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Beyond Einstein GravityWeak-field limit

Beyond Einstein Gravity: Weak-field limit [Astrophysical applications of ETGs include the possibility of replacing dark matter in galaxy and clusters with modifications of gravity, the weak-field (Newtonian and post-Newtonian) limit, and gravitational waves. Dark matter at galactic and cluster scales is traditionally included in the realm of cosmology and is discussed in Chap. 7. Here we focus on the weak-field limit of metric f(R) gravity, referring the reader to well known sources for other ETGs. We then discuss gravitational waves in ETGs.] http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png

Beyond Einstein GravityWeak-field limit

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Publisher
Springer Netherlands
Copyright
© Springer Science+Business Media B.V. 2011
ISBN
978-94-007-0164-9
Pages
165 –208
DOI
10.1007/978-94-007-0165-6_5
Publisher site
See Chapter on Publisher Site

Abstract

[Astrophysical applications of ETGs include the possibility of replacing dark matter in galaxy and clusters with modifications of gravity, the weak-field (Newtonian and post-Newtonian) limit, and gravitational waves. Dark matter at galactic and cluster scales is traditionally included in the realm of cosmology and is discussed in Chap. 7. Here we focus on the weak-field limit of metric f(R) gravity, referring the reader to well known sources for other ETGs. We then discuss gravitational waves in ETGs.]

Published: Sep 30, 2010

Keywords: Dark Matter; Gravitational Wave; Gravitational Potential; Ricci Scalar; Einstein Frame

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