Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-03-17
Nuovo Cim.B117:1285-1289,2003
Astronomy and Astrophysics
Astrophysics
7 pages,1 firure
Scientific paper
Temperature dependence of an electron-nuclear plasma equilibrium density is considered basing on known approaches, which are given in (1)(2). It is shown that at a very high temperature, which is characteristic for a star interior, the equilibrium plasma density is almost constant and equals approximately to $10^{25}$ particles per $cm^3$. At a relatively low temperature, which is characteristic for star surface, the equilibrium plasma density is in several orders lower and depends on temperature as $T^{3/2}$.
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