. Lyons, E. Maros, M. V. Plissi, M. Kawamura, Shantanu Desai, Kip S. Thorne, B. Lantz, K. S. Ganezer, Kouichi Sato, Albert Lazzarini, M. Coles, M. Guenther, Tomiyoshi Haruyama, R. W. P. Drever, Kenji Numata, Masaki Ando, K. Watts, Kenneth G. Libbrecht, I. Salzman, Stefan Goßler, Michael D. Smith, Marco G. Tarallo, K. T. Reilly, W. W. Johnson, J. Myers, F. Nocera, J. Allen, N. Hepler, Ryuichi Fujita, W. O. Hamilton, Scott Koranda, D. Webber, V. P. Mitrofanov, R. M. S. Schofield, C. Vorvick, A. Marin, Yoshio Nishi, Shuzo Takemoto, B. Bochner, Akira Okutomi, Hideaki Kudoh, Benjamin J. Owen, P. Schwinberg, V. Quetschke, Shourov Chatterji, W. R. Johnston, Yoshihide Kozai, Bangalore Suryanarayana Sathyaprakash, E. Black, Norihiko Kamikubota, Patrick Brady, Suvadeep Bose, Takayuki Tomaru, Masatake Ohashi, Kevin C. Schlaufman, E. Myers, K. V. Tokmakov, S. Killbourn, Carlo Ungarelli, Martin M. Fejer, Hideyuki Tagoshi, J. R. Smith, R. Bork, T. Regimbau, Toshifumi Futamase, C. I. Torrie, Herbert Welling, A. Heptonstall, M. Malec, T. Nash, W. G. Anderson, Peter Shawhan, M. Tibbits, B. P. Abbott, A. Sazonov, Seiji Kawamura, Nobuyuki Kanda, Hartmut Grote, James Whelan, P. Ajith, L. Matone, Yukiyoshi Iida, Martin Hewitson, Massimo Tinto, Nergis Mavalvala, J. G. Rollins, Junwei Cao, Reinhard Prix, Naoko Ohishi, B. C. Barish, K. D. Zaleski, Phil Willems, M. Hrynevych, R. DeSalvo, S. Vass, W. Kells, P. Ehrens, D. Busby, D. M. Strom, Masa-Katsu Fujimoto, Kevin M. Carter, T. Delker, P. G. Murray, Osamu Miyakawa, David H. Reitze, Christian J. Killow, S. B. Anderson, Hiroyuki Nakano, Misao Sasaki, Jordan Camp, A. Sibley, J. Dalrymple, Masao Tokunari, Lindon J. Robison, A. S. Sengupta, J. H. Hough, D. Jungwirth, Philippe Grandclément, P. E. Lindquist, K. Wette, Peter Aufmuth, David B. Tanner, M. W. Regehr, Lisa M. Goggin, Douglas R. Cook, M. Sung, P. J. Sutton, Haisheng Rong, Timothy Evans, Helena Armandula, E. J. Elliffe, Kazuhiro Hayama, M. Pedraza, Michele Zanolin, S. Seel, R. Coldwell, Jeffrey A. Edlund, M. A. Barton, D. Sigg, Keiko Kokeyama, Gavin Davies, D. Steussy, Koji Arai, R. Burgess, Maria Alessandra Papa, V. Chickarmane, Daniel C. Woods, B. Sears, Kimio Tsubono, T. Akutsu, S. W. Ballmer, Kent Blackburn, S. Wen, D. I. Robertson, Vicky Kalogera, Souichi Telada, J. Mason, B. Bhawal, D.B. DeBra, S. J. Berukoff, K. Y. Franzen, M. Hammond, J. Kern, Hisa-aki Shinkai, L. Jones, Robert Bennett, A. Yamamoto, Matthew Evans, L. Cardenas, Yi Pan, S. Klimenko, Ryutaro Takahashi, Y. Tsunesada, G. Moreno, Robert Spero, Soumya D. Mohanty, David Crooks, N. Zotov, K. Mason, Sanjeev Dhurandhar, S. Ray-Majumder, Xavier Siemens, C. N. Colacino, Yi Chen, M. Hennessy, Q. Z. Shu, R. L. Ward, M. Ito, J. H. Romie, K. Bayer, F. J. Raab, R. Gustafson, S. Márka, Takakazu Shintomi, J. Zweizig, Kohei Takeno, B. Bland, U. Weiland, Takahiro Tanaka, Kenneth A. Strain, S. E. Seader, A. Weidner, R. A. Mercer, Michael E Zucker, Stephen Fairhurst, Tatsuru Yoshida, A. L. Stuver, O. Matherny, Manuel Luna, B. O'Reilly, J. S. Noel, B. Barr, Hiromi Mizusawa, J. Worden, A. Rüdiger, Namio Matsuda, J. Castiglione, Youhei Fujiki, P. Charlton, R. Riesen, A. Di Credico, Roland Schilling, I. A. Bilenko, V. Dergachev, Ian Taylor, David J. Ottaway, Marco Aurelio Diaz, Nobuhiro Tsuda, David Jones, Peter R. Saulson, Taketoshi Kasai, F. Asiri, Badri Krishnan, H. Ding, Takashi Uchiyama, Antony C. Searle, Kunihito Ioka, Frank Seifert, B. F. Whiting, Joseph M. Kovalik, S. E. Whitcomb, I. Yakushin, Hirotaka Takahashi, Keisuke Taniguchi, B. J. Cusack, Guenakh Mitselmakher, S. R. Rao, O. Spjeld, R. Zhu, Toshitaka Yamazaki, M. Ashley, Mitsuhiro Fukushima, L. Sievers, Jolien D. E. Creighton, Thomas Cokelaer, Lindy Blackburn, Yuriko Yanagi, Chunglee Kim, V. Sandberg, D. Barker, A. Ivanov, H. Radkins, S. P. Vyachanin, S. Chelkowski, W. Tyler, S. Roddy, Raymond G. Beausoleil, R. Balasubramanian, A. M. Sintes, Lee Samuel Finn, M. Barnes, Julien Sylvestre, Yoichi Aso, L. Wallace, R. Frey, P. J. King, D. Grimmett, Philip Nutzman, A. G. Wiseman, D. C. Coyne, K. Reithmaier, Andreas Freise, A. Libson, Matthew Pitkin, R. Wooley, I. Zawischa, Peter H. Sneddon, Yasufumi Kojima, J. Garofoli, K. Kawabe, B. Rivera, M. Mageswaran, H. Ward, John Veitch, Jun'ichi Yokoyama, M. MacInnis, R. S. Amin, Kazuhiro Yamamoto, N. Hindman, Gregory M. Harry, M. Lei, T. Olson, A. Khan, Virginio Sannibale, David E. McClelland, C. Messenger, W. Hua, Aya Sekido, Adrian C. Ottewill, K. Mailand, Krzysztof Belczynski, R. Mittleman, Nelson Christensen, A. Hartunian, Roman Schnabel, The LIGO Scientific Collaboration, and TAMA Collaboration

