Finite temperature makes theoretical white dwarf models in scalar-tensor gravity larger at the same mass, creating a degeneracy with modified gravity signatures.
This frame is obtained from the physical Jordan frame by a conformal transformation of the metric tensor, written as gµν = A2( ˜ϕ)˜gµν and scalar field redefinition
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Temperature effects on white dwarfs in modified gravity
Finite temperature makes theoretical white dwarf models in scalar-tensor gravity larger at the same mass, creating a degeneracy with modified gravity signatures.