Slowly rotating thin shell gravastars

DOI10.1088/0264-9381/33/2/025005zbMath1332.83028arXiv1506.06485OpenAlexW3105022092WikidataQ57751733 ScholiaQ57751733MaRDI QIDQ2787558

Shijun Yoshida, Nami Uchikata

Publication date: 4 March 2016

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

Full work available at URL: https://arxiv.org/abs/1506.06485

zbMATH Keywords

rotationperturbationthin shellgravastar

Mathematics Subject Classification ID

Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (6)

Approximate universal relations for neutron stars and quark stars ⋮ Observational signatures from horizonless black shells imitating rotating black holes ⋮ Slowly rotating ultra-compact Schwarzschild star in the gravastar limit ⋮ The multipolar structure of fuzzballs ⋮ Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections ⋮ Study of gravastars in Rastall gravity

Cites Work

• Ergosphere instability
• Stable gravastars with generalized exteriors
• How to tell a gravastar from a black hole
• A mass shell with flat interior cannot rotate rigidly
• Viscous shear in the Kerr metric
• Stable gravastars—an alternative to black holes?
• Gravastars must have anisotropic pressures

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