Subjects
Nuclear and High Energy Physics, templates, Milky Way, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, 01 natural sciences, coalescence rates, neutron stars, Cosmology, General Relativity and Quantum Cosmology, binary stars, gravitational wave detectors, 0103 physical sciences, Binary star, ddc:530, compact binaries, 010306 general physics, QC, Astrophysics::Galaxy Astrophysics, Physics, 010308 nuclear & particles physics, Gravitational wave, Astronomy, LIGO, Galaxy, Neutron star, Stars, gravitational waves, light interferometry, Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik
Abstract

We search for coincident gravitational wave signals from inspiralling neutron star binaries using LIGO and TAMA300 data taken during early 2003. Using a simple trigger exchange method, we perform an inter-collaboration coincidence search during times when TAMA300 and only one of the LIGO sites were operational. We find no evidence of any gravitational wave signals. We place an observational upper limit on the rate of binary neutron star coalescence with component masses between 1 and 3 M_sun of 49 per year per Milky Way equivalent galaxy at a 90% confidence level. The methods developed during this search will find application in future network inspiral analyses., 9 pages, 5 figures. Updated with published version

Published
2005

38. Flat top beam profile cavity prototype

Author

Juri Agresti, Erika D'Ambrosio, R. DeSalvo, Marco G. Tarallo, B. Simoni, A. Remillieux, J M Mackowski, and Phil Willems

Subjects
Physics, Interferometry, Optics, business.industry, Gravitational wave, Detector, Astronomical interferometer, Thermal fluctuations, Curved mirror, business, Beam (structure), Gaussian beam
Abstract

Mirror thermal noise is one of the fundamental factors limiting the sensitivity of gravitational wave interferometric detectors. Classical Gaussian beams "interrogate" only a small fraction of the mirror surface, and therefore are not well suited to average out fluctuations and minimize the thermal noise. It has been calculated that flat beam profiles would be better suited to average over thermal fluctuations and would allow sensitivity improvements that would more than double the "reach" of GW interferometric detectors. Non-spherical mirrors, shaped to support flat beam profile beams, have been designed and fabricated. A dedicated interferometer has been built to test the performance of these mirrors. We report on the status of this development.

Published
2005
Full Text
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39. Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts

