2004
DOI: 10.1103/physrevc.70.015202
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Chiral symmetry restoration in strange hadronic matter

Abstract: The phase transition of chiral symmetry restoration in strange hadronic matter is studied in the chiral SU(3) quark mean field model. When the baryon density is larger than a critical density ρ c , the minimal energy density of the system occurs at the point where the effective masses of nucleon, Λ or Ξ drop to zero. The physical quantities change discontinuously at this density and the system will be in the phase of chiral symmetry restoration. A rich phase structure of strange hadronic matter with different … Show more

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Cited by 20 publications
(27 citation statements)
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“…Theq 0 τ 0 are chosen from 0.84−1.8 GeV 2 . The suppression factor increases with p T was observed, it is mainly due to the energy dependence of parton energy loss and the less steep initial jet production spectra [44].…”
mentioning
confidence: 95%
“…Theq 0 τ 0 are chosen from 0.84−1.8 GeV 2 . The suppression factor increases with p T was observed, it is mainly due to the energy dependence of parton energy loss and the less steep initial jet production spectra [44].…”
mentioning
confidence: 95%
“…Clearly, such vacuum induced Berry phase would have no counterpart in a model constructed by a classical driving field, hence it would be a direct proof of electromagnetic field quantization. The novel work of I. Fuentes-Guridi et al avalanched a series of following papers [15][16][17][18][19][20][21]. In particular, various extensions of Ref.…”
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confidence: 99%
“…In particular, various extensions of Ref. [14] have been addressed, such as; multi-atom (Dicke) systems [17], geometrical quantum computing [18], decohering cavity modes [19], solid state counterparts [20], and multi-level atom situations [21]. Most of these references picture one or another sort of cavity QED scheme, and more importantly the RWA has been imposed in all of them.…”
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confidence: 99%
“…The conclusion being that the medium formed in central Au+Au collisions at RHIC has a high degree of opacity [34]. In addition, theoretical studies suggest that for a given initial density, the R AA (p T ) values are also sensitive to the lifetime (τ ) of dense matter formed in heavy-ion collisions [29]. The solid curves are predictions from Ref.…”
Section: Jet Quenching and Highly Opaque Mediummentioning
confidence: 93%
“…This phenomena is called as the jet quenching in a dense partonic matter [27]. The energy loss by energetic partons traversing the dense medium formed in high-energy heavy-ion collisions is predicted to be proportional to both the initial gluon density [28] and the lifetime of the dense matter [29]. The results on high-p T suppression are usually presented in terms of the nuclear modification factor (R AA ), defined as:…”
Section: Jet Quenching and Highly Opaque Mediummentioning
confidence: 99%