SLOWLY ROTATING BOSON-FERMION STAR-Reference-Cited by-同舟云学术

SLOWLY ROTATING BOSON-FERMION STAR

Published:2001-12 Issue:06 Volume:10 Page:881-892
ISSN:0218-2718
Container-title:International Journal of Modern Physics D
language:en
Short-container-title:Int. J. Mod. Phys. D

Author:

DE SOUSA CLAUDIO M. G.¹²,SILVEIRA VANDA¹

Affiliation:

1. International Centre of Condensed Matter Physics, Universidade de Brasília, Caixa Postal 04513, 70919-970, Brasília-DF, Brazil

2. Diretoria de Matemática, Universidade Católica de Brasilia, QS 07, Lote 01, EPCT, 72022-900, Brasília-DF, Brazil

Abstract

Relativistic prescription is used to study the slow rotation of stars composed by self-gravitating bosons and fermions (fermions may be considered as neutrons). Previous results demand that purely boson stars are unable to display slow rotation, if one uses relativistic prescription with classical scalar fields. In contrast to this, the present work shows that a combined boson-fermion star in its ground-state can rotate. Its structure and stability are analysed under slow rotation approximations.

Publisher

World Scientific Pub Co Pte Lt

Subject

Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics

Link

https://www.worldscientific.com/doi/pdf/10.1142/S0218271801001360

Reference15 articles.

1. On Massive Neutron Cores

2. Systems of Self-Gravitating Particles in General Relativity and the Concept of an Equation of State

3. Cold Bose stars

4. THE STRUCTURE AND FORMATION OF BOSON STARS

5. Combined boson-fermion stars

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