12 results on '"04.25.dg"'
Search Results
2. The formulation of dynamic Newtonian advanced gravity, DNAg.
- Author
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Worsley, Andrew
- Subjects
- *
NEWTON'S law of gravitation , *GEODESY , *NEWTONIAN fluids , *BINARY pulsars , *GRAVITATIONAL waves , *BLACK holes - Abstract
In this paper we find that the equations for gravity can be adapted by defining the equations for the curvature of space-time in terms of geodesics. Using these equations, we translate this curvature back into equations for an advanced Newtonian force of gravity. Using worked examples, we can show that the advanced Newtonian equations give results that technically agree exactly with gravitational experiment. These equations also technically agree exactly with binary pulsar data. At the same time these gravitational equations resolve the difficulties with the formation of singularities. Importantly, advanced Newtonian gravity provides readily testable gravitational predictions, particularly in the vicinity of black holes. [ABSTRACT FROM AUTHOR]
- Published
- 2014
- Full Text
- View/download PDF
3. Two binary stars gravitational waves: homotopy perturbation method.
- Author
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Zare, M., Jalili, O., and Delshadmanesh, M.
- Abstract
Homotopy perturbation is one of the newest methods for numerical analysis of deferential equations. We have used for solving wave equation around a black hole. Our conclusions have this method far reaching consequences for comparison of theoretical physics and experimental physics. [ABSTRACT FROM AUTHOR]
- Published
- 2012
- Full Text
- View/download PDF
4. Einstein-Born-Infeld on Taub-NUT spacetime in 2 k + 2 dimensions.
- Author
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Khodam-Mohammadi, A.
- Abstract
We wish to construct solutions of Taub-NUT spacetime in Einstein-Born-Infeld gravity in even dimensions. Since the Born-Infeld theory is a nonlinear electrodynamics theory, in leads to nonlinear differential equations. However, a proper analytical solution was not obtained, we try to solve it numerically (by the Runge-Kutta method) with initial conditions coinciding with those of our previous work in Einstein-Maxwell gravity. We solve the equations for 4, 6 and 8 dimensions and do data fitting by the least-squares method. For N = l = b = 1, the metric turns to the NUT solution only in 8 dimensions, but in 4 and 6 dimensions the spacetime does not have any NUT solution. [ABSTRACT FROM AUTHOR]
- Published
- 2009
- Full Text
- View/download PDF
5. Gravitational field around black hole induces photonic spin–orbit interaction that twists light
- Author
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Pan, Deng and Xu, Hong-Xing
- Published
- 2017
- Full Text
- View/download PDF
6. Issue of the spherically symmetric static vacuum metric in the relativistic theory of gravity.
- Author
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Kalashnikov, Vladimir
- Abstract
The spherically symmetric vacuum metric in the relativistic theory of gravity is analyzed numerically. It is found that there is no deviation of the numerical solution from that of general relativity except in the near-horizon range. The solution obtained has the well-established analytical asymptotics for both the near-and far-horizon limits. It satisfies the causality principle and does not impose a lower limit on the graviton mass. [ABSTRACT FROM AUTHOR]
- Published
- 2008
- Full Text
- View/download PDF
7. Systematic study of the stochastic gravitational-wave background due to stellar core collapse
- Author
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K. Crocker, Elisabeth Vangioni, Keith A. Olive, Vuk Mandic, Tania Regimbau, T. Prestegard, Observatoire de la Côte d'Azur ( OCA ), Centre National de la Recherche Scientifique ( CNRS ), Université Pierre et Marie Curie - Paris 6 ( UPMC ), Institut d'Astrophysique de Paris ( IAP ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), and Centre National de la Recherche Scientifique (CNRS)
- Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,gravitational radiation: stochastic ,supernova: collapse ,[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph] ,Collapse (topology) ,FOS: Physical sciences ,Astrophysics ,General Relativity and Quantum Cosmology (gr-qc) ,Parameter space ,01 natural sciences ,General Relativity and Quantum Cosmology ,[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] ,Gravitational wave background ,star: collapse ,Einstein Telescope ,0103 physical sciences ,supernova ,gravitational radiation: spectrum ,LIGO ,010306 general physics ,numerical calculations ,97.60.Jd ,Physics ,010308 nuclear & particles physics ,Gravitational wave ,95.85.Sz ,98.80.Cq ,formation ,gravitational radiation: background ,04.25.dg ,gravitational radiation detector ,detector: sensitivity ,Supernova ,Orders of magnitude (time) ,[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Stellar core collapse events are expected to produce gravitational waves via several mechanisms, most of which are not yet fully understood due to the current limitations in the numerical simulations of these events. In this paper, we begin with an empirical functional form that fits the gravitational-wave spectra from existing simulations of stellar core collapse and integrate over all collapse events in the universe to estimate the resulting stochastic gravitational-wave background. We then use a Gaussian functional form to separately fit and model a low-frequency peak in the core-collapse strain spectra, which likely occurs due to prompt convection. We systematically study the parameter space of both models, as well as the combined case, and investigate their detectability by upcoming gravitational-wave detectors, such as Advanced LIGO and Einstein Telescope. Assuming realistic formation rates for progenitors of core-collapse supernovae, our results indicate that both models are 2--4 orders of magnitude below the expected sensitivity of Advanced LIGO, and 1--2 orders of magnitude below that of the Einstein Telescope., 13 pages, 11 figures
- Published
- 2017
- Full Text
- View/download PDF
8. Digging deeper: Observing primordial gravitational waves below the binary black hole produced stochastic background
- Author
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Bangalore Suryanarayana Sathyaprakash, Salvatore Vitale, E. Katsavounidis, Nelson Christensen, Tania Regimbau, Matthew Evans, 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 ), Observatoire de la Côte d'Azur ( OCA ), Centre National de la Recherche Scientifique ( CNRS ), 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), Observatoire de la Côte d'Azur (OCA), and Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
noise ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,background: primordial ,Astrophysics::High Energy Astrophysical Phenomena ,[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph] ,FOS: Physical sciences ,General Physics and Astronomy ,Primordial black hole ,General Relativity and Quantum Cosmology (gr-qc) ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,General Relativity and Quantum Cosmology ,Gravitational wave background ,Einstein Telescope ,Binary black hole ,0103 physical sciences ,KAGRA ,LIGO ,010303 astronomy & astrophysics ,QC ,Astrophysics::Galaxy Astrophysics ,QB ,Physics ,010308 nuclear & particles physics ,Gravitational wave ,95.85.Sz ,gravitational radiation: background ,gravitational radiation: primordial ,Astronomy ,04.25.dg ,04.80.Nn ,background: stochastic ,gravitational radiation detector ,Black hole ,black hole: binary ,97.80.-d ,efficiency ,gravitational radiation: emission ,Stellar black hole ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,Hawking radiation ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
The merger rate of black hole binaries inferred from the detections in the first Advanced LIGO science run, implies that a stochastic background produced by a cosmological population of mergers will likely mask the primordial gravitational-wave background. Here we demonstrate that the next generation of ground-based detectors, such as the Einstein Telescope and Cosmic Explorer, will be able to observe binary black hole mergers throughout the universe with sufficient efficiency that the confusion background can potentially be subtracted to observe the primordial background at the level of $\Omega_{\mathrm{GW}} \simeq 10^{-13}$ after five years of observation., Comment: accepted for publication in PRL (7 pages, 4 figures)
- Published
- 2017
- Full Text
- View/download PDF
9. Search for intermediate mass black hole binaries in the first observing run of Advanced LIGO
- Author
