Babak, Stanislav - Резултати от търсенето

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Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds / Babak, Stanislav (APC, Paris) ; Falxa, Mikel (LPC2E, Orleans ; APC, Paris) ; Franciolini, Gabriele (CERN) ; Pieroni, Mauro (CERN)
Pulsar Timing Array (PTA) observations hinted towards the existence of a stochastic gravitational wave background (SGWB) in the nHz frequency band. Still, the nature of the SGWB signal cannot be confidently inferred from current data, and the leading explanation invokes mergers of supermassive black holes. [...]
arXiv:2404.02864; CERN-TH-2024-039.- 2024-09-11 - 16 p. - Published in : Phys. Rev. D 110 (2024) 063022 Fulltext: Publication - PDF; 2404.02864 - PDF;

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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.
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Stochastic gravitational wave background from stellar origin binary black holes in LISA / Babak, Stanislav (APC, Paris) ; Caprini, Chiara (Geneva U., Dept. Theor. Phys. ; CERN) ; Figueroa, Daniel G. (Valencia U., IFIC) ; Karnesis, Nikolaos (Aristotle U., Thessaloniki) ; Marcoccia, Paolo (Stavanger U.) ; Nardini, Germano (Stavanger U.) ; Pieroni, Mauro (CERN) ; Ricciardone, Angelo (Pisa U. ; Padua U.) ; Sesana, Alberto (Milan Bicocca U. ; INFN, Milan Bicocca ; Brera Observ.) ; Torrado, Jesús (Padua U. ; INFN, Padua)
We use the latest constraints on the population of stellar origin binary black holes (SOBBH) from LIGO/Virgo/KAGRA (LVK) observations, to estimate the stochastic gravitational wave background (SGWB) they generate in the frequency band of LISA. We account for the faint and distant binaries, which contribute the most to the SGWB, by extending the merger rate at high redshift assuming it tracks the star formation rate. [...]
arXiv:2304.06368.- 2023-08-14 - 39 p. - Published in : JCAP 2308 (2023) 034 Fulltext: 2304.06368 - PDF; document - PDF;

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Observing GW190521-like binary black holes and their environment with LISA / Sberna, Laura (Potsdam, Max Planck Inst.) ; Babak, Stanislav (APC, Paris) ; Marsat, Sylvain (L2IT, Toulouse) ; Caputo, Andrea (Tel Aviv U. ; Weizmann Inst.) ; Cusin, Giulia (Geneva U. ; Paris, Inst. Astrophys.) ; Toubiana, Alexandre (Potsdam, Max Planck Inst.) ; Barausse, Enrico (SISSA, Trieste ; INFN, Trieste ; INFM, Trieste ; IFPU, Trieste) ; Caprini, Chiara (Geneva U. ; CERN) ; Dal Canton, Tito (IJCLab, Orsay) ; Sesana, Alberto (Milan Bicocca U. ; INFN, Milan Bicocca) et al.
Binaries of relatively massive black holes like GW190521 have been proposed to form in dense gas environments, such as the disks of Active Galactic Nuclei (AGNs), and they might be associated with transient electromagnetic counterparts. The interactions of this putative environment with the binary could leave a significant imprint at the low gravitational wave frequencies observable with the Laser Interferometer Space Antenna (LISA). [...]
arXiv:2205.08550.- 2022-09-15 - 17 p. - Published in : Phys. Rev. D 106 (2022) 064056 Fulltext: 2205.08550 - PDF; PhysRevD.106.064056 - PDF;

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Laser Interferometer Space Antenna / LISA Collaboration
Following the selection of The Gravitational Universe by ESA, and the successful flight of LISA Pathfinder, the LISA Consortium now proposes a 4 year mission in response to ESA's call for missions for L3. [...]
arXiv:1702.00786. - 2017. - 41 p.
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Виж също: автори с подобни имена
104	Babak, S
9	Babak, S V
16	Babak, S.
1	Babak, Stas

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