Author

H. Ward, A. Chandler, Kevin M. Ryan, T. Regimbau, Ken'ichi Nakagawa, C. I. Torrie, John Veitch, A. Heptonstall, M. Malec, Jordan Camp, J. Dalrymple, M. Ashley, A. S. Sengupta, Norikatsu Mio, Shinji Miyoki, Jun'ichi Yokoyama, J. Allen, N. Hepler, Akira Okutomi, Phil Willems, D. M. Strom, A. Yamamoto, Jolien D. E. Creighton, Lindy Blackburn, Matthew Evans, L. Cardenas, Yi Pan, Takashi Kuwabara, Richard J. K. Taylor, Gianpietro Cagnoli, Shihori Sakata, C. Aulbert, M. MacInnis, Keita Kawabe, R. S. Amin, Chunglee Kim, Seiji Kawamura, Hiroyuki Nakano, Reinhard Prix, Juri Agresti, A. Rizzi, V. Sandberg, K. Rawlins, A. Bunkowski, Shuzo Takemoto, S. Klimenko, Ryutaro Takahashi, W. R. Johnston, Masa-Katsu Fujimoto, Osamu Miyakawa, David H. Reitze, Christian J. Killow, G. Mendell, J. Myers, Shourov Chatterji, Lindon J. Robison, Helena Armandula, E. J. Elliffe, Suvadeep Bose, A. Ageev, Daisuke Tatsumi, A. Wilson, Kazuyuki Miura, Roy Williams, Kenji Soida, K. S. Ganezer, J. S. Noel, Hiromi Mizusawa, Namio Matsuda, J. Castiglione, Lisa M. Goggin, D. Rose, Hideki Asada, Jan Harms, K. Watts, T. Summerscales, Michael Landry, Roman Schnabel, C. A. Shapiro, Masaru Shibata, Stefan Goßler, K. T. Reilly, Toru Tanji, T. Nakamura, B. F. Whiting, David H. Shoemaker, V. Re, Y. Ogawa, Norihiko Kamikubota, Y. Hefetz, Gerhard Heinzel, C. Hardham, M. R. Smith, Masatake Ohashi, H. Overmier, Robert J. McCarthy, Linqing Wen, Shuichi Sato, Joseph D. Romano, C. King, Shoken M. Miyama, Kasem Mossavi, P. Charlton, A. Di Credico, I. A. Bilenko, V. Dergachev, Ian Taylor, David J. Ottaway, Laura Cadonati, G. Billingsley, D. Sellers, Amber Stuver, Sanichiro Yoshida, A. Ivanov, Y. Saito, J. E. Brau, Subhasish Mitra, D. Churches, P. G. Murray, J. H. Hough, C. Parameswariah, J. Langdale, G. P. Newton, M. Fyffe, Sandra E. Wiley, Gabriela Gonzalez, M. Hrynevych, Peter H. Sneddon, Graham Woan, Zong Hong Zhu, Robert L. Byer, Stuart Reid, Kevin C. Schlaufman, Scott Koranda, Akitoshi Ueda, A. Gillespie, Susan M. Scott, Teviet Creighton, Herbert Welling, F. Mann, Rainer Weiss, Kiminori Kondo, Herbert Walther, Benno Willke, R. W. P. Drever, Nergis Mavalvala, H. Radkins, R. L. Savage, L. Ruet, S. P. Vyachanin, M. Coles, L. Matone, M. Guenther, Yasufumi Kojima, E. Rotthoff, Misao Sasaki, Naoko Ohishi, B. C. Barish, Takaharu Kaneyama, M. Rakhmanov, Michael D. Smith, Bernard F. Schutz, Chad Hanna, G. Stapfer, J. Hanson, C. Torres, A. Rodriguez, S. Meshkov, C. Barker, X. Siemens, K. Kötter, Douglas R. Cook, Michael E Zucker, W. Tyler, Michele Zanolin, S. Seel, C. Wilkinson, G. H. Sanders, R. Lawrence, Mitsuru Musha, W. W. Johnson, B. Johnson, S. Nagano, R. L. Ward, K. D. Zaleski, D. Redding, J. Garofoli, Alessandra Buonanno, R. DeSalvo, Patrick Brady, C. A. Cantley, A. Sibley, Raymond G. Beausoleil, R. Balasubramanian, Ryuichi Fujita, I. Leonor, John K. Cannizzo, C. Robinson, Benjamin William Allen, Alberto Vecchio, M. A. Barton, Rana X. Adhikari, Yoshitaka Nagayama, Guido Mueller, Gareth Jones, B. Machenschalk, R. Rahkola, Pankaj Sarin, Karsten Danzmann, M. C. Sumner, B. Lantz, J. Chapsky, H. Yamamoto, Hideo Iguchi, Tatsuru Yoshida, P. Hoang, Manuel Luna, J. H. Romie, K. Bayer, F. Nocera, F. J. Raab, D.B. DeBra, T. Etzel, K. Y. Franzen, Keisuke Goda, Gavin Davies, Marco G. Tarallo, I. Salzman, D. Farnham, D. Steussy, B. Sears, Akito Araya, V. Schmidt, R. M. S. Schofield, David Jones, Hideaki Kudoh, Benjamin J. Owen, A. M. Gretarsson, Tomiyoshi Haruyama, W. O. Hamilton, R. Gustafson, Erik Katsavounidis, Eugeniy E. Mikhailov, B. J. Cusack, M. Hammond, Kimio Tsubono, Vicky Kalogera, J. Kern, Jeffrey A. Edlund, E. J. Daw, M. J. Lubinski, William E. Butler, D. B. Kozak, E. Myers, K. V. Tokmakov, Takayuki Tomaru, E. Messaritaki, S. Killbourn, Martin Hewitson, Koji Arai, R. Burgess, Daniel C. Woods, B. Rivera, D. Webber, Peter R. Saulson, Hisa-aki Shinkai, L. Jones, M. Lormand, H. Ding, R. Abbott, M. Fine, V. Quetschke, Sheila Rowan, James Whelan, P. Ajith, C. Vorvick, Takashi Uchiyama, Kunihito Ioka, M. Mageswaran, Peter Fritschel, S. Penn, Masao Tokunari, Vladimir B. Braginsky, K. Reithmaier, Andreas Freise, S. R. Rao, Robert Bennett, A. Libson, Marco Aurelio Diaz, D. I. Robertson, Erika D'Ambrosio, Pamela J. Russell, Souichi Telada, Junwei Cao, K. Riles, Martin P McHugh, M. H. P. M. van Putten, S. Tilav, Matthew Pitkin, J. Heefner, Toshitaka Yamazaki, Mayu Katsuki, P. Schwinberg, Yoshihide Kozai, Bangalore Suryanarayana Sathyaprakash, E. Black, Martin M. Fejer, Hideyuki Tagoshi, J. R. Smith, R. Bork, T. Nash, K. C. Cannon, J. Zweizig, R. Wooley, Kazuhiro Hayama, A. Sazonov, J. Mason, Ken-ichi Nakao, W. G. Anderson, K. Oohara, E. Maros, Peter Shawhan, S. Richman, M. Tibbits, B. P. Abbott, Yousuke Itoh, Oliver Jennrich, K. A. Thorne, J. Betzwieser, Kazuaki Kuroda, Koichi Waseda, N. Sato, M. Kawamura, S. Wen, A. Bullington, Michele Vallisneri, I. Zawischa, Robert Spero, Soumya D. Mohanty, Fumiko Kawazoe, D. Ugolini, Carsten Fallnich, Stefan Hild, S. Vass, L. Bogue, A. J. Weinstein, Ik Siong Heng, Shantanu Desai, J. W C McNabb, W. Wu, P. T. Beyersdorf, N. Zotov, W. Kells, Soma Mukherjee, Taketoshi Kasai, K. Mason, Sanjeev Dhurandhar, Kip S. Thorne, Badri Krishnan, Shigemi Otsuka, S. Ray-Majumder, D. Busby, Curt Cutler, T. Findley, C. Gray, Kentaro Somiya, Naoki Seto, D. Ouimette, M. C. Araya, Antony C. Searle, V. V. Frolov, Kevin M. Carter, Frank Seifert, C. N. Colacino, S. B. Anderson, A. Grant, S. Liu, V. Parameshwaraiah, L. Zhang, V. P. Mitrofanov, G. Traylor, Kenji Numata, Masaki Ando, Thomas Corbitt, Akiteru Takamori, Yusaku Hamuro, Joseph M. Kovalik, D. Chin, Stanislav Babak, Walid A. Majid, Yi Chen, M. Hennessy, Q. Z. Shu, David B. Tanner, M. W. Regehr, M. Sung, Duncan A. Brown, S. Wise, S. Grunewald, Brent Ware, Kouichi Sato, M. Pedraza, Maria Alessandra Papa, T. Akutsu, Kenneth G. Libbrecht, Kent Blackburn, N. A. Robertson, Carlo Ungarelli, Walter Winkler, Morag M. Casey, Harald Lück, P. R. Williams, M. Heurs, Toshikazu Suzuki, B. J. Winjum, A. Marin, Yoshio Nishi, A. C. Melissinos, B. Bochner, Massimo Tinto, David Crooks, Philippe Grandclément, P. J. Sutton, Haisheng Rong, Kazuhiro Yamamoto, N. Hindman, Toshifumi Futamase, P. Ehrens, K. Wette, Timothy Evans, R. Coldwell, D. Sigg, S. W. Ballmer, Y. Tsunesada, G. Moreno, J. Logan, R. K. Nayak, Yoshikazu Karasawa, R. J. Dupuis, Youhei Sato, H. Tariq, Shigenori Moriwaki, Vuk Mandic, Ken-ichi Ueda, J. A. Giaime, Katsuaki Kasahara, Eric K. Gustafson, T. T. Lyons, Albert Lazzarini, J. G. Rollins, T. Delker, F. Asiri, S. E. Whitcomb, Adrian C. Ottewill, K. Mailand, Krzysztof Belczynski, R. Mittleman, Kohei Takeno, B. Bland, Nelson Christensen, U. Weiland, Takahiro Tanaka, S. E. Seader, A. Hartunian, Stephen Fairhurst, O. Matherny, B. Barr, J. Worden, A. Rüdiger, Youhei Fujiki, R. Riesen, Roland Schilling, Nobuhiro Tsuda, Gregory M. Harry, M. Lei, I. Yakushin, Hirotaka Takahashi, T. Olson, Keisuke Taniguchi, Guenakh Mitselmakher, A. Khan, Virginio Sannibale, David E. McClelland, O. Spjeld, R. Zhu, Mitsuhiro Fukushima, C. Messenger, W. Hua, L. Sievers, Thomas Cokelaer, Yuriko Yanagi, Aya Sekido, Hideki Ishizuka, D. Barker, S. Chelkowski, S. Roddy, A. M. Sintes, Lee Samuel Finn, M. Barnes, Julien Sylvestre, Yoichi Aso, L. Wallace, R. Frey, S. Márka, Takakazu Shintomi, P. J. King, D. Grimmett, Philip Nutzman, Kenneth A. Strain, A. G. Wiseman, D. C. Coyne, A. Weidner, R. A. Mercer, B. O'Reilly, P. Csatorday, M. V. Plissi, Nobuyuki Kanda, Hartmut Grote, Yukiyoshi Iida, D. Jungwirth, P. E. Lindquist, Peter Aufmuth, V. Chickarmane, B. Bhawal, S. J. Berukoff, Keiko Kokeyama, M. Ito, The LIGO Scientific Collaboration, and TAMA Collaboration

