Directly comparing GW150914 with numerical solutions of Einstein’s equations for binary black hole coalescence
B. P. AbbottCalifornia Institute of TechnologyR. AbbottCalifornia Institute of TechnologyT. D. AbbottLouisiana State UniversityM. R. AbernathyAmerican UniversityF. AcerneseComplesso Universitario di Monte S.AngeloK. AckleyUniversity of FloridaC. AdamsLIGO Livingston ObservatoryT. AdamsUniversité Savoie Mont BlancP. AddessoUniversity of Sannio at BeneventoR. X. AdhikariCalifornia Institute of TechnologyV. B. AdyaAlbert-Einstein-InstitutC. AffeldtAlbert-Einstein-InstitutM. AgathosNikhef, Science ParkK. AgatsumaNikhef, Science ParkN. AggarwalMassachusetts Institute of TechnologyO. D. AguiarInstituto Nacional de Pesquisas EspaciaisL. AielloGran Sasso Science InstituteA. AinInter-University Centre for Astronomy and AstrophysicsP. AjithInternational Centre for Theoretical SciencesB. AllenAlbert-Einstein-InstitutA. AlloccaINFNP. A. AltinAustralian National UniversityS. B. AndersonCalifornia Institute of TechnologyW. G. AndersonUniversity of Wisconsin-MilwaukeeK. AraiCalifornia Institute of TechnologyM. C. ArayaCalifornia Institute of TechnologyC. C. ArceneauxThe University of MississippiJ. S. AreedaCalifornia State University FullertonN. ArnaudUniversité Paris-SaclayK. G. ArunChennai Mathematical InstituteS. AscenziINFNG. AshtonUniversity of SouthamptonM. AstUniversität HamburgS. M. AstonLIGO Livingston ObservatoryP. AstoneINFNP. AufmuthLeibniz Universität HannoverC. AulbertAlbert-Einstein-InstitutS. BabakAlbert-Einstein-InstitutP. BaconUniversité Paris DiderotM. K. M. BaderNikhef, Science ParkP. T. BakerMontana State UniversityF. BaldacciniINFNG. BallardinEuropean Gravitational Observatory (EGO)S. W. BallmerSyracuse UniversityJ. C. BarayogaCalifornia Institute of TechnologyS. E. BarclayUniversity of GlasgowB. C. BarishCalifornia Institute of TechnologyD. BarkerF. BaroneComplesso Universitario di Monte S.AngeloB. BarrUniversity of GlasgowL. BarsottiMassachusetts Institute of TechnologyM. BarsugliaUniversité Paris DiderotD. BartaRMKIJ. BartlettI. BartosColumbia UniversityR. BassiriStanford UniversityA. BastiINFNJ. C. BatchC. BauneAlbert-Einstein-InstitutV. BavigaddaEuropean Gravitational Observatory (EGO)M. BazzanINFNM. BejgerA. S. BellUniversity of GlasgowB. K. BergerCalifornia Institute of TechnologyG. BergmannAlbert-Einstein-InstitutC. P. L. BerryUniversity of BirminghamD. BersanettiINFNA. BertoliniNikhef, Science ParkJ. BetzwieserLIGO Livingston ObservatoryS. BhagwatSyracuse UniversityR. BhandareRRCATI. A. BilenkoLomonosov Moscow State UniversityG. BillingsleyCalifornia Institute of TechnologyJ. BirchLIGO Livingston ObservatoryR. BirneyUniversity of the West of ScotlandS. BiscansMassachusetts Institute of TechnologyA. BishtAlbert-Einstein-InstitutM. BitossiEuropean Gravitational Observatory (EGO)C. BiwerSyracuse UniversityM. A. BizouardUniv. Paris-SudJ. K. BlackburnCalifornia Institute of TechnologyC. D. BlairUniversity of Western AustraliaD. G. BlairUniversity of Western AustraliaR. M. BlairS. BloemenRadboud University NijmegenO. BockAlbert-Einstein-InstitutM. BoërUniversité Côte d’AzurG. BogaertUniversité Côte d’AzurC. BoganAlbert-Einstein-InstitutA. BohéAlbert-Einstein-InstitutC. BondUniversity of BirminghamF. BonduInstitut de Physique de RennesR. BonnandUniversité Savoie Mont BlancB. A. BoomNikhef, Science ParkR. BorkCalifornia Institute of TechnologyV. BoschiINFNS. BoseInter-University Centre for Astronomy and AstrophysicsY. BouffanaisUniversité Paris DiderotA. BozziEuropean Gravitational Observatory (EGO)C. BradaschiaINFN
2016en
ABI
Аннотация
Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
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