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Abbott, and Abbott, B. P., and Abbott, R., and Acernese, T. D., and Ackley, F., and Adams, K., and Adams, C., and Addesso, T., and Adhikari, P., and Adya, R. X., and Affeldt, V. B., and Afrough, C., and Agarwal, M., and Agatsuma, B., and Aggarwal, K., and Aguiar, N., and Aiello, O. D., and Ain, L., and Allen, A., and Allen, B., and Allocca, G., and Almoubayyed, A., and Altin, H., and Amato, P. A., and Ananyeva, A., and Anderson, A., and Anderson, S. B., and Antier, W. G., and Appert, S., and Arai, S., and Araya, K., and Areeda, M. C., and Arnaud, J. S., and Arun, N., and Ascenzi, K. G., and Ashton, S., and Ast, G., and Aston, M., and Astone, S. M., and Aufmuth, P., and Aulbert, P., and AultONeal, C., and Avila-Alvarez, K., and Babak, A., and Bacon, S., and Bader, P., and Bae, M. K. M., and Baker, S., and Baldaccini, P. T., and Ballardin, F., and Ballmer, G., and Banagiri, S. W., and Barayoga, S., and Barclay, J. C., and Barish, S. E., and Barker, B. C., and Barone, D., and Barr, F., and Barsotti, B., and Barsuglia, L., and Barta, M., and Bartlett, D., and Bartos, J., and Bassiri, I., and Basti, R., and Batch, A., and Baune, J. C., and Bawaj, C., and Bazzan, M., and Becsy, M., and Beer, B., and Bejger, C., and Belahcene, M., and Bell, I., and Berger, A. S., and Bergmann, B. K., and Bell, G., and Berry, G., and Bersanetti, C. P. L., and Bertolini, D., and Betzwieser, A., and Bhagwat, J., and Bhandare, S., and Bilenko, R., and Billingsley, I. A., and Billman, G., and Birch, C. R., and Birney, J., and Birnholtz, R., and Biscans, O., and Bisht, S., and Bitossi, A., and Biwer, M., and Bizouard, C., and Blackburn, M. A., and Blackman, J. K., and Blair, J., and Blair, C. D., and Blair, D. G., and Bloemen, R. M., and Bock, S., and Bode, O., and Boer, N., and Bogaert, M., and Bohe, G., and Bondu, A., and Bonnand, F., and Boom, R., and Bork, B. A., and Boschi, R., and Bose, V., and Bouffanais, S., and Bozzi, Y., and Bradaschia, A., and Brady, C., and Braginsky, P. R., and Branchesi, V. B., and Brau, M., and Briant, J. E., and Brillet, T., and Brinkmann, A., and Brisson, M., and Brockill, V., and Broida, P., and Brooks, J. E., and Brown, A. F., and Brown, D. A., and Brown, D. D., and Brunett, N. M., and Buchanan, S., and Buikema, C. C., and Bulik, A., and Bulten, T., and Buonanno, H. J., and Buskulic, A., and Buy, D., and Byer, C., and Cabero, R. L., and Cadonati, M., and Cagnoli, L., and Cahillane, G., and Bustillo, C., Calderon and Callister, J., and Calloni, T. A., and Camp, E., and Canepa, J. B., and Canizares, M., and Cannon, P., and Cao, K. C., and Cao, H., and Capano, J., and Capocasa, C. D., and Carbognani, E., and Caride, F., and Carney, S., and Diaz, M. F., Casanueva and Casentini, J., and Caudill, C., and Cavaglia, S., and Cavalier, M., and Cavalieri, F., and Cella, R., and Cepeda, G., and Baiardi, C. B., Cerboni and Cerretani, L., and Cesarini, G., and Chamberlin, E., and Chan, S. J., and Chao, M., and Charlton, S., and Chassande-Mottin, P., and Chatterjee, E., and Cheeseboro, D., and Chen, B. D., and Chen, H. Y., and Cheng, Y., and Chincarini, H. -. P., and Chiummo, A., and Chmiel, A., and Cho, T., and Cho, H. S., and Chow, M., and Christensen, J. H., and Chu, N., and Chua, Q., and Chua, A. J. K., and Chung, S., and Chung, A. K. W., and Ciani, S., and Ciolfi, G., and Cirelli, R., and Cirone, C. E., and Clara, A., and Clark, F., and Cleva, J. A., and Cocchieri, F., and Coccia, C., and Cohadon, E., and Colla, P. -. F., and Collette, A., and Cominsky, C. G., and Constancio, L. R., J. r., and Conti, M., and Cooper, L., and Corban, S. J., and Corbitt, P., and Corley, T. R., and Cornish, K. R., and Corsi, N., and Cortese, A., and Costa, S., and Coughlin, C. A., and Coughlin, M. W., and Coulon, S. B., and Countryman, J. -. P., and Couvares, S. T., and Covas, P., and Cowan, P. B., and Coward, E. E., and Cowart, D. M., and Coyne, M. J., and Coyne, D. C., and Creighton, R., and Creighton, J. D. E., and Cripe, T. D., and Crowder, J., and Cullen, S. G., and Cumming, T. J., and Cunningham, A., and Cuoco, L., and Dal Canton, E., and Danilishin, T., and D'Antonio, S. L., and Danzmann, S., and Dasgupta, K., and Costa, A., Da Silva and Dattilo, C. F., and Dave, V., and Davier, I., and Davies, M., and Davis, G. S., and Daw, D., and Day, E. J., and De, B., and DeBra, S., and Deelman, D., and Degallaix, E., and De laurentis, J., and Deleglise, M., and Del Pozzo, S., and Denker, W., and Dent, T., and Dergachev, T., and De Rosa, V., and DeRosa, R., and DeSalvo, R. T., and Devenson, R., and Devine, J., and Dhurandhar, R. C., and Diaz, S., and Di Fiore, M. C., and Di Giovanni, L., and Di Girolamo, M., and Di Lieto, T., and Di Pace, A., and Di Palma, S., and Di Renzo, I., and Doctor, F., and Dolique, Z., and Donovan, V., and Dooley, F., and Doravari, K. L., and