Based on fundamental concepts of thermodynamics we examine phase transitions
in black holes defined in Anti-de Sitter (AdS) spaces. The method is in line
with that used a long ago to understand the liquid-vapour phase transition
where the first order derivatives of Gibbs potential are discontinuous and
Clausius-Clapeyron equation is satisfied. The idea here is to consider the AdS
black holes as grand-canonical ensembles and study phase transition defined by
the discontinuity of second order derivatives of Gibbs potential. We
analytically check that this phase transition between the smaller' and larger’ mass black holes obey Ehrenfest relations defined at the critical
point and hence confirm a second order phase transition. This include both the
rotating and charged black holes in Einstein gravity.

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