CERN Accelerating science

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1.
Cosmology with massive black hole binary mergers in the LISA era / Mangiagli, Alberto (APC, Paris) ; Caprini, Chiara (Geneva U. ; CERN) ; Volonteri, Marta (Paris, Inst. Astrophys.) ; Marsat, Sylvain (L2IT, Toulouse) ; Vergani, Susanna (LUTH, Meudon ; GEPI, Meudon ; LERMA, Ivry) ; Tamanini, Nicola (L2IT, Toulouse) ; Speri, Lorenzo (Potsdam, Max Planck Inst.)
In $\sim2034$ the Laser Interferometer Space Antenna (LISA) will detect the coalescence of massive black hole binaries (MBHBs) from $10^5$ to $10^7 {\, \rm M}_\odot$ up to $z\sim10$. The gravitational wave (GW) signal is expected to be accompanied by a powerful electromagnetic (EM) counterpart, from radio to X-ray, generated by the gas accreting on the binary. If LISA locates the MBHB merger within an error box $<10 \, \rm deg^2$, EM telescopes can be pointed in the same portion of the sky to detect the emission from the last stages of the MBHB orbits or the very onset of the nuclear activity, paving the way to test the nature of gas in a rapidly changing space-time. [...]
2022 - 6 p. - Published in : PoS ICHEP2022 (2022) 125 Fulltext: PDF;
In : 41st International Conference on High Energy Physics (ICHEP 2022), Bologna, Italy, 6 - 13 Jul 2022, pp.125
2.
Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts / Mangiagli, Alberto (APC, Paris) ; Caprini, Chiara (Geneva U. ; CERN) ; Volonteri, Marta (Paris, Inst. Astrophys.) ; Marsat, Sylvain (L2IT, Toulouse) ; Vergani, Susanna (LUTH, Meudon) ; Tamanini, Nicola (L2IT, Toulouse) ; Inchauspé, Henri (APC, Paris ; Heidelberg U.)
In the next decade, the Laser Interferometer Space Antenna (LISA) will detect the coalescence of massive black hole binaries (MBHBs) in the range $[10^4, 10^8] \, \rm M_{\odot}$, up to $z\sim10$. Their gravitational wave (GW) signal is expected to be accompanied by an electromagnetic counterpart (EMcp), generated by the gas accreting on the binary or on the remnant BH. [...]
arXiv:2207.10678.- 2022-11-15 - 28 p. - Published in : Phys. Rev. D 106 (2022) 103017 Fulltext: 2207.10678 - PDF; Publication - PDF;

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