z-logo
Premium
On Ellis' programme within fourth order gravity
Author(s) -
Schmidt H.J.
Publication year - 1988
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.2113090431
Subject(s) - physics , scalar curvature , curvature , mathematical physics , einstein , conformal map , scalar field , de sitter universe , action (physics) , equivalence (formal languages) , infinity , f(r) gravity , theoretical physics , geometry , mathematical analysis , mathematics , universe , quantum mechanics , quantum gravity , pure mathematics , quantum
For the non‐tachyonic curvature squared action we show that the expanding Bianchi‐type I models tend to the dust‐filled Einstein‐de Sitter model for t tending to infinity if the metric is averaged over the typical oscillation period. Applying a conformal equivalence between curvature squared action and a minimally coupled scalar field (which holds for all dimensions > 2) the problem is solved by discussing a massive scalar field in an anisotropic cosmological model.

This content is not available in your region!

Continue researching here.

Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom