Spherically symmetric models for stars and voids II: constraints on the radial pressures-Reference-Cited by-同舟云学术

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Spherically symmetric models for stars and voids II: constraints on the radial pressures

Published:2004-02-20 Issue:6 Volume:21 Page:1351-1370
ISSN:0264-9381
Container-title:Classical and Quantum Gravity
language:
Short-container-title:Class. Quantum Grav.

Author:

Fayos Francesc,Torres Ramón

Publisher

IOP Publishing

Subject

Physics and Astronomy (miscellaneous)

Reference32 articles.

1. Spherically symmetric models for charged stars and voids: I. Charge bound

2. Exterior solution for a charged radiating sphere in general relativity (stars)

3. General matching of two spherically symmetric spacetimes

Cited by 5 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Role of equation of states and thermodynamic potentials in avoidance of trapped surfaces in gravitational collapse;General Relativity and Gravitation;2019-12-17

2. Charged radiating stars with Lie symmetries;The European Physical Journal C;2019-10

3. A quantum improvement to the gravitational collapse of radiating stars;Classical and Quantum Gravity;2011-04-06

4. A class of interiors for Vaidya's radiating metric: singularity-free gravitational collapse;Classical and Quantum Gravity;2008-08-15

5. Some aspects of bubbles and voids in a cosmological context;Classical and Quantum Gravity;2005-10-03

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