Metastability of electron-nuclear astrophysical plasmas: motivations, signals and conditions

DOI10.1007/S10509-006-9200-2zbMath1108.85002OpenAlexW2068878109MaRDI QIDQ863249

A. Lavagno, Piero Quarati

Publication date: 25 January 2007

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-006-9200-2

zbMATH Keywords

atomic processes in plasmasatomic radiative processes in electron-nuclear plasmasion distributionsJupiter's energy productionlithium abundanceneutrino fluxesnuclear fusion reactionsresonant nuclear reactionsstellar plasmas

Mathematics Subject Classification ID

Electromagnetic fields in general relativity and gravitational theory (83C50) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (1)

Nonextensivity and the power-law distributions for the systems with self-gravitating long-range interactions

Cites Work

• Unnamed Item
• On thermonuclear reaction rates
• What should a statistical mechanics satisfy to reflect nature?
• Solar structure in terms of Gauss' hypergeometric function
• Nonextensivity in nonequilibrium plasma systems with Coulombian long-range interactions
• Metastable and stable equilibrium states of stellar electron-nuclear plasmas
• Self-gravitating stellar systems and non-extensive thermostatistics
• Superstatistics
• Deuterium burning in Jupiter interior

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