Possibility of amorphous glassy state in astrophysical dense plasmas

Details Possibility of amorphous glassy state in astrophysical dense plasmas Possibility of amorphous glassy state in astrophysical dense plasmas

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982phst....2..560i&link_type=abstract

(International Conference on Plasma Physics, Goteborg, Sweden, June 9-15, 1982) Physica Scripta (ISSN 0031-8949), vol. T2:2, 198

Physics

Plasma Physics

Amorphous Materials, Cold Plasmas, Cosmic Plasma, Metastable State, Microscopy, Monte Carlo Method, Stellar Models

Scientific paper

Microscopic analysis on the basis of the improved hypernetted chain equations shows that the plasma fluid may form a metastable glassy state in the supercooled domain over a wide range of the plasma parameter. Transition time from the metastble state to the crystalline state is estimated to be sufficiently large so that the possibility of the glassy state has an astrophysical relevance.

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