A general solution in the Newtonian limit of f(R)- gravity
| dc.creator | Capozziello, S. | |
| dc.creator | Stabile, A. | |
| dc.creator | Troisi, A. | |
| dc.date | 2009-01-05 | |
| dc.date.accessioned | 2026-07-07T13:06:14Z | |
| dc.date.available | 2026-07-07T13:06:14Z | |
| dc.description | We show that any analytic $f(R)$-gravity model, in the metric approach, presents a weak field limit where the standard Newtonian potential is corrected by a Yukawa-like term. This general result has never been pointed out but often derived for some particular theories. This means that only $f(R)=R$ allows to recover the standard Newton potential while this is not the case for other relativistic theories of gravity. Some considerations on the physical consequences of such a general solution are addressed. | |
| dc.description | 5 pages | |
| dc.identifier | https://arxiv.org/abs/0901.0448 | |
| dc.identifier | http://arxiv.org/abs/0901.0448 | |
| dc.identifier | Mod.Phys.Lett.A24:659-665,2009 | |
| dc.identifier | doi:10.1142/S0217732309030382 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/227714 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | Cosmology and Nongalactic Astrophysics | |
| dc.title | A general solution in the Newtonian limit of f(R)- gravity | |
| dc.type | text |