Nonlocality effects on color spin locking condensates

被引:22
作者
Aguilera, D. N.
Blaschke, D.
Grigorian, H.
Scoccola, N. N.
机构
[1] Univ Alicante, Dept Appl Phys, E-03080 Alicante, Spain
[2] Univ Wroclaw, Inst Theoret Phys, PL-50204 Wroclaw, Poland
[3] Univ Rostock, Inst Phys, D-18051 Rostock, Germany
[4] Joint Inst Nucl Res, Bogoliubov Lab Theoret Phys, Dubna 141980, Russia
[5] Joint Inst Nucl Res, Informat Technol Lab, Dubna 141980, Russia
[6] Yerevan State Univ, Dept Phys, Yerevan 375047, Armenia
[7] Comis Nacl Energia Atom, Dept Phys, RA-1429 Buenos Aires, DF, Argentina
[8] Univ Favaloro, RA-1078 Buenos Aires, DF, Argentina
[9] Consejo Nacl Invest Cient & Tecn, RA-1033 Buenos Aires, DF, Argentina
来源
PHYSICAL REVIEW D | 2006年 / 74卷 / 11期
关键词
D O I
10.1103/PhysRevD.74.114005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider the color spin locking (CSL) phase of two-flavor quark matter at zero temperature for nonlocal instantaneous separable interactions. We employ a Lorentzian-type form factor allowing a parametric interpolation between the sharp [Nambu-Jona-Lasinio (NJL) model] and very smooth (e.g. Gaussian) cutoff models for systematic studies of the influence on the CSL condensate the deviation from the NJL model entails. This smoothing of the NJL model form factor shows advantageous features for the phenomenology of compact stars: (i) a lowering of the critical chemical potential for the onset of the chiral phase transition as a prerequisite for stability of hybrid stars with extended quark matter cores and (ii) a reduction of the smallest pairing gap to the order of 100 keV, being in the range of values interesting for phenomenological studies of hybrid star cooling evolution.
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页数:7
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