In a 2D CGHS black hole with a linear Horndeski G3 coupling, the derived first-order correction lowers the Hawking temperature as mass decreases, and an assumed resummation leads to a cold remnant with logarithmically growing radiation entropy.
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Anomaly quenching and dynamical cooling of Hawking evaporation in Horndeski gravity
In a 2D CGHS black hole with a linear Horndeski G3 coupling, the derived first-order correction lowers the Hawking temperature as mass decreases, and an assumed resummation leads to a cold remnant with logarithmically growing radiation entropy.