Dorrington, S., and Douglas, I., and Alvarez, R., Dovale and Downes, M., and Drago, T. P., and Drever, M., and Driggers, R. W. P., and Du, J. C., and Ducrot, Z., and Duncan, M., and Dwyer, J., and Edo, S. E., and Edwards, T. B., and Effler, M. C., and Eggenstein, A., and Ehrens, H. -. B., and Eichholz, P., and Eikenberry, J., and Eisenstein, S. S., and Essick, R. A., and Etienne, R. C., and Etzel, Z. B., and Evans, T., and Evans, M., and Factourovich, T. M., and Fafone, M., and Fair, V., and Fairhurst, H., and Fan, S., and Farinon, X., and Farr, S., and Farr, B., and Fauchon-Jones, W. M., and Favata, E. J., and Fays, M., and Fehrmann, M., and Feicht, H., and Fejer, J., and Fernandez-Galiana, M. M., and Ferrante, A., and Ferreira, I., and Ferrini, E. C., and Fidecaro, F., and Fiori, F., and Fiorucci, I., and Fisher, D., and Flaminio, R. P., and Fletcher, R., and Fong, M., and Forsyth, H., and Forsyth, P. W. F., and Fournier, S. S., and Frasca, J. -. D., and Frasconi, S., and Frei, F., and Freise, Z., and Frey, A., and Frey, R., and Fries, V., and Fritschel, E. M., and Frolov, P., and Fulda, V. V., and Fyffe, P., and Gabbard, M., and Gabel, H., and Gadre, M., and Gaebel, B. U., and Gair, S. M., and Gammaitoni, J. R., and Ganija, L., and Gaonkar, M. R., and Garufi, S. G., and Gaudio, F., and Gaur, S., and Gayathri, G., and Gehrels, V., and Gemme, N., and Genin, G., and Gennai, E., and George, A., and George, D., and Gergely, J., and Germain, L., and Ghonge, V., and Ghosh, S., Abhirup and Ghosh, Archisman and Ghosh, and Giaime, S., and Giardina, J. A., and Giazotto, K. D., and Gill, A., and Glover, K., and Goetz, L., and Goetz, E., and Gomes, R., and Gonzalez, S., and Castro, G., Gonzalez and Gopakumar, J. M., and Gorodetsky, A., and Gossan, M. L., and Gosselin, S. E., and Gouaty, M., and Grado, R., and Graef, A., and Granata, C., and Grant, M., and Gras, A., and Gray, S., and Greco, C., and Green, G., and Groot, A. C., and Grote, P., and Grunewald, H., and Gruning, S., and Guidi, P., and Guo, G. M., and Gupta, X., and Gupta, A., and Gushwa, M. K., and Gustafson, K. E., and Gustafson, E. K., and Hall, R., and Hall, B. R., and Hammond, E. D., and Haney, G., and Hanke, M., and Hanks, M. M., and Hanna, J., and Hannam, C., and Hannuksela, M. D., and Hanson, O. A., and Hardwick, J., and Harms, T., and Harry, J., and Harry, G. M., and Hart, I. W., and Haster, M. J., and Haughian, C. -. J., and Healy, K., and Heidmann, J., and Heintze, A., and Heitmann, M. C., and Hello, H., and Hemming, P., and Hendry, G., and Heng, M., and Hennig, I. S., and Henry, J., and Heptonstall, J., and Heurs, A. W., and Hild, M., and Hoak, S., and Hofman, D., and Holt, D., and Holz, K., and Hopkins, D. E., and Horst, P., and Hough, C., and Houston, J., and Howell, E. A., and Hu, E. J., and Huerta, Y. M., and Huet, E. A., and Hughey, D., and Husa, B., and Huttner, S., and Huynh-Dinh, S. H., and Indik, T., and Ingram, N., and Inta, D. R., and Intini, R., and Isa, G., and Isac, H. N., and Isi, J. -. M., and Iyer, M., and Izumi, B. R., and Jacqmin, K., and Jani, T., and Jaranowski, K., and Jawahar, P., and Jimenez-Forteza, S., and Johnson, F., and Jones, W. W., and Jones, D. I., and Jonker, R., and Ju, R. J. G., and Junker, L., and Kalaghatgi, J., and Kalogera, C. V., and Kandhasamy, V., and Kang, S., and Kanner, G., and Karki, J. B., and Karvinen, S., and Kasprzack, K. S., and Katolik, M., and Katsavounidis, M., and Katzman, E., and Kaufer, W., and Kawabe, S., and Kefelian, K., and Keitel, F., and Kemball, D., and Kennedy, A. J., and Kent, R., and Key, C., and Khalili, J. S., and Khan, F. Y., and Khan, I., and Khan, S., and Khazanov, Z., and Kijbunchoo, E. A., and Kim, N., Chunglee and Kim, and Kim, J. C., and Kim, W., and Kim, W. S., and Kimbrell, Y. -. M., and King, S. J., and King, E. J., and Kirchhoff, P. J., and Kissel, R., and Kleybolte, J. S., and Klimenko, L., and Koch, S., and Koehlenbeck, P., and Koley, S. M., and Kondrashov, S., and Kontos, V., and Korobko, A., and Korth, M., and Kowalska, W. Z., and Kozak, I., and Kraemer, D. B., and Kringel, C., and Krishnan, V., and Krolak, B., and Kuehn, A., and Kumar, G., and Kumar, P., and Kumar, R., and Kuo, S., and Kutynia, L., and Kwang, A., and Lackey, S., and Lai, B. D., and Landry, K. H., and Lang, M., and Lange, R. N., and Lantz, J., and Lanza, B., and Lartaux-Vollard, K., and Lasky, A., and Laxen, P. D., and Lazzarini, M., and Lazzaro, A., and Leaci, C., and Leavey, P., and Lee, S., and Lee, C. H., and Lee, H. K., and Lee, H. M., and Lee, H. W., and Lehmann, K., and