High-spin states in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Gd</mml:mi><mml:mprescripts /><mml:none /><mml:mrow><mml:mn>152</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>

Wang, S.; Hua, H.; Meng, J.; Li, Z. H.; Zhang, S. Q.; Fang, Xu; Liu, H. L.; Ye, Y. L.; Jiang, D. X.; Zheng, Tao; Wang, Q. J.; Chen, Z. Q.; Wu, Chen; Zhang, G. L.; Pang, D. Y.; Wang, J.; Lou, J. L.; Guo, Boling; Gao, Jin; Zhou, Shan‐Gui; Zhu, Long; Wu, X. G.; Li, G. S.; Wen, S. X.; He, C. Y.; Cui, X. Z.; Liu, Y.

doi:10.1103/physrevc.72.024317

Cited by 25 publications

(17 citation statements)

References 15 publications

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“…Further, the variation of effective magnetic moments of baryons as a function of temperature is negligible for nuclear matter density higher than 4ρ 0 . This indicates second order phase transition at higher densities [69].…”

Section: Discussionmentioning

confidence: 74%

Magnetic moments of octet baryons in hot and dense nuclear matter

2017

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We have calculated the in-medium magnetic moments of octet baryons in the presence of hot and dense symmetric nuclear matter. Effective magnetic moments of baryons have been derived from medium modified quark masses within chiral SU(3) quark mean field model. Further, for better insight of medium modification of baryonic magnetic moments, we have considered the explicit contributions from the valence quarks, sea quarks as well as sea orbital angular momentum of sea quarks. These effects have been successful in giving the description of baryonic magnetic moments in vacuum. The magnetic moments of baryons are found to vary significantly as a function of density of nuclear medium. * Electronic address:

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Section: Discussionmentioning

confidence: 74%

Magnetic moments of octet baryons in hot and dense nuclear matter

2017

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“…Many observables are responsible for learning properties of the nuclear matter, such as thermodynamic variables and transport coefficients. A core observable is the nuclear temperature which has been extensively investigated by theories and experiments with different approaches [3] like double ratio of isotopic yield [4,5], kinetic approaches [6][7][8][9][10][11][12], isospin thermometer [13,14], double Fermi-sphere [15], classical fluctuation method [16] and quantum fluctuation method [17,18]. Nevertheless, there is no consensus on the best thermometer from the nuclear system [3].…”

Section: Introductionmentioning

confidence: 99%

Thermal and transport properties in central heavy-ion reactions around a few hundred MeV/nucleon

Deng

Veselský

2016

Phys. Rev. C

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Thermalization process of nuclear matter in central fireball region of heavy-ion collisions is investigated by employing an extension model of Boltzmann-Uehling-Uhlenbeck, namely the Van der Waals Boltzmann-Uehling-Uhlenbeck (VdWBUU) model. Temperature (T ) is extracted by the quantum Fermion fluctuation approach and other thermodynamic quantities, such as density (ρ), entropy density (s), shear viscosity (η), isospin diffusivity (DI ) and heat conductivity (κ), are also deduced. The liquid-like and gas-like phase signs are discussed through the behavior of shear viscosity during heavy-ion collisions process with the VdWBUU model.

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“…This is because of the reduced compressibility of nuclear matter at finite temperature as compared to that at zero temperature. Furthermore, the variation of effective magnetic moments of baryons as a function of temperature is negligible for nuclear matter density higher than 4ρ 0 indicating second order phase transition at higher densities [82]. The present approach along with Polyakov loop corrections (which becomes important near critical temperature) can be used to study the phenomena like chiral restoration, deconfinement phase transition and inverse magnetic catalysis [97][98][99][100].…”

Section: Discussionmentioning

confidence: 99%

Octet baryon masses and magnetic moments in hot and dense isospin asymmetric nuclear matter

2019

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Medium modification of the magnetic moments of octet baryons in the isospin asymmetric nuclear medium at finite temperature has been calculated using medium modified quark and baryon masses derived in chiral SU(3) quark mean field model. The magnetic moments of baryons are found to vary significantly as a function of density of nuclear medium as well as with the increase in isospin asymmetry of the medium. The rise of temperature is found to decrease the effect of isospin asymmetry on masses and magnetic moments of baryons. The results of present investigation may be helpful to understand the experimentally observed values of octet baryon magnetic moments at different experimental facilities.

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High-spin states inGd152

Cited by 25 publications

References 15 publications

Magnetic moments of octet baryons in hot and dense nuclear matter

Magnetic moments of octet baryons in hot and dense nuclear matter

Thermal and transport properties in central heavy-ion reactions around a few hundred MeV/nucleon

Octet baryon masses and magnetic moments in hot and dense isospin asymmetric nuclear matter

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