Subjects
Nuclear and High Energy Physics, noise, Frequency band, FOS: Physical sciences, Astrophysics, General Relativity and Quantum Cosmology (gr-qc), 01 natural sciences, General Relativity and Quantum Cosmology, Coincidence, gravitational wave detectors, Coincident, 0103 physical sciences, black-hole coalescences, ddc:530, 010303 astronomy & astrophysics, QC, Physics, 010308 nuclear & particles physics, Gravitational wave, Bandwidth (signal processing), Detector, LIGO, Amplitude, gravitational waves, light interferometry, network, Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik
Abstract

We report on the first joint search for gravitational waves by the TAMA and LIGO collaborations. We looked for millisecond-duration unmodelled gravitational-wave bursts in 473 hr of coincident data collected during early 2003. No candidate signals were found. We set an upper limit of 0.12 events per day on the rate of detectable gravitational-wave bursts, at 90% confidence level. From simulations, we estimate that our detector network was sensitive to bursts with root-sum-square strain amplitude above approximately 1-3x10^{-19} Hz^{-1/2} in the frequency band 700-2000 Hz. We describe the details of this collaborative search, with particular emphasis on its advantages and disadvantages compared to searches by LIGO and TAMA separately using the same data. Benefits include a lower background and longer observation time, at some cost in sensitivity and bandwidth. We also demonstrate techniques for performing coincidence searches with a heterogeneous network of detectors with different noise spectra and orientations. These techniques include using coordinated signal injections to estimate the network sensitivity, and tuning the analysis to maximize the sensitivity and the livetime, subject to constraints on the background., Comment: 15 pages, 11 figures, to be submitted to Phys Rev D. Updated author list

