Published in:
EPJ Web of Conferences, 274 (2022), Seite 07006
Language:
Not determined
DOI:
10.1051/epjconf/202227407006
ISSN:
2100-014X
Origination:
Footnote:
Description:
<jats:p>Determining the phase structure of Quantum Chromodynamics (QCD) and its Equation of State (EOS) at densities and temperatures realized inside neutron stars and their mergers is a long-standing open problem. The holographic V-QCD framework provides a model for the EOS of dense and hot QCD, which describes the deconfinement phase transition between a dense baryonic and a quark matter phase. We use this model in fully general relativistic hydrodynamic (GRHD) simulations to study the formation of quark matter and the emitted gravitational wave signal of binary systems that are similar to the first ever observed neutron star merger event GW170817.</jats:p>