\(f(R)\) gravity constrained by PPN parameters and stochastic background of gravitational waves
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Publication:1031875
DOI10.1007/S10714-009-0758-1zbMATH Open1176.83001arXiv0808.1335OpenAlexW2125817250WikidataQ63380460 ScholiaQ63380460MaRDI QIDQ1031875
Author name not available (Why is that?)
Publication date: 23 October 2009
Published in: (Search for Journal in Brave)
Abstract: We analyze seven different viable -gravities towards the Solar System tests and stochastic gravitational waves background. The aim is to achieve experimental bounds for the theory at local and cosmological scales in order to select models capable of addressing the accelerating cosmological expansion without cosmological constant but evading the weak field constraints. Beside large scale structure and galactic dynamics, these bounds can be considered complimentary in order to select self-consistent theories of gravity working at the infrared limit. It is demonstrated that seven viable -gravities under consideration not only satisfy the local tests, but additionally, pass the above PPN-and stochastic gravitational waves bounds for large classes of parameters.
Full work available at URL: https://arxiv.org/abs/0808.1335
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