Amorphous glassy plasma in dense stellar matter

Details Amorphous glassy plasma in dense stellar matter Amorphous glassy plasma in dense stellar matter

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...265l..83i&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 265, Feb. 15, 1983, p. L83-L86.

Astronomy and Astrophysics

Astrophysics

26

Amorphous Materials, Astrophysics, Dense Plasmas, Neutron Stars, Metastable State, Transport Properties, White Dwarf Stars

Scientific paper

It is shown through microscopic analyses that the plasma fluid below the Wigner transition temperature may form an amorphous glassy state, rather than a crystalline state, and that the magnitudes of transport coefficients differ substantially in those two states. The lifetime of the metastable glassy state is estimated to be significantly large; the possibility of matter being in a glassy state should be seriously taken into account in the analyses of the physical processes in the neutron stars and in the white dwarfs.

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