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Invariant quantities of Scalar-Tensor Theories for stellar structure
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Invariant quantities of Scalar-Tensor Theories for stellar structure
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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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Cited by 1 Pith paper
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Einstein crystals in Snyder and Snyder-de Sitter noncommutative backgrounds
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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