  We present an investigation on thermodynamics of two different types of black
holes viz. Kiselev black hole (asymptotically flat) and Taub-NUT
(non-asymptotically flat) black hole. We compute the thermodynamic variables
like black hole's Hawking temperature, entropy at the black hole's event
horizon. Further we derive the heat capacity and examine it to study the
thermal stability of the black holes. We also calculate the rate of emission
assuming the black holes radiate energy in terms of photons by tunneling. We
represent all the parameters including the rate of emission of the black holes
graphically and interpret them physically. We depict a comparative study of
thermodynamics between the afroesaid types of black holes. Here we find the
existence of a transition of phase. Finally, we obtain the quantum-corrected
thermodynamics on the basis of general uncertainty principle and it is seen
from the quantum-corrected entropy that it contains the logarithmic term. We
offer comparative studies on joint effect of generalised uncertainty principle
parameter $\alpha$ along with the concerned black holes' parameters on the
thermodynamics.
