Interacting THDE in linear and quadratic f(R,T) gravity reaches the Lambda CDM fixed point and has its parameters constrained by chi-squared fits to observational data.
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Cosmology of the interacting Tsallis holographic dark energy in $f(R,T)$ gravity framework
Interacting THDE in linear and quadratic f(R,T) gravity reaches the Lambda CDM fixed point and has its parameters constrained by chi-squared fits to observational data.