Evaporation of strange matter (and similar condensed phases) at high temperatures

Details Evaporation of strange matter (and similar condensed phases) at high temperatures Evaporation of strange matter (and similar condensed phases) at high temperatures

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvd..39.1233a&link_type=abstract

, Volume 39, Issue 4, 15 February 1989, pp.1233-1234

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51

Particle-Theory And Field-Theory Models Of The Early Universe, Nuclear Matter, Origin, Formation, And Abundances Of The Elements

Scientific paper

Strange matter is a form of quark matter that has been conjectured to be stable at zero temperature. If heated to a temperature T>=2 MeV, a strange-matter lump evaporates nucleons from its surface. We show that at higher temperatures (T>=20 MeV), strange matter boils, with bubbles of hadronic gas forming and growing throughout the interior. Strange matter, or any other phase which resembles strange matter, could not have survived this process in the early Universe.

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