Thermodynamic instabilities in holographic neutron stars at finite temperature

DOI10.1088/1361-6382/ABB1F5zbMath1479.85006arXiv1911.02554OpenAlexW3080127120MaRDI QIDQ5162050

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Publication date: 1 November 2021

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1911.02554

zbMATH Keywords

holographyAdS/CMTholographic metals

Mathematics Subject Classification ID

Stefan problems, phase changes, etc. (80A22) Classical and relativistic thermodynamics (80A10) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Fermionic systems in quantum theory (81V74)

Related Items (1)

Scalar correlators and normal modes in holographic neutron stars

Cites Work

• Statistical mechanics of gravitating systems
• Holographic metals at finite temperature
• Degenerate stars and gravitational collapse in ads/CFT
• Fermionic halos at finite temperature in AdS/CFT
• Holographic neutron stars
• Thermodynamical instabilities of perfect fluid spheres in General Relativity
• PHASE TRANSITIONS IN SELF-GRAVITATING SYSTEMS
• Relativistic gravothermal instabilities
• On the number of unstable modes of an equilibrium
• Turning point instabilities for relativistic stars and black holes
• On Massive Neutron Cores

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