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Invariant quantities of Scalar-Tensor Theories for stellar structure

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arxiv 2103.06601 v3 pith:L3EE2J2D submitted 2021-03-11 gr-qc

Aleksander Kozak , Aneta Wojnar This is my paper · ORCID
classification gr-qc
keywords scalar-tensorequationsstellarstructuretheoriesallowingclassequilibrium
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We present the relativistic hydrostatic equilibrium equations for a wide class of gravitational theories possessing a scalar-tensor representation. It turns out that the stellar structure equations can be written with respect to the scalar-tensor invariants, allowing to interpret their physical role.

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  1. Einstein crystals in Snyder and Snyder-de Sitter noncommutative backgrounds

    gr-qc 2026-07 conditional novelty 4.0 of 10

    Snyder and Snyder-de Sitter noncommutativity shifts the Einstein-crystal partition function, internal energy, and specific heat, yielding weak self-consistency bounds on the deformation parameter zeta.

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