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4 results on '"Boris Hage"'

1. 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

2. The GEO-HF project

Author

C. A. Cantley, C. Robinson, Benjamin William Allen, Karsten Danzmann, L. Ribichini, Boris Hage, Gerhard Heinzel, Benno Willke, T. Regimbau, B. Barr, A. Grant, S. H. Huttner, S. Babak, Roland Schilling, R. Balasubramanian, Manuel Luna, Yousuke Itoh, C. Aulbert, U. Weiland, Roman Schnabel, D. Churches, V. Re, C. Messenger, Soumya D. Mohanty, Martin Hewitson, Ik Siong Heng, Richard J. K. Taylor, V. Quetschke, Bangalore Suryanarayana Sathyaprakash, Gianpietro Cagnoli, J. R. Smith, R. J. Dupuis, Ian Taylor, Badri Krishnan, C. N. Colacino, M. Malec, Kenneth A. Strain, R. A. Mercer, Karsten Kötter, Yi Chen, Frank Seifert, T. Meier, G. Newton, Alberto Vecchio, Carsten Fallnich, Stefan Hild, Peter Aufmuth, A. Hepstonstall, S. Berukoff, I. Gholami, Walter Winkler, Harald Lück, M. V. Plissi, D. I. Robertson, Hartmut Grote, Henning Vahlbruch, P. Ajith, A. Bunkowski, Stefan Goßler, S. Grunewald, Linqing Wen, Herbert Welling, Alexander Franzen, Graham Woan, Stuart Reid, Thomas Cokelaer, Joseph D. Romano, H. Rehbein, Bernard F. Schutz, Kasem Mossavi, Soma Mukherjee, Jan Harms, P. G. Murray, Andreas Freise, J. H. Hough, Matthew Pitkin, Michael Perreur-Lloyd, P. Kwee, A. M. Sintes, Andre Thüring, E. J. Elliffe, N. A. Robertson, Gareth Jones, B. Machenschalk, R. Zhu, Carlo Ungarelli, Sheila Rowan, Simon Chelkowski, Curt Cutler, H. Ward, John Veitch, Reinhard Prix, Peter H. Sneddon, P. Williams, Roger Jones, Maria Alessandra Papa, Albrecht Rüdiger, David Crooks, Morag M. Casey, and M. Heurs

Subjects
Physics, Upgrade, Gravitational-wave observatory, Physics and Astronomy (miscellaneous), Work (electrical), Emerging technologies, Scale (chemistry), SIGNAL (programming language), Detector, Systems engineering, LIGO
Abstract

The GEO 600 gravitational wave detector uses advanced technologies including signal recycling and monolithic fused-silica suspensions to achieve a sensitivity close to the kilometre scale LIGO and VIRGO detectors. As soon as the design sensitivity of GEO 600 is reached, the detector will be operated as part of the worldwide network to acquire data of scientific interest. The limited infrastructure at the GEO site does not allow for a major upgrade of the detector. Hence the GEO collaboration decided to improve the sensitivity of the GEO detector by small sequential upgrades some of which will be tested in prototypes first. The development, test and installation of these upgrades are named 'The GEO-HF Project.' This paper describes the upgrades considered in the GEO-HF project as well as their scientific reasons. We will describe the changes in the GEO 600 infrastructure and the prototype work that is planned to support these upgrades. Finally, we will point to some laboratory research that identifies new technologies or optical configurations that might undergo a transition into detector subsystems within the GEO-HF project.

Published
2006

3. Squeezed-field injection for gravitational wave interferometers

Author

Alexander Franzen, Simon Chelkowski, Karsten Danzmann, Roman Schnabel, Boris Hage, and Henning Vahlbruch

Subjects
Physics, Quantum Physics, Physics and Astronomy (miscellaneous), Gravitational wave, business.industry, Detector, FOS: Physical sciences, GEO600, Interferometry, Optics, Astronomical interferometer, Coherent states, Quantum Physics (quant-ph), business
Abstract

In a recent table-top experiment we demonstrated the compatibility of three advanced interferometer techniques for gravitational wave detection, namely power-recycling, detuned signal-recycling and squeezed field injection. The interferometer's signal to noise ratio was improved by up to 2.8 dB beyond the coherent state's shot-noise. This value was mainly limited by optical losses on the squeezed field. We present a detailed analysis of the optical losses of in our experiment and provide an estimation of the possible nonclassical performance of a future squeezed field enhanced GEO600 detector., Comment: 5 pages, 3 figures

Published
2006

4. Status of the GEO600 detector

Author

S. J. Berukoff, S. H. Huttner, B. Barr, P. G. Murray, Roland Schilling, Peter Aufmuth, T. Meier, Reinhard Prix, G. Newton, Roman Schnabel, J. H. Hough, Gerhard Heinzel, Alberto Vecchio, Sheila Rowan, Benno Willke, V. Quetschke, Bangalore Suryanarayana Sathyaprakash, H. Ward, Graham Woan, Stuart Reid, D. Churches, J. R. Smith, Maria Alessandra Papa, A. Hepstonstall, Curt Cutler, Ian Taylor, Jan Harms, D. I. Robertson, Bernard F. Schutz, Morag M. Casey, M. Heurs, Albrecht Rüdiger, N. A. Robertson, A. Bunkowski, R. Zhu, A. Thüring, F. Seifert, Thomas Cokelaer, John Veitch, C. A. Cantley, Karsten Kötter, C. Robinson, Gareth Jones, Stefan Goßler, B. Machenschalk, Benjamin William Allen, Karsten Danzmann, Carlo Ungarelli, Peter H. Sneddon, R. Balasubramanian, M. V. Plissi, Carsten Fallnich, Stefan Hild, Stanislav Babak, Soma Mukherjee, V. Re, A. M. Sintes, Herbert Welling, S. Grunewald, Roger Jones, Simon Chelkowski, Hartmut Grote, A. Franzen, C. Messenger, L. Ribichini, U. Weiland, H. Rehbein, Andreas Freise, H. Vahlbruch, Walter Winkler, Harald Lück, Matthew Pitkin, Michael Perreur-Lloyd, Kenneth A. Strain, R. A. Mercer, P. R. Williams, P. Ajith, David Crooks, Yousuke Itoh, Ik Siong Heng, I. Gholami, R. J. Dupuis, Richard J. K. Taylor, Gianpietro Cagnoli, Martin Hewitson, A. Grant, E. J. Elliffe, T. Regimbau, Soumya D. Mohanty, Boris Hage, Linqing Wen, Joseph D. Romano, Kasem Mossavi, C. N. Colacino, M. Malec, Yi Chen, Manuel Luna, Badri Krishnan, P. Kwee, and C. Aulbert

Subjects
Physics, Optics, Physics and Astronomy (miscellaneous), business.industry, Duty cycle, Detector, business, GEO600, Sensitivity (electronics)
Abstract

Of all the large interferometric gravitational-wave detectors, the German/British project GEO600 is the only one which uses dual recycling. During the four weeks of the international S4 data-taking run it reached an instrumental duty cycle of 97% with a peak sensitivity of 7 × 10-22 Hz-1/2 at 1 kHz. This paper describes the status during S4 and improvements thereafter.

Published
2006

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