Gravitational Clustering of Galaxies in an Expanding Universe

Details Gravitational Clustering of Galaxies in an Expanding Universe Gravitational Clustering of Galaxies in an Expanding Universe

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006japa...27..373i&link_type=abstract

Journal of Astrophysics and Astronomy, vol. 27, no.4, p. 373-379.

Astronomy and Astrophysics

Astrophysics

Gravitational Clustering, Thermodynamics, Correlation Function: Structure Of Universe

Scientific paper

We inquire the phenomena of clustering of galaxies in an expanding universe from a theoretical point of view on the basis of thermodynamics and correlation functions. The partial differential equation is developed both for the point mass and extended mass structures of a two-point correlation function by using thermodynamic equations in combination with the equation of state taking gravitational interaction between particles into consideration. The unique solution physically satisfies a set of boundary conditions for correlated systems and provides a new insight into the gravitational clustering problem.

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