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Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-54438

Näf, J; Jetzer, P (2011). Gravitational radiation in quadratic f(R) gravity. Physical Review D, 84(2):024027.

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Abstract

We investigate the gravitational radiation emitted by an isolated system for gravity theories with Lagrange density f(R)=R+aR2. As a formal result, we obtain leading order corrections to the quadrupole formula in general relativity. We make use of the analogy of f(R) theories with scalar-tensor theories, which in contrast to general relativity feature an additional scalar degree of freedom. Unlike general relativity, where the leading order gravitational radiation is produced by quadrupole moments, the additional degree of freedom predicts gravitational radiation of all multipoles, in particular, monopoles and dipoles, as this is the case for the most alternative gravity theories known today. An application to a hypothetical binary pulsar moving in a circular orbit yields the rough limit a≲1.7×1017m2 by constraining the dipole power to account at most for 1% of the quadrupole power as predicted by general relativity.

Other titles:On gravitational radiation in quadratic $f(R)$ gravity
Item Type:Journal Article, refereed, original work
Communities & Collections:07 Faculty of Science > Institute of Theoretical Physics
DDC:530 Physics
Language:English
Date:July 2011
Deposited On:19 Feb 2012 11:28
Last Modified:21 Apr 2014 09:15
Publisher:American Physical Society
ISSN:1550-7998 (P) 1089-4918 (E)
Publisher DOI:10.1103/PhysRevD.84.024027
Related URLs:http://arxiv.org/abs/1104.2200
Citations:Web of Science®. Times Cited: 7
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