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LISA Definition Study Report / Colpi, Monica (INFN, Milan Bicocca) ; Danzmann, Karsten (Hannover, Max Planck Inst. Grav.) ; Hewitson, Martin (Hannover, Max Planck Inst. Grav.) ; Jetzer, Philippe (U. Zurich (main)) ; Nelemans, Gijs (Nijmegen U., IMAPP) ; Petiteau, Antoine (IRFU, Saclay) ; Shoemaker, David (MIT, MKI) ; Sopuerta, Carlos (ICE, Bellaterra) ; Stebbins, Robin (Colorado U.) ; Tanvir, Nial (Leicester U.) et al.
The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to detect and study gravitational waves from space. [...]
arXiv:2402.07571. - 155.
Fulltext

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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

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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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Cosmology with the Laser Interferometer Space Antenna / LISA Cosmology Working Group Collaboration
The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational wave observations extends well beyond these two objectives. [...]
arXiv:2204.05434; LISA CosWG-22-03; FERMILAB-PUB-22-349-SCD.- 2023-08-28 - 176 p. - Published in : Living Rev. Relativ. 26 (2023) 5 Fulltext: jt - PDF; 2204.05434 - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server

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Unveiling the gravitational universe at $\mu$-Hz frequencies / Sesana, Alberto (Milan Bicocca U.) ; Korsakova, Natalia (Cote d'Azur Observ., Nice) ; Sedda, Manuel Arca (U. Heidelberg (main)) ; Baibhav, Vishal (Johns Hopkins U. (main)) ; Barausse, Enrico (SISSA, Trieste) ; Barke, Simon (U. Florida, Gainesville (main)) ; Berti, Emanuele (Johns Hopkins U. (main)) ; Bonetti, Matteo (Milan Bicocca U.) ; Capelo, Pedro R. (U. Zurich (main)) ; Caprini, Chiara (APC, Paris) et al.
We propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to $\mu$-Hz frequency range. By the 2040s', the $\mu$-Hz frequency band, bracketed in between the Laser Interferometer Space Antenna (LISA) and pulsar timing arrays, will constitute the largest gap in the coverage of the astrophysically relevant GW spectrum. [...]
arXiv:1908.11391.- 2021-09-04 - 28 p. - Published in : Exp. Astron. 51 (2021) 1333-1383 Fulltext: 1908.11391 - PDF; document - PDF;

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Se också: liknande författarnamn
58	Volonteri, M
2	Volonteri, M J R M

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