Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-07-16
Nucl.Phys.B711:604-620,2005
Astronomy and Astrophysics
Astrophysics
LaTex 12 pages, 1 figure .ps
Scientific paper
10.1016/j.nuclphysb.2004.12.022
We develop the cluster expansion and the Mayer expansion for the self-gravitating thermal gas and prove the existence and stability of the thermodynamic limit N, V to infty with N/V^{1/3} fixed. The essential (dimensionless) variable is here eta = [G m^2 N]/[V^{1/3} T] (which is kept fixed in the thermodynamic limit). We succeed in this way to obtain the expansion of the grand canonical partition function in powers of the fugacity. The corresponding cluster coefficients behave in the thermodynamic limit as [eta/N]^{j-1} c_j where c_j are pure numbers. They are expressed as integrals associated to tree cluster diagrams. A bilinear recurrence relation for the coefficients c_j is obtained from the mean field equations in the Abel form. In this way the large j behaviour of the c_j is calculated. This large j behaviour provides the position of the nearest singularity which corresponds to the critical point (collapse) of the self-gravitating gas in the grand canonical ensemble. Finally, we discuss why other attempts to define a thermodynamic limit for the self-gravitating gas fail.
de Vega Hector J.
Sánchez Nadia
No associations
LandOfFree
The Cluster Expansion for the Self-Gravitating gas and the Thermodynamic Limit does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Cluster Expansion for the Self-Gravitating gas and the Thermodynamic Limit, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Cluster Expansion for the Self-Gravitating gas and the Thermodynamic Limit will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-206679