Cooling process of substellar objects in scalar-tensor gravity

Abstract

Cooling processes of brown dwarf stars and giant planets are studied in the framework of DHOST theories. We confirm the previous results in the field that the effect of modified gravity on substellar objects' age is pronounced the most.

17 pages, 8 figures, matching the version to be published in PRD

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Cited by in corpus (5)

• Fermi equation of state with finite temperature corrections in quantum space-times approach: Snyder model vs GUP case
• Constraining Snyder and GUP models with low-mass stars
• Planetary seismology as a test of modified gravity proposals
• Cooling Process of White Dwarf Stars in Palatini $f(R)$ Gravity
• Crystallized white dwarf stars in scalar-tensor gravity