Determinant-Gravity: Cosmological implications
Author(s) -
Denis Comelli,
A. D. Dolgov
Publication year - 2004
Publication title -
journal of high energy physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.998
H-Index - 261
eISSN - 1126-6708
pISSN - 1029-8479
DOI - 10.1088/1126-6708/2004/11/062
Subject(s) - cosmological constant , einstein , physics , action (physics) , metric (unit) , term (time) , mathematical physics , theoretical physics , f(r) gravity , gravitation , constant (computer programming) , lagrangian , classical mechanics , quantum gravity , quantum mechanics , economics , computer science , operations management , quantum , programming language
We analyze the action $\int d^4x \sqrt{\det||{\cal B} g_{\mu\nu}+ {\cal C} R_{\mu\nu}}||$ as a possible alternative or addition to the Einstein gravity.Choosing a particular form of ${\cal B}(R)= \sqrt {R}$ we can restore theEinstein gravity and, if ${\cal B}=m^2$, we obtain the cosmological constantterm. Taking ${\cal B} = m^2 + {\cal B}_1 R$ and expanding the action in $1/m^2$, we obtain as a leading term the Einstein Lagrangian with a cosmologicalconstant proportional to $m^4$ and a series of higher order operators. Ingeneral case of non-vanishing ${\cal B}$ and ${\cal C}$ new cosmologicalsolutions for the Robertson-Walker metric are obtained.Comment: revtex format, 5 pages,8 figures,references adde
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