Published December 12, 2014 | Version v1
Journal article

Jeans instability in classical and modified gravity

  • 1. Department of Higher Mathematics, University "Dubna", 141980 Dubna (Russian Federation)
  • 2. Novosibirsk State University, Novosibirsk, 630090 (Russian Federation)
  • 3. Dipartimento di Fisica e Scienze della Terra, Università degli Studi di Ferrara, Polo Scientifico e Tecnologico – Edificio C, Via Saragat 1, 44122 Ferrara (Italy)
  • 4. ITEP, Bol. Cheremushkinsaya ul., 25, 113259 Moscow (Russian Federation)
  • 5. Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Ferrara, Polo Scientifico e Tecnologico – Edificio C, Via Saragat 1, 44122 Ferrara (Italy)

Description

Gravitational instability in classical Jeans theory, General Relativity, and modified gravity is considered. The background density increase leads to a faster growth of perturbations in comparison with the standard theory. The transition to the Newtonian gauge in the case of coordinate dependent background metric functions is studied. For modified gravity a new high frequency stable solution is found

Availability note (English)

Available from http://dx.doi.org/10.1016/j.physletb.2014.11.004

Additional details

Identifiers

DOI
10.1016/j.physletb.2014.11.004;
arXiv
arXiv:1406.7104v2;
PII
S0370-2693(14)00806-5;

Publishing Information

Journal Title
Physics Letters. Section B
Journal Volume
739
Journal Page Range
p. 279-284
ISSN
0370-2693
CODEN
PYLBAJ

Optional Information

Copyright
Copyright (c) 2014 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.