English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/38355
Title: Modified F(R) Hořava–Lifshitz gravity: a way to accelerating FRW cosmology
Authors: Chaichian, Masud; Nojiri, Shin'ichi; Odintsov, Sergei D.
Issue Date: 10-Aug-2010
Publisher: Institute of Physics Publishing
Citation: Classical and Quantum Gravity 27 (18) : 185021 (2010)
Abstract: We propose a general approach for the construction of modified gravity which is invariant under foliation-preserving diffeomorphisms. Special attention is paid to the formulation of a modified F(R) Hořava–Lifshitz gravity (FRHL), whose Hamiltonian structure is studied. It is demonstrated that the spatially flat FRW equations of FRHL are consistent with the constraint equations. The analysis of de Sitter solutions for several versions of FRHL indicates that the unification of the early-time inflation with the late-time acceleration is possible. It is shown that a special choice of parameters for FRHL leads to the same spatially flat FRW equations as in the case of the traditional F(R)-gravity. Finally, an essentially most general modified Hořava–Lifshitz gravity is proposed, motivated by its fully diffeomorphism-invariant counterpart, with the restriction that the action does not contain derivatives higher than the second order with respect to the time coordinate.
Publisher version (URL): http://dx.doi.org/10.1088/0264-9381/27/18/185021
URI: http://hdl.handle.net/10261/38355
ISSN: 0264-9381
DOI: 10.1088/0264-9381/27/18/185021
Embargoed until: 2011-08-11
E-ISSN: 1361-6382
Appears in Collections:(ICE) Artículos
Files in This Item:
File Description SizeFormat 
1001.4102v3.pdf207,24 kBAdobe PDFView/Open
Show full item record

WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.