Statistical description of galactic clusters in Finzi gravity model
  We exploit a new theory of gravity proposed by Finzi, which gives stronger
interaction at large scales, to study the thermodynamic description of galaxy
clusters. We employ a statistical model to deduce various thermodynamics
equations of state. In addition, we analyze the behavior of clustering
parameter in comparison to its standard (Newtonian) counterpart. The general
distribution function and its behavior with varying strength of clustering
parameter are also studied. The possibility of phase transition is also
investigated and observed that a phase transition is possible though
hierarchically.
