Galactic Clustering Under Power-law Modified Newtonian Potential
  We estimate galaxy clustering under a modified gravitational potential. In
particular, the modifications in gravitational potential energy occur due to a
power-law and cosmological constant terms. We derive a canonical partition
function for the system of galaxies interacting under such a modified
gravitational potential. Moreover, we compute various thermodynamical equation
of states for the system. We do comparative analysis in order to emphasize the
effect of corrections on thermodynamics of the system. Interestingly, the
modifications in thermodynamical quantities are embedded in clustering
parameter only.
