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相关论文: Neutral color-spin locking phase in neutron stars

200 篇论文

We present results of a microscopic calculation using NJL-type model of possible spin-one pairings in two flavor quark matter for applications in compact star phenomenology. We focus on the color-spin locking phase (CSL) in which all quarks…

高能物理 - 唯象学 · 物理学 2008-11-26 D. N. Aguilera

We study a spin-1 single flavor color superconducting phase which results from a color-spin locking (CSL) interaction in two-flavor quark matter. This phase is particularly interesting for compact star cooling applications since the CSL…

高能物理 - 唯象学 · 物理学 2009-11-11 D. N. Aguilera , D. Blaschke , M. Buballa , V. L. Yudichev

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…

高能物理 - 唯象学 · 物理学 2008-11-26 D. N. Aguilera , D. Blaschke , H. Grigorian , N. N. Scoccola

We calculate the phase diagram of color and electrically neutral quark matter in weak equilibrium using the NJL model at high baryon densities. We extend previous analyses by taking into account the possibility of formation of pseudoscalar…

高能物理 - 唯象学 · 物理学 2007-05-23 Harmen J. Warringa

We show that within a recently developed nonlocal chiral quark model the critical density for a phase transition to color superconducting quark matter under neutron star conditions can be low enough for these phases to occur in compact star…

高能物理 - 唯象学 · 物理学 2009-09-29 David Blaschke , Dmitri N. Voskresensky , Hovik Grigorian

The possibility of compact stars as hideouts for color-spin-locked (CSL) quark matter (QM) is investigated in both MIT bag model and Nambu-Jona-Lasinio (NJL) model. Within the framework of NJL model, the idea of absolutely stable quark…

高能物理 - 唯象学 · 物理学 2025-09-16 Xin-Ying Song

We analyze the phases of dense quark matter at nonzero quark masses. We map out the phase diagrams for charged quark matter as well as charge neutral matter containing leptons. We find that in Color Flavor Locked (CFL) quark matter, the…

高能物理 - 唯象学 · 物理学 2009-11-07 David B. Kaplan , Sanjay Reddy

We present results for neutrino emissivities and bulk viscosities of a two-flavor color superconducting quark matter phase with isotropic color-spin-locked (iso-CSL) single-flavor pairing which fulfill the constraints on quark matter…

高能物理 - 唯象学 · 物理学 2008-11-26 David B. Blaschke , Jens Berdermann

We suggest a scenario where the three light quark flavors are sequentially deconfined under increasing pressure in cold asymmetric nuclear matter as e.g. in neutron stars. The basis for our analysis is a chiral quark matter model of…

天体物理学 · 物理学 2009-11-13 David Blaschke , Fredrik Sandin , Thomas Klahn , Jens Berdermann

We show that within a recently developed nonlocal, chiral quark model the critical densities for a phase transition to color superconducting quark matter under neutron star conditions can be low enough that these phases occur in compact…

天体物理学 · 物理学 2017-08-23 D. Blaschke , D. N. Voskresensky , H. Grigorian

We study the influence of nonlocality in the interaction on two spin one pairing patterns of two-flavor quark matter: the anisotropic blue color paring besides the usual two color superconducting matter (2SCb), in which red and green colors…

高能物理 - 唯象学 · 物理学 2008-11-26 D. N. Aguilera , D. B. Blaschke

We show that within a recently developed nonlocal chiral quark model the critical density for a phase transition to color superconducting quark matter under neutron star conditions can be low enough for these phases to occur in compact star…

天体物理学 · 物理学 2009-11-10 Hovik Grigorian , David Blaschke , Dmitri Voskresensky

The gapless color-flavor locked (gCFL) phase is the second-densest phase of matter in the QCD phase diagram, making it a plausible constituent of the core of neutron stars. We show that even a relatively small region of gCFL matter in a…

天体物理学 · 物理学 2009-11-10 Mark Alford , Pooja Jotwani , Chris Kouvaris , Joydip Kundu , Krishna Rajagopal

We study thermodynamic and transport properties for the isotropic color-spin-locking (iso-CSL) phase of two-flavor superconducting quark matter under compact star constraints within a NJL-type chiral quark model. Chiral symmetry breaking…

高能天体物理现象 · 物理学 2016-12-28 J. Berdermann , D. Blaschke , T. Fischer , A. Kachanovich

In this paper, we use a three flavor non-local Nambu--Jona-Lasinio (NJL) model, an~improved effective model of Quantum Chromodynamics (QCD) at low energies, to investigate the existence of deconfined quarks in the cores of neutron stars.…

高能天体物理现象 · 物理学 2017-01-26 R. D. Mellinger , F. Weber , W. Spinella , G. A. Contrera , M. G. Orsaria

We study the gluonic color-spin locked (GCSL) phase in dense two-flavor quark matter. In this phase, the color and spatial rotational symmetries are spontaneously broken down to SO(2)_{diag} with the generator being an appropriate linear…

高能物理 - 唯象学 · 物理学 2008-11-26 Michio Hashimoto

Investigations of deconfined quark matter within NJL-type models are reviewed, focusing on the regime of low temperatures and ``moderate'' densities, which is not accessible by perturbative QCD. Central issue is the interplay between chiral…

高能物理 - 唯象学 · 物理学 2009-11-10 Michael Buballa

We investigate the phase diagram of isospin asymmetric matter at T=0 in the two flavor Nambu-Jona-Lasinio model. Our approach describes the single nucleon as a confined quark-diquark state, the saturation properties of nuclear matter at…

核理论 · 物理学 2010-02-17 S. Lawley , W. Bentz , A. W. Thomas

We study the effect of neutrino trapping in new-born quark stars within a three-flavor Nambu - Jona-Lasinio (NJL) model with self-consistently calculated quark masses. The phase diagrams and equations of state for charge neutral quark…

天体物理学 · 物理学 2009-09-29 F. Sandin , D. Blaschke

The effect of color superconductivity on the cooling of quark stars and neutron stars with large quark cores is investigated. Various known and new quark-neutrino processes are studied. As a result, stars being in the color flavor locked…

天体物理学 · 物理学 2010-04-06 D. Blaschke , T. Klaehn , D. N. Voskresensky
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