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Title: Neutron star mergers chirp about vacuum energy

Journal Article · · Journal of High Energy Physics (Online)
 [1];  [2];  [2]; ORCiD logo [2];  [3]
  1. Cornell University, Ithaca, NY (United States); None
  2. Syracuse University, Syracuse, NY (United States)
  3. University of California, Davis, CA (United States)

Observations of gravitational waves from neutron star mergers open up novel directions for exploring fundamental physics: they offer the first access to the structure of objects with a non-negligible contribution from vacuum energy to their total mass. The presence of such vacuum energy in the inner cores of neutron stars occurs in new QCD phases at large densities, with the vacuum energy appearing in the equation of state for a new phase. This in turn leads to a change in the internal structure of neutron stars and influences their tidal deformabilities which are measurable in the chirp signals of merging neutron stars. By considering three commonly used neutron star models we show that for large chirp masses the effect of vacuum energy on the tidal deformabilities can be sizable. Measurements of this sort have the potential to provide a first test of the gravitational properties of vacuum energy independent from the acceleration of the Universe, and to determine the size of QCD contributions to the vacuum energy.

Research Organization:
University of California, Riverside, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
SC0018298; SC0009998
OSTI ID:
1512287
Alternate ID(s):
OSTI ID: 1905123
Journal Information:
Journal of High Energy Physics (Online), Journal Name: Journal of High Energy Physics (Online) Journal Issue: 9 Vol. 2018; ISSN 1029-8479
Publisher:
Springer NatureCopyright Statement
Country of Publication:
United States
Language:
English

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Cited By (8)

Tidal deformability with sharp phase transitions in (binary) neutron stars text January 2018
Pixelated Dark Energy journal August 2019
Tidal deformability with sharp phase transitions in binary neutron stars journal April 2019
Equation-of-state constraints and the QCD phase transition in the era of gravitational-wave astronomy
  • Bauswein, Andreas; Bastian, Niels-Uwe Friedrich; Blaschke, David
  • XIAMEN-CUSTIPEN WORKSHOP ON THE EQUATION OF STATE OF DENSE NEUTRON-RICH MATTER IN THE ERA OF GRAVITATIONAL WAVE ASTRONOMY, AIP Conference Proceedings https://doi.org/10.1063/1.5117803
conference January 2019
Equation-of-state Constraints and the QCD Phase Transition in the Era of Gravitational-Wave Astronomy text January 2019
Gravitational waves from neutron star mergers and their relation to the nuclear equation of state text January 2019
Identifying a first-order phase transition in neutron star mergers through gravitational waves text January 2018
Identifying a First-Order Phase Transition in Neutron-Star Mergers through Gravitational Waves journal February 2019