Free Energy of Gravitating Fermions

Thirring, Walter

Thirring, Walter

Les rencontres physiciens-mathématiciens de Strasbourg -RCP25, Conférences de J. Bros, P. Schapira et W. Thirring et un texte de R. Gérard et A.H.M. Levelt, Tome 14 (1972), Exposé no. 3, 26 p.

EuDML

@article{RCP25_1972__14__A3_0,
     author = {Thirring, Walter},
     title = {Free {Energy} of {Gravitating} {Fermions}},
     journal = {Les rencontres physiciens-math\'ematiciens de Strasbourg -RCP25},
     note = {talk:3},
     pages = {1--26},
     publisher = {Institut de Recherche Math\'ematique Avanc\'ee - Universit\'e Louis Pasteur},
     volume = {14},
     year = {1972},
     language = {en},
     url = {http://archive.numdam.org/item/RCP25_1972__14__A3_0/}
}

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VL  - 14
PB  - Institut de Recherche Mathématique Avancée - Université Louis Pasteur
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Thirring, Walter. Free Energy of Gravitating Fermions. Les rencontres physiciens-mathématiciens de Strasbourg -RCP25, Conférences de J. Bros, P. Schapira et W. Thirring et un texte de R. Gérard et A.H.M. Levelt, Tome 14 (1972), Exposé no. 3, 26 p. http://archive.numdam.org/item/RCP25_1972__14__A3_0/

Bibliographie
Cité par

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6) A typical "neutron star" of $10^{57}$ particles at a temperature of 5 MeV and enclosed into a sphere of 100 km radius corresponds to $(λ N, λ^{- 4 / 3} β, λ^{- 1 / 3} R)$ with $N = 1$ , $β = 60 ℏ^{2} κ^{- 2} m_{N}^{- 5}$ , $R = 29 ℏ^{2} κ^{- 1} m_{N}^{- 1}$ and $λ = 10^{57}$ . Since $N$ , $S$ and $R$ are of order unity (if measured in their natural units) and since $λ = 10^{57}$ is sufficiently large, we will describe the above "neutron star" by the limit $λ \to \infty$ . For $N = 1057$ , $β = {(5 M e V)}^{- 1}$ and $R = 100$ km we would have reached the same accuracy for $λ = 1$ .

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