Zobrazeno 1 - 10
of 25
pro vyhledávání: '"black hole: coalescence"'
Autor:
Joseph D. Miller, Giorgio Bianciardi
Publikováno v:
Journal of High Energy Astrophysics. 31:31-36
The recent observations of gravitational waves during the coalescence of black holes has confirmed various predictions of general relativity. However, some concerns have been raised that these putative waves are artifacts. We have analyzed the ten co
Autor:
Kalogera, Vicky, Sathyaprakash, B. S., Bailes, Matthew, Bizouard, Marie-Anne, Buonanno, Alessandra, Burrows, Adam, Colpi, Monica, Evans, Matt, Fairhurst, Stephen, Hild, Stefan, Kasliwal, Mansi M., Lehner, Luis, Mandel, Ilya, Mandic, Vuk, Nissanke, Samaya, Papa, Maria Alessandra, Reddy, Sanjay, Rosswog, Stephan, Broeck, Chris Den, Ajith, P., Anand, Shreya, Andreoni, Igor, Arun, K. G., Barausse, Enrico, Baryakhtar, Masha, Belgacem, Enis, Berry, Christopher P. L., Bertacca, Daniele, Brito, Richard, Caprini, Chiara, Chatziioannou, Katerina, Coughlin, Michael, Cusin, Giulia, Dietrich, Tim, Dirian, Yves, East, William E., Fan, Xilong, Daniel G. Figueroa, Foffa, Stefano, Ghosh, Archisman, Hall, Evan, Harms, Jan, Harry, Ian, Hinderer, Tanja, Janka, Thomas, Justham, Stephen, Kasen, Dan, Kotake, Kei, Lovelace, Geoffrey, Maggiore, Michele, Mangiagli, Alberto, Mapelli, Michela, Maselli, Andrea, Matas, Andrew, Mciver, Jess, Messer, Bronson, Mezzacappa, Tony, Mills, Cameron, Mueller, Bernhard, Müller, Ewald, Pürrer, Michael, Pani, Paolo, Pratten, Geraint, Regimbau, Tania, Sakellariadou, Mairi, Schneider, Raffaella, Sesana, Alberto, Shao, Lijing, Sotiriou, P. Thomas, Tamanini, Nicola, Tauris, Thomas, Thrane, Eric, Valiante, Rosa, Meent, Maarten, Varma, Vijay, Vines, Justin, Vitale, Salvatore, Yang, Huan, Yunes, Nicolas, Zumalacarregui, Miguel, Punturo, Michele, Reitze, David, Couvares, Peter, Katsanevas, Stavros, Kajita, Takaaki, Lueck, Harald, Mcclelland, David, Rowan, Sheila, Sanders, Gary, Shoemaker, David, Den Brand, Jo
Publikováno v:
INSPIRE-HEP
Richard Brito
Richard Brito
The next generation of ground-based gravitational-wave detectors will observe coalescences of black holes and neutron stars throughout the cosmos, thousands of them with exceptional fidelity. The Science Book is the result of a 3-year effort to study
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b1ec3b193f37c11bc196911be782def
http://arxiv.org/abs/2111.06990
http://arxiv.org/abs/2111.06990
We present a comprehensive comparison between numerical relativity (NR) angular momentum fluxes at infinity and the corresponding quantity entering the radiation reaction in TEOBResumS, an Effective-One-Body (EOB) waveform model for nonprecessing coa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::028b92c6f036d97e19f58961d2ac6fad
Publikováno v:
Physical review / D 103(12), 123023 (2021). doi:10.1103/PhysRevD.103.123023
Physical review / D 103(12), 123023 (2021). doi:10.1103/PhysRevD.103.123023
The waveform templates of the matched filtering-based gravitational-wave search ought to cover wide range of parameters for the prosperous detection. Numerical relativit
The waveform templates of the matched filtering-based gravitational-wave search ought to cover wide range of parameters for the prosperous detection. Numerical relativit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::856b6cfe42ee637d49f497cd7d05c8ac
Publikováno v:
Physical Review Research
Physical Review Research, American Physical Society, 2020, 2, pp.023314. ⟨10.1103/PhysRevResearch.2.023314⟩
