@article{RCP25_1972__14__A3_0,
author = {Thirring, Walter},
title = {Free Energy of Gravitating Fermions},
journal = {Les rencontres physiciens-math\'ematiciens de Strasbourg -RCP25},
volume = {14},
year = {1972},
pages = {1-26},
language = {en},
url = {http://dml.mathdoc.fr/item/RCP25_1972__14__A3_0}
}
Thirring, Walter. Free Energy of Gravitating Fermions. Les rencontres physiciens-mathématiciens de Strasbourg -RCP25, Tome 14 (1972) pp. 1-26. http://gdmltest.u-ga.fr/item/RCP25_1972__14__A3_0/
1) in Statistical Physics, Phase transitions and Superfluidity, 1966 Brandeis University Suramer School in Theoretical Physics, lecture notes ;
and , J.Math.Phys. 8 (1967) 423 | MR 2408896 | Zbl 0948.81665
2) and , Phys. Rev. Letter 22. (1969) 631
3) , J.Math.Phys. 10 (1969) 806.
4) , Z. Phys. 235 (1970) 339;
and , Annals of Physics 63 (1971).
5) and , CEEN preprint TH. 1338 (1971). | MR 1552579
6) A typical "neutron star" of particles at a temperature of 5 MeV and enclosed into a sphere of 100 km radius corresponds to with , , and . Since , and are of order unity (if measured in their natural units) and since is sufficiently large, we will describe the above "neutron star" by the limit . For , and km we would have reached the same accuracy for .
7) , Perturbation theory for linear operators, Berlin, Springer 1966. There the infinite volume case is studied, however, the result also holds for finite volume. | Zbl 0836.47009
8) , Analyticity of the partition function for finite quantum Systems, CERN preprint TH. 1299 (1971). | MR 303887 | Zbl 0218.47017
9) , Eléments d'analyse, Tome I, Paris, Gauthier-Villars 1969. | Zbl 0326.22001
10) , J.Math.Phys. 10 (1969) 1123. Again this estimate for infinité volume is a fortiori also valid for finite volume. | MR 246593
11) , Statistical mechanics - rigorous results, New York, Benjamin 1961. | MR 289084 | Zbl 0177.57301
12) , Physica 32 (1966) 933. | MR 207351
13) , Commun.Math.Phys. 8 (1968) 26. | MR 225552 | Zbl 0155.32701