2016
DOI: 10.1016/j.nuclphysa.2016.04.020
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On the anomalous mass defect of strange stars in the Field Correlator Method

Abstract: We investigate general aspects of the mass defects of strange stars in the context of the Field Correlator Method, without magnetic field. The main parameters of the model that enter the corresponding nonperturbative equation of state of the quark gluon plasma are the gluon condensate G 2 and the large distance static QQ potential V 1 .We calculate mass defects of stellar configurations in the central density range 11 < log ρ c < 18. In general, the mass defects are strongly dependent on the model parameters. … Show more

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Cited by 2 publications
(4 citation statements)
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“…4 in Ref. [16]). Dotted lines: ∆ 2 M at the point 3 of the low stellar masses ranging from M/M ⊙ ≃ 0.…”
Section: Figure Captionmentioning
confidence: 91%
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“…4 in Ref. [16]). Dotted lines: ∆ 2 M at the point 3 of the low stellar masses ranging from M/M ⊙ ≃ 0.…”
Section: Figure Captionmentioning
confidence: 91%
“…Let us summarize the main equations concerning the FCM thermodynamics of quarks (see Refs. [16,18,19] for a more detailed description). The main parameters of the nonperturbative equation of state are the large distance static q q potential V 1 and the gluon condensate G 2 .…”
Section: Temperaturementioning
confidence: 99%
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