Non-analytical power-law correction to the Einstein–Hilbert action: Gravitational wave propagation

Author:

Fiorucci D.1,Lecian O. M.1,Montani G.2

Affiliation:

1. Physics Department, "Sapienza" University of Rome, P.le Aldo Moro 5, 00185 Roma, Italy

2. Physics Department, "Sapienza" University of Rome, ENEA-UTFUSMAG, C. R. Frascati, c/o Via Enrico Fermi 45, 00044 Frascati, Roma, Italy

Abstract

We analyze the features of the Minkowskian limit of a particular non-analytical f(R) model, whose Taylor expansion in the weak-field limit does not hold, as far as gravitational waves (GWs) are concerned. We solve the corresponding Einstein equations and we find an explicit expression of the modified GWs as the sum of two terms, i.e. the standard one and a modified part. As a result, GWs in this model are not transverse, and their polarization is different from that of General Relativity. The velocity of the GW modified part depends crucially on the parameters characterizing the model, and it mostly results much smaller than the speed of light. Moreover, this investigation allows one to further test the viability of this particular f(R) gravity theory as far as interferometric observations of GWs are concerned.

Publisher

World Scientific Pub Co Pte Lt

Subject

General Physics and Astronomy,Astronomy and Astrophysics,Nuclear and High Energy Physics

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