Lenon, J., and Leonardi, A., and Leroy, M., and Letendre, N., and Levin, N., and Li, Y., and Libson, T. G. F., and Littenberg, A., and Liu, T. B., and Lockerbie, J., and London, N. A., and Lord, L. T., and Lorenzini, J. E., and Loriette, M., and Lormand, V., and Losurdo, M., and Lough, G., and Lousto, J. D., and Lovelace, C. O., and Lueck, G., and Lumaca, H., and Lundgren, D., and Lynch, A. P., and Ma, R., and Macfoy, Y., and Machenschalk, S., and MacInnis, B., and Macleod, M., and Hernandez, D. M., Magana and Magana-Sandoval, I., and Zertuche, F., Magana and Magee, L., and Majorana, R. M., and Maksimovic, E., and Man, I., and Mandic, N., and Mangano, V., and Mansell, V., and Manske, G. L., and Mantovani, M., And, M., Marchesoni, F., And, Marion, and Marka, F., and Marka, S., and Markakis, Z., and Markosyan, C., and Maros, A. S., and Martelli, E., and Martellini, F., and Martin, L., and Martynov, I. W., and Marx, D. V., and Mason, J. N., and Masserot, K., and Massinger, A., and Masso-Reid, T. J., and Mastrogiovanni, M., and Matas, S., and Matichard, A., and Matone, F., and Mavalvala, L., and Mayani, N., and Mazumder, R., and McCarthy, N., and McClelland, R., and McCormick, D. E., and McCuller and McGuire, S., and McIntyre, S. C., and McIver, G., and McManus, J., and McRae, D. J., and McWilliams, T., and Meacher, S. T., and Meadors, D., and Meidam, G. D., and Mejuto-Villa, J., and Melatos, E., and Mendell, A., and Mercer, G., and Merilh, R. A., and Merzougui, E. L., and Meshkov, M., and Messenger, S., and Messick, C., and Metzdorff, C., and Meyers, R., and Mezzani, P. M., and Miao, F., and Michel, H., and Middleton, C., and Mikhailov, H., and Milano, E. E., and Miller, L., and Miller, A. L., and Miller, A., and Miller, B. B., and Millhouse, J., and Minazzoli, M., and Minenkov, O., and Ming, Y., and Mishra, J., and Mitra, C., and Mitrofanov, S., and Mitselmakher, V. P., and Mittleman, G., and Moggi, R., and Mohan, A., and Mohapatra, M., and Montani, S. R. P., and Moore, M., and Moore, B. C., and Moraru, C. J., and Moreno, D., and Morriss, G., and Mours, S. R., and Mow-Lowry, B., and Mueller, C. M., and Muir, G., and Mukherjee, A. W., Arunava and Mukherjee, and Mukherjee, D., and Mukund, S., and Mullavey, N., and Munch, A., and Muniz, J., and Murray, E. A. M., and Napier, P. G., and Nardecchia, K., and Naticchioni, I., and Nayak, L., and Nelemans, R. K., and Nelson, G., and Neri, T. J. N., and Nery, M., and Neunzert, M., and Newport, A., and Newton, J. M., and Ng, G., and Nguyen, K. K. Y., and Nichols, T. T., and Nielsen, D., and Nissanke, A. B., and Noack, S., and Nocera, A., and Nolting, F., and Normandin, D., and Nuttall, M. E. N., and Oberling, L. K., and Ochsner, J., and Oelker, E., and Ogin, E., and Oh, G. H., and Oh, J. J., and Ohme, S. H., and Oliver, F., and Oppermann, M., and Oram, P., and O'Reilly, Richard J., and Ormiston, B., and Ortega, R., and O'Shaughnessy, L. F., and Ottaway, R., and Overmier, D. J., and Owen, H., and Pace, B. J., and Page, A. E., and Page, J., and Pai, M. A., and Pai, A., and Palamos, S. A., and Palashov, J. R., and Palomba, O., and Pal-Singh, C., and Pan, A., and Pang, H., and Pang, B., and Pankow, P. T. H., and Pannarale, C., and Pant, F., and Paoletti, B. C., and Paoli, F., and Papa, A., and Paris, M. A., and Parker, H. R., and Pascucci, W., and Pasqualetti, D., and Passaquieti, A., and Passuello, R., and Patricelli, D., and Pearlstone, B., and Pedraza, B. L., and Pedurand, M., and Pekowsky, R., and Pele, L., and Penn, A., and Perez, S., and Perreca, C. J., and Perri, A., and Pfeiffer, L. M., and Phelps, H. P., and Piccinni, M., and Pichot, O. J., and Piergiovanni, M., and Pierro, F., and Pillant, V., and Pinard, G., and Pinto, L., and Pitkin, I. M., and Poggiani, M., and Popolizio, R., and Porter, P., and Post, E. K., and Powell, A., and Prasad, J., and Pratt, J., and Predoi, J. W. W., and Prestegard, V., and Prijatelj, T., and Principe, M., and Privitera, M., and Prodi, S., and Prokhorov, G. A., and Puncken, L. G., and Punturo, O., and Puppo, M., and Puerrer, P., and Qi, M., and Qin, H., and Qiu, J., and Quetschke, S., and Quintero, V., and Quitzow-James, E. A., and Raab, R., and Rabeling, F. J., and Radkins, D. 