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Exploring the Nature of Gravity

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arxiv 1602.01474 v2 pith:CGMYILB4 submitted 2016-02-03 gr-qc astro-ph.COhep-th

classification gr-qcastro-ph.COhep-th
keywords spacetimefieldgravityremainshouldatomsconstantcontributed
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abstract

I clarify the differences between various approaches in the literature which attempt to link gravity and thermodynamics. I then describe a new perspective based on the following features: (1) As in the case of any other matter field, the gravitational field equations should also remain unchanged if a constant is added to the Lagrangian; in other words, the field equations of gravity should remain invariant under the transformation $T^a_b \to T^a_b + \delta^a_b $(constant). (2) Each event of spacetime has a certain number ($f$) of microscopic degrees of freedom (`atoms of spacetime'). This quantity $f$ is proportional to the area measure of an equi-geodesic surface, centered at that event, when the geodesic distance tends to zero. The spacetime should have a zero-point length in order for $f$ to remain finite. (3) The dynamics is determined by extremizing the heat density at all events of the spacetime. The heat density is the sum of a part contributed by matter and a part contributed by the atoms of spacetime, with the latter being $L_P^{-4} f$. The implications of this approach are discussed.

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Cited by 1 Pith paper

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  1. Is The Internal Entropy of F(R)-Gravity Really An Entropy?

    gr-qc 2024-11 reject novelty 5.0 of 10

    A combined Padmanabhan-Hammad entropy functional for F(R)-gravity yields an internal entropy whose derivative structure disagrees with previous derivations, hinting that the internal entropy may actually be a pressure.

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