Holographic cold dense matter constrained by neutron stars
Lin Zhang, Mei Huang

TL;DR
This paper uses holographic QCD models within Einstein-Maxwell-dilaton and KKSS frameworks to construct a neutron star equation of state, aligning with astrophysical data and suggesting matter remains confined in the core.
Contribution
It introduces a novel holographic approach combining EMD and KKSS models to constrain neutron star matter, differing from previous DBI-based methods.
Findings
Hybrid EoS consistent with astrophysical constraints
Maximum neutron star mass around 2.5 solar masses
Stable nuclear matter branch with no favored quark matter core
Abstract
The equation of state (EoS) for cold dense matter inside neutron stars is investigated by using holographic QCD models in the framework of the Einstein-Maxwell-dilaton (EMD) system and the improved Karch-Katz-Son-Stephanov (KKSS) action for matter part. This method of describing holographic nuclear matter in the EMDKKSS framework is different from that by using the Dirac-Born-Infeld (DBI) action and the Chern-Simons (CS) terms. Combining with the Hebeler-Lattimer-Pethick-Schwenk (HLPS) intermediate equation of state (EoS), the hybrid EoS inside the neutron stars is constructed. The obtained hybrid EoS is located in the range that is defined by the low-density chiral effective theory, the high-density perturbative QCD, and the polytropic interpolations between them, and is constrained by the astrophysics observations. The square of the sound velocity reaches a maximum value larger…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · High-pressure geophysics and materials · Quantum, superfluid, helium dynamics