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m. . s., Schönbeck, A., Schreiber, E., Schuette, D., Schulte, B. . w., Schutz, B. . f., Schwalbe, S. . g., Scott, J., Scott, S. . m., Seidel, E., Sellers, D., Sengupta, A. . s., Sentenac, D., Sequino, V., Sergeev, A., Shaddock, D. . a., Shaffer, T. . j., Shah, A. . a., Shahriar, M. . s., Shao, L., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. . h., Shoemaker, D. . m., Siellez, K., Siemens, X., Sieniawska, M., Sigg, D., Silva, A. . d., Singer, A., Singer, L. . p., Singh, A., Singh, R., Singhal, A., Sintes, A. . m., Slagmolen, B. . j. . j., Smith, B., Smith, J. . r., Smith, R. . j. . e., Son, E. . j., Sonnenberg, J. . a., Sorazu, B., Sorrentino, F., Souradeep, T., Spencer, A. . p., Srivastava, A. . k., Staley, A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stephens, B. . c., Stone, R., Strain, K. . a., Stratta, G., Strigin, S. . e., Sturani, R., Stuver, A. . l., Summerscales, T. . z., Sun, L., Sunil, S., Sutton, P. . j., Swinkels, B. . l., Szczepańczyk, M. . j., Tacca, M., Talukder, D., Tanner, D. . b., Tápai, M., Taracchini, A., Taylor, J. . a., Taylor, R., Theeg, T., Thomas, E. . g., Thomas, M., Thomas, P., Thorne, K. . a., Thorne, K. . s., Thrane, E., Tiwari, S., Tiwari, V., Tokmakov, K. . v., Toland, K., Tonelli, M., Tornasi, Z., Torrie, C. . i., Töyrä, D., Travasso, F., Traylor, G., Trifirò, D., Trinastic, J., Tringali, M. . c., Trozzo, L., Tsang, K. . w., Tse, M., Tso, R., Tuyenbayev, D., Ueno, K., Ugolini, D., Unnikrishnan, C. . s., Urban, A. . l., Usman, S. . a., Vahi, K., Vahlbruch, H., Vajente, G., Valdes, G., van Bakel, N., van Beuzekom, M., van den Brand, J. . f. . j., Van Den Broeck, C., Vander Hyde, D. . c., van der Schaaf, L., van Heijningen, J. . v., van Veggel, A. . a., Vardaro, M., Varma, V., Vass, S., Vasúth, M., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. . j., Venkateswara, K., Venugopalan, G., Verkindt, D., Vetrano, F., Viceré, A., Viets, A. . d., Vinciguerra, S., Vine, D. . j., Vinet, J. Y., Vitale, S., Vo, T., Vocca, H., Vorvick, C., Voss, D. . v., Vousden, W. . d., Vyatchanin, S. . p., Wade, A. . r., Wade, L. . e., Wade, M., Walet, R., Walker, M., Wallace, L., Walsh, S., Wang, G., Wang, H., Wang, J. . z., Wang, M., Wang, Y. F., Wang, Y., Ward, R. . l., Warner, J., Was, M., Watchi, J., Weaver, B., Wei, L. W., Weinert, M., Weinstein, A. . j., Weiss, R., Wen, L., Wessel, E. . k., Weßels, P., Westphal, T., Wette, K., Whelan, J. . t., Whiting, B. . f., Whittle, C., Williams, D., Williams, R. . d., Williamson, A. . r., Willis, J. . l., Willke, B., Wimmer, M. . h., Winkler, W., Wipf, C. . c., Wittel, H., Woan, G., Woehler, J., Wofford, J., Wong, K. . w. . k., Worden, J., Wright, J. . l., Wu, D. . s., Wu, G., Yam, W., Yamamoto, H., Yancey, C. . c., Yap, M. . j., Yu, Hang, Yu, Haocun, Yvert, M., Zadrożny, A., Zanolin, M., Zelenova, T., Zendri, J. P., Zevin, M., Zhang, L., Zhang, M., Zhang, T., Zhang, Y. H., Zhao, C., Zhou, M., Zhou, Z., Zhu, X. . j., Zucker, M. . e., Zweizig, J., 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 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), 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), 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)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique de Rennes (IPR), Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Kastler Brossel (LKB [Collège de France]), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF (institution))-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), LIGO Scientific, Virgo, 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), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Collège de France (CdF (institution)), 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), (Astro)-Particles Physics, Abbott, B. .p., Abbott, T. .d., Adhikari, R. .x., Adya, V. .b., Aguiar, O. .d., Altin, P. .a., Anderson, S. .b., Anderson, W. .g., Araya, M. .c., Areeda, J. .s., Arun, K. .g., Aston, S. .m., Bader, M. .k. .m., Baker, P. .t., Ballmer, S. .w., Barayoga, J. .c., Barclay, S. .e., Barish, B. .c., Batch, J. .c., Bell, A. .s., Berger, B. .k., Berry, C. .p. .l., Bilenko, I. .a., Billman, C. .r., Bizouard, M. .a., Blackburn, J. .k., Blair, C. .d., Blair, D. .g., Blair, R. .m., Boom, B. .a., Brady, P. .r., Braginsky, V. .b., BRANCHESI, MARICA, Brau, J. .e., Broida, J. .e., Brooks, A. .f., Brown, D. .a., Brown, D. .d., Brown, N. .m., Buchanan, C. .c., Bulten, H. .j., Byer, R. .l., Callister, T. .a., Calloni, E., Camp, J. .b., Cannon, K. .c., Capano, C. .d., Carney, M. .f., Cepeda, C. .b., CERBONI BAIARDI, LORENZO, Chamberlin, S. .j., Cheeseboro, B. .d., Chen, H. .y., Cho, H. .s., Chow, J. .h., Chua, A. .j. .k., Chung, A. .k. .w., Cirelli, C. .e., Clark, J. .a., Collette, C. .g., Cominsky, L. .r., Cooper, S. .j., Corbitt, T. .r., Corley, K. .r., Costa, C. .a., Coughlin, M. .w., Coughlin, S. .b., Countryman, S. .t., Covas, P. .b., Cowan, E. .e., Coward, D. .m., Cowart, M. .j., Coyne, D. .c., Creighton, J. .d. .e., Creighton, T. .d., Crowder, S. .g., Cullen, T. .j., Danilishin, S. .l., Da