A general solution in the Newtonian limit of f(R)- gravity
arXiv:0901.0448 · doi:10.1142/S0217732309030382
Abstract
We show that any analytic -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 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.
5 pages
References in corpus (14)
- Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
- Modified f(R) gravity consistent with realistic cosmology: from matter dominated epoch to dark energy universe
- Extended Theories of Gravity and their Cosmological and Astrophysical Applications
- Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase
- Low surface brightness galaxies rotation curves in the low energy limit of gravity : no need for dark matter?
- Spherically symmetric solutions of modified field equations in f(R) theories of gravity
- Solar System constraints to general f(R) gravity
- The Newtonian Limit of F(R) gravity
- Solar system and equivalence principle constraints on f(R) gravity by chameleon approach
- Dark Energy: the equation of state description versus scalar-tensor or modified gravity
- Solar System tests DO rule out 1/R gravity
- Theory of gravitation theories: a no-progress report
- The Cauchy problem of f(R) gravity
- Breakdown of the initial value formulation of scalar-tensor gravity and its physical meaning
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