2000
DOI: 10.1103/physrevc.62.025801
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Thermodynamics, strange quark matter, and strange stars

Abstract: Because of the mass density-dependence, an extra term should be added to the expression of pressure. However, it should not appear in that of energy according to both the general ensemble theory and basic thermodynamic principle. We give a detail derivation of the thermodynamics with density-dependent particle masses. With our recently determined quark mass scaling, we study strange quark matter in this new thermodynamic treatment, which still indicates a possible absolute stability as previously found. Howeve… Show more

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Cited by 139 publications
(162 citation statements)
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“…many physical properties of strange quark matter [12,13,14,15,16,17,18,19,20,21,22,23,24,25] and strange quark star [26,27] have been studied, and the results are in good agreement with those given by MIT bag model [28].…”
Section: Introductionsupporting
confidence: 75%
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“…many physical properties of strange quark matter [12,13,14,15,16,17,18,19,20,21,22,23,24,25] and strange quark star [26,27] have been studied, and the results are in good agreement with those given by MIT bag model [28].…”
Section: Introductionsupporting
confidence: 75%
“…[15] and the treatment in Ref. [17], respectively. The tendencies of these curves are similar at large energy density region, but at small energy density region, different treatments have quite different behaviors.…”
Section: Summary and Discussionmentioning
confidence: 99%
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