Published
2005

40. Astrophysically triggered searches for gravitational waves: status and prospects

Author

H. Ward, Benno Willke, J. Clark, L. Ruet, H. Lin, C. Palomba, Alessandra Buonanno, I. Leonor, John K. Cannizzo, I. Duke, Alessandra Corsi, L. Baggio, John Veitch, Sascha Schediwy, M. MacInnis, P. Rapagnani, R. S. Amin, E. Chalkley, Rainer Weiss, F. Ricci, R. W. P. Drever, W. W. Johnson, A. L. Stuver, K. Flasch, F. Carbognani, S. Giampanis, Antonio Lucianetti, Patrice Hello, J. Ulmen, R. L. Ward, T. Casebolt, P. J. Sutton, J. H. Romie, K. Bayer, L. Cunningham, F. J. Raab, S. Saraf, R. Gustafson, Roman Schnabel, J. E. Brau, Subhasish Mitra, Efim A. Khazanov, G. Ballardin, H. R. Williams, M. M. Lang, M. Degree, K. Mailand, R. Mittleman, Andreas Freise, Matthew Pitkin, R. Wooley, T. Hayler, S. Kamat, A. Giazotto, P. Shawhan, I. Ferrante, David Blair, T. Regimbau, A. Heptonstall, D. R. Ingram, Phil Willems, K. D. Giardina, Nick Leindecker, J. Zweizig, Saverio Avino, A. Ivanov, H. Radkins, S. P. Vyachanin, M. Brinkmann, W. Tyler, Nelson Christensen, D. Barker, N. Morgado, P. G. Murray, G. McIvor, Alberto Vecchio, N. D. Smith, Fausto Acernese, C. Gray, M. Mantovani, E. Myers, D. M. Strom, Kirk McKenzie, S. Roddy, P. Charlton, J. H. Hough, S. Kreckelbergh, Kentaro Somiya, I. A. Bilenko, V. Dergachev, David J. Ottaway, Robert Stone, A. Di Virgilio, Lisa M. Goggin, D. Huet, S. Braccini, I. Wilmut, F. Kawazoe, J. Garofoli, J. S. Kissel, Roger Jones, Kenji Numata, T. Petrie, A. M. Sintes, Lee Samuel Finn, K. Kawabe, R. Gouaty, B. Lantz, Elena Cesarini, Martin P McHugh, B. J. J. Slagmolen, B. Sorazu, A. Thüring, D. S. Rabeling, S. M. Aston, B. Rivera, Pablo Barriga, M. Mageswaran, J. S. Miller, A. C. Melissinos, Douglas R. Cook, Michele Zanolin, Rocco Romano, S. Penn, Pamela J. Russell, R. A. Mercer, T. Z. Summerscales, S. Márka, Roger K. Route, V. Dattilo, K. A. Thorne, R. M. S. Schofield, Benjamin J. Owen, J. F. J. van den Brand, Seiji Kawamura, Reinhard Prix, A. Effler, Elizabeth Harstad, M. Laval, V. Kalogera, Stefan Hild, Kenneth A. Strain, E. Maros, Jesper Munch, M. Rakhmanov, A. Brillet, Christopher Wipf, K. V. Tokmakov, Martin Hewitson, Junwei Cao, Ettore Majorana, Fabio Marchesoni, F. Menzinger, A. Remillieux, Osamu Miyakawa, David H. Reitze, M. R. Smith, K. L. Dooley, R. De Rosa, A. S. Sengupta, P. Ehrens, Lisa Barsotti, B. O'Reilly, F. Travasso, Alessandra Toncelli, Carlos Cepeda, Robert J. McCarthy, S. Bigotta, I. Kozhevatov, Yi Pan, Anna Dari, A. Rocchi, Hirotaka Takahashi, Soumya D. Mohanty, Keisuke Goda, A. Perreca, Guenakh Mitselmakher, P. Amico, R. J. S. Greenhalgh, Shuichi Sato, P. La Penna, N. Zotov, Erik Katsavounidis, M. J. Lubinski, Gavin Davies, Maria Ilaria Del Principe, D. Lodhia, John G. Dwyer, Vladimir B. Braginsky, K. Mason, B. Sears, Sanjeev Dhurandhar, V. Boschi, Joseph D. Romano, H. Vahlbruch, K. Riles, J. Y. Vinet, M. Tonelli, E. Espinoza, M. Weinert, R. M. Martin, F. Fidecaro, Kasem Mossavi, G. M. Guidi, Igor Neri, Innocenzo M. Pinto, F. Grimaldi, Xavier Siemens, Yaohui Fan, Thomas Cokelaer, A. Viceré, Jonah Kanner, K. Wette, Yi Chen, J. C. Dumas, M. Hennessy, Timothy Evans, Albert Lazzarini, Tom Fricke, D. Sigg, P. Sarin, S. W. Ballmer, M. Bastarrika, R. M. Cutler, A. Spallicci, A. Rodriguez, David Jones, C. Barker, G. Moreno, K. Kokeyama, F. Garufi, Peter R. Saulson, C. N. Man, V. Leonhardt, F. Cleva, Peter Fritschel, R. Terenzi, H. J. Pletsch, Enrico Calloni, G. Traylor, Thomas Corbitt, A. J. Weinstein, I. Gholami, W. Wu, R. Abbott, P. T. Beyersdorf, M. V. van der Sluys, D. J. Hosken, E. Coccia, L. Di Fiore, J. Betzwieser, J. G. Rollins, H. Overmier, Chonghoon Kim, A. Grant, Leo C. Stein, D. Sellers, Gianpietro Cagnoli, S. Birindelli, Badri Krishnan, L. Zhang, Simon Chelkowski, E. Hirose, V. Fafone, F. Vetrano, M. Guenther, Antony C. Searle, C. M. Mow-Lowry, J. Myers, N. Fotopoulos, Shourov Chatterji, A. Di Lieto, D. Fazi, S. J. Waldman, Suvadeep Bose, Patrick Brady, B. F. Whiting, Z. Márka, H. Müller-Ebhardt, A. Cumming, M. Lorenzini, C. Van Den Broeck, V. V. Frolov, Kevin M. Ryan, E. Genin, Michael E Zucker, V. Kondrashov, M. Barsuglia, Michael Landry, L. Giordano, J. Minelli, R. DeSalvo, V. Parameshwaraiah, Chunnong Zhao, Kipp Cannon, A. M. Gretarsson, David H. Shoemaker, Y. Minenkov, R. S. Ottens, R. J. Dupuis, F. Martelli, D. Verkindt, E. E. Doomes, Giulia Pagliaroli, C. Echols, G. Billingsley, Ravi Kumar Kopparapu, E. Chassande-Mottin, Peter Aufmuth, P. Puppo, P. Lu, O. Burmeister, L. Bosi, Sheila Rowan, Marco Aurelio Diaz, R. Taylor, L. Sancho De La Jordana, M. Alshourbagy, Jolien D. E. Creighton, J. N. Marx, Laura Cadonati, T. P. Bodiya, Supriyo Sinha, B. Johnson, D. Kasprzyk, Stanislav Babak, Sanichiro Yoshida, S. Mosca, M. Samidi, François Bondu, H. Rehbein, Vuk Mandic, S. B. Anderson, Ruslan Vaulin, David B. Tanner, Susan M. Scott, Th. S. Bauer, J. Dickson, C. I. Torrie, Jan Harms, M. Sung, Lindy Blackburn, Duncan A. Brown, Helena Armandula, M. Pedraza, J. A. Giaime, Maria Alessandra Papa, Rosa Poggiani, F. Cavalier, J. O'Dell, Ke-Xun Sun, V. Sandberg, F. Antonucci, Kent Blackburn, N. Rainer, N. A. Robertson, Chad Hanna, Graham Woan, Evan