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- W2094715503 abstract "Density and temperature conditions in many stellar core (like the solar core) imply the presence of nonideal plasma effects with memory and long-range interactions between particles. This aspect suggests the possibility that the stellar core could not be in a global thermodynamical equilibrium but satisfies the conditions of a metastable state with a stationary (nonextensive) power law distribution function among ions. The order of magnitude of the deviation from the standard Maxwell-Boltzmann distribution can be derived microscopically by considering the presence of random electrical microfields in the stellar plasma. We show that such a nonextensive statistical effect can be very relevant in many nuclear astrophysical problems." @default.
- W2094715503 created "2016-06-24" @default.
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- W2094715503 date "2005-04-01" @default.
- W2094715503 modified "2023-09-24" @default.
- W2094715503 title "NONEXTENSIVE STATISTICAL EFFECTS ON NUCLEAR ASTROPHYSICS AND MANY-BODY PROBLEMS" @default.
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- W2094715503 doi "https://doi.org/10.1142/9789812701985_0011" @default.
- W2094715503 hasPublicationYear "2005" @default.
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