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Galaxies 2014, 2(4), 520-576;

Self-Gravitating Systems in Extended Gravity

Dipartimento di Ingegneria, Università del Sannio, Palazzo Dell'Aquila Bosco Lucarelli, Corso Garibaldi, 107-82100 Benevento, Italy
Dipartimento di Fisica, Università di Napoli "Federico II", Complesso Universitario di Monte Sant'Angelo, Edificio G, Via Cinthia, I-80126 Napoli, Italy
INFN Sezione di Napoli, Complesso Universitario di Monte Sant' Angelo, Ed. G, Via Cinthia, I-80126 Napoli, Italy
Gran Sasso Science Institute (INFN), Via F. Crispi 7, I-67100 L' Aquila, Italy
Authors to whom correspondence should be addressed.
Received: 21 July 2014 / Revised: 10 November 2014 / Accepted: 14 November 2014 / Published: 4 December 2014
(This article belongs to the Special Issue Beyond Standard Gravity and Cosmology)
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Starting from the weak field limit, we discuss astrophysical applications of Extended Theories of Gravity where higher order curvature invariants and scalar fields are considered by generalizing the Hilbert-Einstein action linear in the Ricci curvature scalar R. Results are compared to General Relativity in the hypothesis that Dark Matter contributions to the dynamics can be neglected thanks to modified gravity. In particular, we consider stellar hydrostatic equilibrium, galactic rotation curves, and gravitational lensing. Finally, we discuss the weak field limit in the Jordan and Einstein frames pointing out how effective quantities, as gravitational potentials, transform from one frame to the other and the interpretation of results can completely change accordingly. View Full-Text
Keywords: Alternative Theories of Gravity; weak field limit; spherical symmetry; self-gravitating systems; conformal transformations Alternative Theories of Gravity; weak field limit; spherical symmetry; self-gravitating systems; conformal transformations

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Stabile, A.; Capozziello, S. Self-Gravitating Systems in Extended Gravity. Galaxies 2014, 2, 520-576.

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