Goetz, D. Hammer, V. Granata, F. Seifert, Malcolm B. Gray, D. Buskulic, Silvio Pardi, E. Cuoco, C. Wilkinson, Sofiane Aoudia, Peter Kalmus, I. Ricciardi, Robert L. Byer, B. Lopez, Stuart Reid, Rana X. Adhikari, Gareth Jones, S. Meshkov, G. S. Allen, B. Machenschalk, Guido Russo, F. Donovan, Francesco Cottone, L. Pinard, G. Vajente, S. Van Der Putten, Bernard F. Schutz, Li Ju, A. Pasqualetti, Shantanu Desai, T. Etzel, F. Nocera, Salvatore Solimeno, Kip S. Thorne, J. Hanson, J. Thacker, B. L. Swinkels, M. Ramsunder, C. Greverie, A. E. Villar, Soma Mukherjee, Guido Mueller, Drew Keppel, Marie-Anne Bizouard, Christian Corda, Zewu Yan, D. Hoak, M. V. Plissi, Nergis Mavalvala, Marco G. Tarallo, Jerome Degallaix, Hartmut Grote, G. Losurdo, B. C. Barish, J. Slutsky, P. E. Lindquist, V. Quetschke, A. Stochino, J. Heefner, R. Grosso, V. P. Mitrofanov, Bangalore Suryanarayana Sathyaprakash, E. Black, Walter Winkler, Martin M. Fejer, A. S. Markosyan, J. R. Smith, R. Bork, T. Nash, J.-M. Mackowski, Harald Lück, G. H. Ogin, C. Bradaschia, H. Heitmann, Boris Hage, Ik Siong Heng, Emma L. Robinson, H. Mukhopadhyay, S. C. McGuire, D. J. A. McKechan, John Nelson, P. Astone, J. Marque, John S. Markowitz, G. Mendell, Richard A. Matzner, D. Ugolini, Karel E. Urbanek, F. Frasconi, G. P. Newton, M. Fyffe, Gabriela Gonzalez, J. M. Hallam, R. Flaminio, H. Yamamoto, M. Lormand, H. Fehrmann, A. C. Clapson, B. Moe, R. Passaquieti, C. Robinson, Benjamin William Allen, Karsten Danzmann, N. A. Lockerbie, C. Moins, M. Punturo, M. C. Araya, Leopoldo Milano, Slawomir Gras, P. Savov, James Whelan, A. Bullington, P. Ajith, Rahul Biswas, V. Brisson, L. Bogue, F. Piergiovanni, M. Davier, A. F. Brooks, D. Passuello, M. Yvert, S. Grunewald, Yoichi Aso, L. Wallace, R. Frey, C. Messenger, I. Yakushin, N. Letendre, C. Aulbert, R. Cavalieri, P. J. King, F. Marion, S. E. Whitcomb, M. Di Paolo Emilio, N. Leroy, E. Tournefier, Julien Moreau, A. G. Wiseman, J.-P. Coulon, V. Loriette, Ping Koy Lam, J.-D. Fournier, Kenneth G. Libbrecht, I. Fiori, D. C. Coyne, G. McIntyre, Jordan Camp, T. Meier, J. Dalrymple, M. A. Arain, Gregory M. Harry, S. D'Antonio, M. Lei, A. Gennai, I. W. Martin, Virginio Sannibale, David E. McClelland, B. Mours, H. Bantilan, M. A. Barton, D.B. DeBra, S. H. Huttner, B. Bland, G. Brunet, A. Masserot, A. Dietz, D. Grosjean, E. Campagna, Claude Boccara, Fabio Postiglione, M. Ito, Luca Gammaitoni, F. Ya. Khalili, Atsushi J. Nishizawa, S. Gossler, P. Kwee, A. M. Rogan, F. Matichard, Roberto Conte, L. Matone, P. J. Veitch, Matthew Evans, L. Cardenas, A. Sibley, M. Del Prete, S. Frasca, S. Klimenko, Stephen Fairhurst, Giuseppe Castaldi, F. Paoletti, S. Sakata, L. Rolland, Fabrizio Barone, P. Ruggi, Rubab Khan, Miquel Trias, Richard O'Shaughnessy, B. Barr, P. Patel, D. B. Kozak, C. Vorvick, S. Hebri, J. Worden, L. Williams, A. Rüdiger, R. Riesen, S. Hamdani, Roland Schilling, Kazuhiro Hayama, D. Meyers, C. Pankow, P. Schwinberg, S. Wen, W. G. Anderson, G. Cella, B. P. Abbott, E. K. Gustafson, D. E. Clark, S. Vass, Jian Zhang, W. Kells, R. L. Savage, P. Armor, C. Torres, H. Vocca, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Laboratoire des matériaux avancés (LMA), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Virgo, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), VIRGO, The Virgo Collaboration, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux ( ARTEMIS ), Université Nice Sophia Antipolis ( UNS ), Université Côte d'Azur ( UCA ) -Université Côte d'Azur ( UCA ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de la Côte d'Azur, Université Côte d'Azur ( UCA ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Physique Corpusculaire et Cosmologie - Collège de France ( PCC ), Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -Collège de France ( CdF ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ) -AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Observatoire de Paris-Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Laboratoire de l'Accélérateur Linéaire ( LAL ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), ESPCI ParisTech, APC - Gravitation ( APC-Gravitation ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Max-Planck-Institut-Max-Planck-Institut, Laboratoire des matériaux avancés ( LMA ), Université Claude Bernard Lyon 1 ( UCBL ), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), B., Abbott, R., Abbott, R., Adhikari, P., Ajith, B., Allen, G., Allen, R., Amin, S. B., Anderson, W. G., Anderson, M. A., Arain, M., Araya, H., Armandula, P., Armor, Y., Aso, S., Aston, P., Aufmuth, C., Aulbert, S., Babak, S., Ballmer, H., Bantilan, B. C., Barish, C., Barker, D., Barker, B., Barr, P., Barriga, M. A., Barton, M., Bastarrika, K., Bayer, J., Betzwieser, P. T., Beyersdorf, I. A., Bilenko, G., Billingsley, R., Biswa, E., Black, K., Blackburn, L., Blackburn, D., Blair, B., Bland, T. P., Bodiya, L., Bogue, R., Bork, V., Boschi, S., Bose, P. R., Brady, V. B., Braginsky, J. E., Brau, M., Brinkmann, A., Brook, D. A., Brown, G., Brunet, A., Bullington, A., Buonanno, O., Burmeister, R. L., Byer, L., Cadonati, G., Cagnoli, J. B., Camp, J., Cannizzo, K., Cannon, J., Cao, L., Cardena, T., Casebolt, G., Castaldi, C., Cepeda, E., Chalkley, P., Charlton, S., Chatterji, S., Chelkowski, Y., Chen, N., Christensen, D., Clark, J., Clark, T., Cokelaer, R., Conte, D., Cook, T., Corbitt, D., Coyne, J. D. E., Creighton, A., Cumming, L., Cunningham, R. M., Cutler, J., Dalrymple, K., Danzmann, G., Davie, D., Debra, J., Degallaix, M., Degree, V., Dergachev, S., Desai, R., Desalvo, S., Dhurandhar, M., Díaz, J., Dickson, A., Dietz, F., Donovan, K. L., Dooley, E. E., Doome, R. W. P., Drever, I., Duke, J. C., Duma, R. J., Dupui, J. G., Dwyer, C., Echol, A., Effler, P., Ehren, E., Espinoza, T., Etzel, T., Evan, S., Fairhurst, Y., Fan, D., Fazi, H., Fehrmann, M. M., Fejer, L. S., Finn, K., Flasch, N., Fotopoulo, A., Freise, R., Frey, T., Fricke, P., Fritschel, V. V., Frolov, M., Fyffe, J., Garofoli, I., Gholami, J. A., Giaime, S., Giampani, K. D., Giardina, K., Goda, E., Goetz, L., Goggin, G., González, S., Gossler, R., Gouaty, A., Grant, S., Gra, C., Gray, M., Gray, R. J. S., Greenhalgh, A. M., Gretarsson, F., Grimaldi, R., Grosso, H., Grote, S., Grunewald, M., Guenther, E. K., Gustafson, R., Gustafson, B., Hage, J. M., Hallam, D., Hammer, C., Hanna, J., Hanson, J., Harm, G., Harry, E., Harstad, K., Hayama, T., Hayler, J., Heefner, I. S., Heng, M., Hennessy, A., Heptonstall, M., Hewitson, S., Hild, E., Hirose, D., Hoak, D., Hosken, J., Hough, S. H., Huttner, D., Ingram, M., Ito, A., Ivanov, B., Johnson, W. W., Johnson, D. I., Jone, G., Jone, R., Jone, L., Ju, P., Kalmu, V., Kalogera, S., Kamat, J., Kanner, D., Kasprzyk, E., Katsavounidi, K., Kawabe, S., Kawamura, F., Kawazoe, W., Kell, D. G., Keppel, F., Ya Khalili, R., Khan, E., Khazanov, C., Kim, P., King, J. S., Kissel, S., Klimenko, K., Kokeyama, V., Kondrashov, R. K., Kopparapu, D., Kozak, I., Kozhevatov, B., Krishnan, P., Kwee, P. K., Lam, M., Landry, M. M., Lang, B., Lantz, A., Lazzarini, M., Lei, N., Leindecker, V., Leonhardt, I., Leonor, K., Libbrecht, H., Lin, P., Lindquist, N. A., Lockerbie, D., Lodhia, M., Lormand, P., Lu, M., Lubinski, A., Lucianetti, H., Lück, B., Machenschalk, M., Macinni, M., Mageswaran, K., Mailand, V., Mandic, S., Márka, Z., Márka, A., Markosyan, J., Markowitz, E., Maro, I., Martin, R. M., Martin, J. N., Marx, K., Mason, F., Matichard, L., Matone, R., Matzner, N., Mavalvala, R., Mccarthy, D. E., Mcclelland, S. C., Mcguire, M., Mchugh, G., Mcintyre, G., Mcivor, D., Mckechan, K., Mckenzie, T., Meier, A., Melissino, G., Mendell, R. A., Mercer, S., Meshkov, C. J., Messenger, D., Meyer, J., Miller, J., Minelli, S., Mitra, V. P., Mitrofanov, G., Mitselmakher, R., Mittleman, O., Miyakawa, B., Moe, S., Mohanty, G., Moreno, K., Mossavi, C., Mowlowry, G., Mueller, S., Mukherjee, H., Mukhopadhyay, H., Müller Ebhardt, J., Munch, P., Murray, E., Myer, J., Myer, T., Nash, J., Nelson, G., Newton, A., Nishizawa, K., Numata, J., O'Dell, G., Ogin, B., O'Reilly, R., O'Shaughnessy, D. J., Ottaway, R. S., Otten, H., Overmier, B. J., Owen, Y., Pan, C., Pankow, M. A., Papa, V., Parameshwaraiah, P., Patel, M., Pedraza, S., Penn, A., Perreca, T., Petrie, I. M., Pinto, M., Pitkin, H. J., Pletsch, M. V., Plissi, F., Postiglione, M., Principe, R., Prix, V., Quetschke, F., Raab, D. S., Rabeling, H., Radkin, N., Rainer, M., Rakhmanov, M., Ramsunder, H., Rehbein, S., Reid, D. H., Reitze, R., Riesen, K., Rile, B., Rivera, N. A., Robertson, C., Robinson, E. L., Robinson, S., Roddy, A., Rodriguez, A. M., Rogan, J., Rollin, J. D., Romano, J., Romie, R., Route, S., Rowan, A., Rüdiger, L., Ruet, P., Russell, K., Ryan, S., Sakata, M., Samidi, L., Sancho de la Jordana, V., Sandberg, V., Sannibale, S., Saraf, P., Sarin, B. S., Sathyaprakash, S., Sato, P. R., Saulson, R., Savage, P., Savov, S. W., Schediwy, R., Schilling, R., Schnabel, R., Schofield, B. F., Schutz, P., Schwinberg, S. M., Scott, A. C., Searle, B., Sear, F., Seifert, D., Seller, A. S., Sengupta, P., Shawhan, D. H., Shoemaker, A., Sibley, X., Siemen, D., Sigg, S., Sinha, A. M., Sinte, B. J. J., Slagmolen, J., Slutsky, J. R., Smith, M. R., Smith, N. D., Smith, K., Somiya, B., Sorazu, L. C., Stein, A., Stochino, R., Stone, K. A., Strain, D. M., Strom, A., Stuver, T. Z., Summerscale, K. X., Sun, M., Sung, P. 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Subjects
Physics and Astronomy (miscellaneous), gamma-ray bursts, accreting neutron-stars, sgr 1806-20, energy neutrinos, 2004 hyperflare, giant flare, discovery, oscillations, sensitivity, detector, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, General Relativity and Quantum Cosmology (gr-qc), 01 natural sciences, General Relativity and Quantum Cosmology, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Pulsar, 0103 physical sciences, OSCILLATIONS, ENERGY NEUTRINOS, 010303 astronomy & astrophysics, DETECTOR, QC, QB, Physics, GAMMA-RAY BURSTS, TAIL, COSMIC cancer database, 010308 nuclear & particles physics, Gravitational wave, Settore FIS/01 - Fisica Sperimentale, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, LIGO, 2004 HYPERFLARE, Supernova, DISCOVERY, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], SGR 1806-20, Neutrino, SENSITIVITY, Gamma-ray burst, Event (particle physics), GIANT FLARE
Abstract