Silva Costa, C. .f., Davies, G. .s., Daw, E. .j., De Laurentis, M., De Rosa, R., Derosa, R. .t., Devine, R. .c., Díaz, M. .c., Di Girolamo, T., Dooley, K. .l., Downes, T. .p., Drever, R. .w. .p., Driggers, J. .c., Dwyer, S. .e., Edo, T. .b., Edwards, M. .c., Eikenberry, S. .s., Eisenstein, R. .a., Essick, R. .c., Evans, T. .m., Farr, W. .m., Fauchon Jones, E. .j., Fejer, M. .m., Ferreira, E. .c., Fisher, R. .p., Forsyth, P. .w. .f., Forsyth, S. .s., Fries, E. .m., Frolov, V. .v., Gadre, B. .u., Gaebel, S. .m., Gair, J. .r., Ganija, M. .r., Gaonkar, S. .g., Garufi, F., Giaime, J. .a., Giardina, K. .d., Gonzalez Castro, J. .m., Gorodetsky, M. .l., Gossan, S. .e., GRECO, GIUSEPPE, Green, A. .c., GUIDI, GIANLUCA MARIA, Gupta, M. .k., Gushwa, K. .e., Gustafson, E. .k., Hall, B. .r., Hall, E. .d., Hanke, M. .m., Hannam, M. .d., Hannuksela, O. .a., HARMS, JAN, Harry, G. .m., Harry, I. .w., Hart, M. .j., Heintze, M. .c., Heng, I. .s., Heptonstall, A. .w., Holz, D. .e., Houston, E. .a., Howell, E. .j., Hu, Y. .m., Huerta, E. .a., Huttner, S. .h., Ingram, D. .r., Isa, H. .n., Iyer, B. .r., Johnson, W. .w., Jones, D. .i., Jonker, R. .j. .g., Kalaghatgi, C. .v., Kanner, J. .b., Karvinen, K. .s., Kemball, A. .j., Key, J. .s., Khalili, F. .y., Khazanov, E. .a., Kim, J. .c., Kim, W. .s., Kimbrell, S. .j., King, E. .j., King, P. .j., Kissel, J. .s., Koehlenbeck, S. .m., Korth, W. .z., Kozak, D. .b., Lackey, B. .d., Lai, K. .h., Lang, R. .n., Lanza, R. .k., Lasky, P. .d., Lee, C. .h., Lee, H. .k., Lee, H. .m., Lee, H. .w., Li, T. .g. .f., Littenberg, T. .b., Lockerbie, N. .a., London, L. .t., Lord, J. .e., Lough, J. .d., Lousto, C. .o., Lundgren, A. .p., Macleod, D. .m., Magee, R. .m., Mansell, G. .l., Markosyan, A. .s., MARTELLI, FILIPPO, Martin, I. .w., Martynov, D. .v., Marx, J. .n., Massinger, T. .j., Mcclelland, D. .e., Mcguire, S. .c., Mcmanus, D. .j., Mcwilliams, S. .t., Meadors, G. .d., Mercer, R. .a., Merilh, E. .l., Meyers, P. .m., Mikhailov, E. .e., Milano, L., Miller, A. .l., Miller, B. .b., Mitrofanov, V. .p., Mohapatra, S. .r. .p., MONTANI, MATTEO, Moore, B. .c., Moore, C. .j., Morriss, S. .r., Mow Lowry, C. .m., Muir, A. .w., Muniz, E. .a. .m., Murray, P. .g., Nayak, R. .k., Nelson, T. .j. .n., Newport, J. .m., Ng, K. .k. .y., Nguyen, T. .t., Nielsen, A. .b., Normandin, M. .e. .n., Nuttall, L. .k., Ogin, G. .h., Oh, J. .j., Oh, S. .h., Ortega, L. .f., Ottaway, D. .j., Owen, B. .j., Pace, A. .e., Page, M. .a., Pai, S. .a., Palamos, J. .r., Pang, P. .t. .h., Pant, B. .c., Papa, M. .a., Paris, H. .r., Pearlstone, B. .l., Perez, C. .j., Perri, L. .m., Pfeiffer, H. .p., Piccinni, O. .j., PIERGIOVANNI, FRANCESCO, Pinto, I. .m., Porter, E. .k., Pratt, J. .w. .w., Prodi, G. .a., Prokhorov, L. .g., Quintero, E. .a., Raab, F. .j., Rabeling, D. .s., Ramirez, K. .e., Reitze, D. .h., Reyes, S. .d., Ricker, P. .m., Robertson, N. .a., Rollins, J. .g., Roma, V. .j., Romel, C. .l., Romie, J. .h., Ross, M. .p., Sampson, L. .m., Sanchez, E. .j., Sanders, J. .r., Sathyaprakash, B. .s., Saulson, P. .r., Savage, R. .l., Schofield, R. .m. .s., Schulte, B. .w., Schutz, B. .f., Schwalbe, S. .g., Scott, S. .m., Sengupta, A. .s., Shaddock, D. .a., Shaffer, T. .j., Shah, A. .a., Shahriar, M. .s., Shoemaker, D. .h., Shoemaker, D. .m., Silva, A. .d., Singer, L. .p., Sintes, A. .m., Slagmolen, B. .j. .j., Smith, J. .r., Smith, R. .j. .e., Son, E. .j., Sonnenberg, J. .a., Spencer, A. .p., Srivastava, A. .k., Stephens, B. .c., Strain, K. .a., STRATTA, MARIA GIULIANA, Strigin, S. .e., Stuver, A. .l., Summerscales, T. .z., Sutton, P. .j., Swinkels, B. .l., Szczepańczyk, M. .j., Tanner, D. .b., Taylor, J. .a., Thomas, E. .g., Thorne, K. .a., Thorne, K. .s., Tokmakov, K. .v., Torrie, C. .i., Tringali, M. .c., Tsang, K. .w., Unnikrishnan, C. .s., Urban, A. .l., Usman, S. .a., van den Brand, J. .f. .j., Vander Hyde, D. .c., van Heijningen, J. .v., van Veggel, A. .a., Veitch, P. .j., VETRANO, FLAVIO, VICERE', ANDREA, Viets, A. .d., Vine, D. .j., Voss, D. .v., Vousden, W. .d., Vyatchanin, S. .p., Wade, A. .r., Wade, L. .e., Wang, J. .z., Ward, R. .l., Weinstein, A. .j., Wessel, E. .k., Whelan, J. .t., Whiting, B. .f., Williams, R. .d., Williamson, A. .r., Willis, J. .l., Wimmer, M. .h., Wipf, C. .c., Wong, K. .w. .k., Wright, J. .l., Wu, D. .s., Yancey, C. .c., Yap, M. .j., Zhu, X. .j., and Zucker, M. .e.
