The Static Gravitational Field of a Spherically Symmetric Body
M. Novello, L. R. Freitas, V. A. De Lorenci

TL;DR
This paper explores a gravity theory satisfying the Einstein Equivalence Principle for matter but not for gravitational energy, deriving a static spherically symmetric gravitational field with PPN parameters matching GR, but differing in gravitational wave velocity.
Contribution
It presents a field theory of gravity that aligns with observations for matter interactions and reproduces GR's PPN parameters, while proposing a different gravitational wave velocity.
Findings
PPN parameters match those of GR: α=β=γ=1
Gravitational field of a static sphere derived in this theory
Main difference from GR is in gravitational wave velocity
Abstract
We continue here the exam \cite{LuMa} of a theory of gravity that satisfies the Einstein Equivalence Principle (EEP) for any kind of matter/energy, except for the gravitational energy. This is part of a research program that intends to re-examine the standard Feynman-Deser approach of field theoretical derivation of Einstein\rq s General Relativity. The hypothesis implicit in such precedent derivations \cite{Feynman} \cite{Deser} concerns the universality of gravity interaction. Although there is a strong observational basis supporting the universality of matter to gravity interaction, there is not an equivalent situation that supports the hypothesis that gravity interacts with gravity as any other form of non-gravitational energy. We analyse here a kind of gravity-gravity interaction distinct from GR but, as we shall see, that conforms with the actual status of observation. We exhibit…
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Taxonomy
TopicsCosmology and Gravitation Theories · Earth Systems and Cosmic Evolution · Relativity and Gravitational Theory
