Megahertz Gravitational Waves from Neutron Star Mergers
Institució Catalana de Recerca i Estudis Avançats · Barcelona Institute of Science and Technology · +3 more institutions
Abstract
Neutron star mergers provide a unique laboratory for the study of strong-field gravity coupled to quantum chromodynamics in extreme conditions. The frequencies and amplitudes of the resulting gravitational waves encode invaluable information about the merger. Simulations to date have shown that these frequencies lie in the kilohertz range. They have also shown that, if quantum chromodynamics possesses a first-order phase transition at high baryon density, then this is likely to be accessed during the merger dynamics. Here, we show that this would result in the nucleation of superheated and/or supercompressed bubbles whose subsequent dynamics would produce gravitational waves in the megahertz range. We estimate…
Citation impact
- FWCI
- 35.89
- Percentile
- 99%
- References
- 0
Authors
4- DBDiego BlasCorresponding
Institució Catalana de Recerca i Estudis Avançats, Barcelona Institute of Science and Technology, Institute of Science and Technology
- JCJorge Casalderrey-Solana
Universitat de Barcelona
- DMDavid Mateos
Institució Catalana de Recerca i Estudis Avançats, Centre de Physique Théorique, Universitat de Barcelona
- MSMikel Sanchez-Garitaonandia
Centre de Physique Théorique, Universitat de Barcelona
Topics & keywords
- Physics
- Gravitational wave
- Neutron star
- Hertz
- Amplitude
- Astrophysics
- Quantum mechanics
Funding
- ECEuropean Commission
- GDGeneralitat de Catalunya
- MDMinisterio de Ciencia e InnovaciónAward: PID2023-146686NB-C31
- H2Horizon 2020 Framework ProgrammeAwards: 101141909, 758759
- EREuropean Research Council
- EREuropean Regional Development Fund
- AEAgencia Estatal de Investigación
- IDInstitut de Ciències del CosmosAwards: 2021-SGR-872, PID2019–105614 GB-C21, PID2022-136224NB-C21, CEX2019-000918-M, PID2019–105614 GB-C22, PID2022-136224NB-C22