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The temperature dependence of equilibrium plasma density | B.V.Vasiliev
; | Date: |
17 Mar 2002 | Journal: | Nuovo Cim. 117B (2003) 1285-1289 | Subject: | astro-ph | Abstract: | 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 $T^{3/2}$. | Source: | arXiv, astro-ph/0203265 | Services: | Forum | Review | PDF | Favorites |
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