Spin-dependent particle creation densities, greybody factors, absorption cross sections, and evaporation lifetimes are computed for scalar, vector, tensor, and spinorial modes around black holes in f(R,T) gravity.
There are no quantum corrections to the hawking temperature via tunneling from a fixed background,
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Spin effects on particle creation and evaporation in $f(R,T)$ gravity
Spin-dependent particle creation densities, greybody factors, absorption cross sections, and evaporation lifetimes are computed for scalar, vector, tensor, and spinorial modes around black holes in f(R,T) gravity.