- Subjects
Physics and Astronomy (miscellaneous) ,Astronomy ,Gravitational Wave ,Binary number ,Astrophysics ,01 natural sciences ,General Relativity and Quantum Cosmology ,star ,jet ,clusters ,LIGO ,010303 astronomy & astrophysics ,GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries) ,QC ,97.60.Lf ,QB ,candidate ,Physics ,black hole: spin ,04.25.dg ,04.30.-w ,[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] ,mergers ,Angular momentum ,coalescences ,Astrophysics::High Energy Astrophysical Phenomena ,IMBH ,FOS: Physical sciences ,General Relativity and Quantum Cosmology (gr-qc) ,Astrophysics::Cosmology and Extragalactic Astrophysics ,gravitational radiation: direct detection ,angular momentum ,O1 ,Intermediate BH search ,Binary black hole ,0103 physical sciences ,Binary star ,gravitational radiation: burst ,ddc:530 ,Gravitational Waves ,010308 nuclear & particles physics ,Gravitational wave ,gravitational radiation ,black hole: mass ,Gravitational Waves, LIGO, O1, IMBH ,530 Physik ,04.80.Nn ,gravitational radiation detector ,detector: sensitivity ,Physics and Astronomy ,Orders of magnitude (time) ,black hole: binary ,Intermediate-mass black hole ,gravitational radiation: emission ,Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik ,limits ,gravitational-waves - Abstract
During their first observational run, the two Advanced LIGO detectors attained an unprecedented sensitivity, resulting in the first direct detections of gravitational-wave signals and GW151226, produced by stellar-mass binary black hole systems. This paper reports on an all-sky search for gravitational waves (GWs) from merging intermediate mass black hole binaries (IMBHBs). The combined results from two independent search techniques were used in this study: the first employs a matched-filter algorithm that uses a bank of filters covering the GW signal parameter space, while the second is a generic search for GW transients (bursts). No GWs from IMBHBs were detected, therefore, we constrain the rate of several classes of IMBHB mergers. The most stringent limit is obtained for black holes of individual mass $100\,M_\odot$, with spins aligned with the binary orbital angular momentum. For such systems, the merger rate is constrained to be less than $0.93~\mathrm{Gpc^{-3}\,yr}^{-1}$ in comoving units at the $90\%$ confidence level, an improvement of nearly 2 orders of magnitude over previous upper limits., 8 pages, 2 figures
- Published
- 2017
- Full Text
- View/download PDF
10. Einstein-Born-Infeld on Taub-NUT spacetime in 2k + 2 dimensions
- Author
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Khodam-Mohammadi, A.
- Published
- 2009
- Full Text
- View/download PDF
11. Stochastic resonance in the flow of test particles in the field of a Kerr black hole
- Author
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Pyragas, K. and Svirskas, K.
- Published
- 2009
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- View/download PDF
12. Toward a dynamical shift condition for unequal mass black hole binary simulations
- Author
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Doreen Mueller, Bernd Bruegmann, Theoretical Physics Institute, and Friedrich-Schiller-Universität = Friedrich Schiller University Jena [Jena, Germany]
- Subjects
Physics ,Physics and Astronomy (miscellaneous) ,010308 nuclear & particles physics ,Gravitational wave ,Binary number ,04.25.dg ,FOS: Physical sciences ,General Relativity and Quantum Cosmology (gr-qc) ,Gauge (firearms) ,01 natural sciences ,Position dependent ,General Relativity and Quantum Cosmology ,Black hole ,Quantum electrodynamics ,0103 physical sciences ,04.25.D ,010306 general physics ,Constant (mathematics) ,04.30.Db - Abstract
Moving puncture simulations of black hole binaries rely on a specific gauge choice that leads to approximately stationary coordinates near each black hole. Part of the shift condition is a damping parameter, which has to be properly chosen for stable evolutions. However, a constant damping parameter does not account for the difference in mass in unequal mass binaries. We introduce a position dependent shift damping that addresses this problem. Although the coordinates change, the changes in the extracted gravitational waves are small., Comment: 15 pages, submitted to CQG for NRDA 2009 conference proceedings
- Published
- 2009
- Full Text
- View/download PDF
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