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Singularity avoidance in classical gravity from four-fermion interaction

delete2014-06-01
delete26
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OA
AI
C
Cosimo Bambi
D
Daniele Malafarina
A
Antonino Marcianò *
L
Leonardo Modesto
DOI:10.1016/j.physletb.2014.05.013delete
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摘要

摘要

En 中文
We derive the dynamics of the gravitational collapse of a homogeneous and spherically symmetric cloud in a classical set-up endowed with a topological sector of gravity and a non-minimal coupling to fermions. The effective theory consists of the Einstein-Hilbert action plus Dirac fermions interacting through a four-fermion vertex. At the classical level we obtain the same picture that has been recently studied by some of us within a wide range of effective theories inspired by a super-renormalizable and a symptotically free theory of gravity. The classical singularity is replaced by a bounce beyond which the cloud re-expands indefinitely. We thus show that even at a classical level if we allow for a non-minimal coupling of gravity to fermions event horizons may never form for a suitable choice of some parameters of the theory. (C) 2014 The Authors. Published by Elsevier B.V
Keyword:
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期刊

Physics Letters B 封面图
Physics Letters B
IF:
4.5
论文数:
3.2W
被引数:
7.3W

机构

F
fudan university
学者数:
11.8W
论文数: 7.7W
被引数: 121
引用论文

引用论文

a Terminating black holes in asymptotically free quantum gravity
err2014-02-20
err76
errOAAI
errBambi, Cosimo; Malafarina, Daniele; Modesto, Leonardo
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