What is the source of the PTA GW signal?
King's College London · National Institute of Chemical Physics and Biophysics · +7 more institutions
Abstract
The most conservative interpretation of the nHz stochastic gravitational wave background (SGWB) discovered by NANOGrav and other pulsar timing array (PTA) collaborations is astrophysical, namely that it originates from supermassive black hole (SMBH) binaries. However, alternative cosmological models have been proposed, including cosmic strings, phase transitions, domain walls, primordial fluctuations, and ``audible'' axions. We perform a multimodel analysis (MMA) to compare how well these different hypotheses fit the NANOGrav data, both in isolation and in combination with SMBH binaries, and address the questions: Which interpretations fit the data best, and which are disfavored? We also discuss experimental…
Citation impact
- FWCI
- 46.82
- Percentile
- 100%
- References
- 279
Authors
10- JEJohn EllisCorresponding
King's College London, National Institute of Chemical Physics and Biophysics, European Organization for Nuclear Research
- MFMalcolm Fairbairn
King's College London
- GFGabriele Franciolini
Istituto Nazionale di Fisica Nucleare, Sezione di Roma I, Sapienza University of Rome
- GHGert Hütsi
National Institute of Chemical Physics and Biophysics
- AJAntonio J. Iovino
National Institute of Chemical Physics and Biophysics, Istituto Nazionale di Fisica Nucleare, Sezione di Roma I, Sapienza University of Rome
Topics & keywords
- Gravitational wave
- Physics
- Pulsar
- Supermassive black hole
- Axion
- SIGNAL (programming language)
- Astrophysics
- Gravitational wave background
Funding
- ECEuropean CommissionAwards: 101065736, 101007855, H2020, 757480, TK133, DarkGRA-757480
- ETEesti TeadusagentuurAwards: TK133, PSG869, PRG803
- MDMinistero dell’Istruzione, dell’Università e della RicercaAwards: B81I18001170001, H2020, 00001
- NCNarodowe Centrum NaukiAward: 2018/31/D/ST2/02048
- H2Horizon 2020 Framework ProgrammeAward: 101007855
- HEHORIZON EUROPE Framework ProgrammeAward: 101007855
- SAScience and Technology Facilities CouncilAwards: ST/T000759/1, ST/T000759/1, ST/T00679X/1
- EREuropean Regional Development FundAwards: H2020, TK133
- ARAmaldi Research CenterAward: B81I18001170001
- HEH2020 European Research CouncilAward: DarkGRA–757480
- HEHORIZON EUROPE Marie Sklodowska-Curie ActionsAwards: 101065736, 101007855