The cooling processes of brown dwarf stars and giant planets are examined within the framework of degenerate higher-order scalar-tensor theories. The findings confirm previous studies that modified gravity has the most pronounced effect on the age of substellar objects.
Cooling processes of brown dwarf stars and giant planets are studied in the framework of degenerate higher-order scalar-tensor theories. We confirm the previous results in the field that the effect of modified gravity on substellar objects' age is pronounced the most.
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