Cosmology and nuclear physics implications of a subsolar gravitational-wave event
Detecting a compact subsolar object would have profound implications in physics, the reach of which depends on the nature of the object. Here, we explore such consequences for a putative subsolar-mass gravitational wave event detected by the LIGO-Virgo-KAGRA Collaboration. We forecast that the nature of a subsolar binary (made of light neutron stars, primordial black holes, or more exotic compact objects) can be inferred with a great statistical confidence level already during the ongoing fourth observing run, based on the large tidal deformability effects on the signal. The detection of a primordial black hole would have implications for cosmology and dark matter scenarios, while the measurement of the tidal deformability of a subsolar neutron star could rule out or confirm the existence of strange stars made of quarks.
Authors
- Paolo Pani (ORCID: https://orcid.org/0000-0003-4443-1761)
- Massimo Vaglio (ORCID: https://orcid.org/0000-0002-7285-3489)
- Gabriele Franciolini (ORCID: https://orcid.org/0000-0002-6892-9145)
- Francesco Crescimbeni (ORCID: https://orcid.org/0009-0001-4088-5443)
Institutions
- Scuola Internazionale Superiore di Studi Avanzati (IT)
- Istituto Nazionale di Fisica Nucleare (IT)
- Institute for Fundamental Physics of the Universe (IT)
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma I (IT)
- European Organization for Nuclear Research (CH)
- Sapienza University of Rome (IT)
Publication Details
- Journal
- Physical review. D/Physical review. D.
- Published
- 2025-04-18
- DOI
- https://doi.org/10.1103/physrevd.111.083538
- Citations
- 6
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 6.93
Funders
- Sapienza Università di Roma
- Ministero dell'Università e della Ricerca