Physical Review Research, American Physical Society, 2020, 2, pp.023314. ⟨10.1103/PhysRevResearch.2.023314⟩
Unveiling the origin of the coalescing binaries detected via gravitational waves (GW) is challenging, notably if no multi-wavelength counterpart is detected. One important diagnostic tool is the coalescing binary distribution with respect to the larg
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2020, 102 (2), pp.023033. ⟨10.1103/PhysRevD.102.023033⟩
Physical Review D
Physical Review D, American Physical Society, 2020, 102 (2), pp.023033. ⟨10.1103/PhysRevD.102.023033⟩
Phys.Rev.D, 2020, 102 (2), pp.023033. ⟨10.1103/PhysRevD.102.023033⟩
Physical Review D
Physical Review D, American Physical Society, 2020, 102 (2), pp.023033. ⟨10.1103/PhysRevD.102.023033⟩
The Laser Interferometer Space Antenna (LISA) is slated for launch in the early 2030s. A main target of the mission is massive black hole binaries that have an expected detection rate of $\sim20$ yr$^{-1}$. We present a parameter estimation analysis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::552b680f48ab2fcab268180ba12787f6
https://hal.science/hal-02634682
https://hal.science/hal-02634682
Publikováno v:
Classical and quantum gravity, 36 (24
Intermediate mass-ratio coalescences are potential signals of ground-based and space-based gravitational observatories. Accurate modeling of their waveforms within general relativity can be achieved within black hole perturbation theory including sel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e110fa81e941a4b91885f8c6a4854d0c
http://arxiv.org/abs/1901.05370
http://arxiv.org/abs/1901.05370
Publikováno v:
Class.Quant.Grav.
Class.Quant.Grav., 2019, 36 (10), pp.105009. ⟨10.1088/1361-6382/ab185e⟩
Classical and Quantum Gravity
Classical and Quantum Gravity, IOP Publishing, 2019, 36 (10), pp.105009. ⟨10.1088/1361-6382/ab185e⟩
Class.Quant.Grav., 2019, 36 (10), pp.105009. ⟨10.1088/1361-6382/ab185e⟩
Classical and Quantum Gravity
Classical and Quantum Gravity, IOP Publishing, 2019, 36 (10), pp.105009. ⟨10.1088/1361-6382/ab185e⟩
We introduce a novel test of General Relativity in the strong-field regime of a binary black hole coalescence. Combining information coming from Numerical Relativity simulations of coalescing black hole binaries with a Bayesian reconstruction of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::23ee4c2b3457a3fce8533e4f30ab48af
http://hdl.handle.net/11568/988484
http://hdl.handle.net/11568/988484
Akademický článek
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Publikováno v:
Astron.Astrophys.
Astron.Astrophys., 2018, 610, pp.A58. ⟨10.1051/0004-6361/201731875⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 610, pp.A58. ⟨10.1051/0004-6361/201731875⟩
Astron.Astrophys., 2018, 610, pp.A58. 〈10.1051/0004-6361/201731875〉
Astron.Astrophys., 2018, 610, pp.A58. ⟨10.1051/0004-6361/201731875⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 610, pp.A58. ⟨10.1051/0004-6361/201731875⟩
Astron.Astrophys., 2018, 610, pp.A58. 〈10.1051/0004-6361/201731875〉
Context. Gravitational wave interferometers have proven the existence of a new class of binary black hole (BBH) weighing tens of solar masses, and have provided the first reliable measurement of the rate of coalescing black holes (BHs) in the local U
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4677daf06c26345b2dbb287060b3a591
https://hal.archives-ouvertes.fr/hal-01730089
https://hal.archives-ouvertes.fr/hal-01730089