LIGO Scientific Collaboration, Virgo Collaboration; In gravitational-wave detection, special emphasis is put onto searches that focus on cosmic events detected by other types of astrophysical observatories. The astrophysical triggers, e.g. from gamma-ray and X-ray satellites, optical telescopes and neutrino observatories, provide a trigger time for analyzing gravitational wave data coincident with the event. In certain cases the expected frequency range, source energetics, directional and progenitor information is also available. Beyond allowing the recognition of gravitational waveforms with amplitudes closer to the noise floor of the detector, these triggered searches should also lead to rich science results even before the onset of Advanced LIGO. In this paper we provide a broad review of LIGO's astrophysically triggered searches and the sources they target.

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41. iSense: A technology platform for cold atom based: Quantum technologies

Author

Hannes Duncker, Mark Fromhold, Jon Malcolm, Thijs Wendrich, T. Valenzuela, Manuel Popp, Min-Kang Zhou, Ernst M. Rasel, Franck Pereira Dos Santos, Anton Piccardo-Selg, Patrick Windpassinger, FranceAndrea Bertoldi, B. Pelle, Clemens Ramelloo, Nicola Poli, Adele Hilico, Andreas Wicht, Marco G. Tarallo, Tommaso Mazzoni, Christian Kürbis, Florian Schreck, Guglielmo M. Tino, Alexander Grote, Ortwin Hellmig, Klaus Sengstock, Fiodor Sorrentino, Marie Christine Angonin, Wolfgang Ertmer, Christoph Becker, Simon Stellmer, Vincent Boyer, S. Dörscher, Lingxiao Zhu, Waldemar Herr, Achim Peters, J.O. Maclean, Peter Wolf, Peter Krüger, Kai Bongs, Christopher J. Mellor, Thomas Fernholz, and Philippe Bouyer

Subjects
Quantum technology, Physics, Atom interferometer, Gravimeter, Ultracold atom, Laser cooling, Nanotechnology, Laser amplifiers, Engineering physics, Bottleneck, Laser light
Abstract

A breakthrough in cold atom quantum technology is hindered by a bottleneck in the supporting technologies. We discuss a cold atom technology platform developed within the European iSense project, aiming at a gravimeter as demonstrator.

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