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相关论文: Inhomogeneous chiral symmetry breaking in dense ne…

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Recent studies of our group are reviewed about the inhomogeneous chiral phase. Appearance of the inhomogeneous chiral phase is a new paradigm in the field of the QCD phase diagram. We consider the dual-chiral-density-wave in the presence of…

高能物理 - 唯象学 · 物理学 2015-12-15 T. Tatsumi

The inhomogeneous quark condensate, responsible for dynamical chiral symmetry breaking in cold nuclear matter, is studied by putting skyrmions onto the face-centered cubic crystal and treating the skyrmion matter as nuclear matter. By…

高能物理 - 唯象学 · 物理学 2015-06-03 Masayasu Harada , Hyun Kyu Lee , Yong-Liang Ma , Mannque Rho

In the past few years, a growing number of compelling arguments, backed up by model calculations, pointed out that the intermediate-density region of the QCD phase diagram may be characterized by the formation of inhomogeneous condensates…

高能物理 - 唯象学 · 物理学 2014-11-07 Stefano Carignano , Efrain J. Ferrer , Vivian de la Incera

It is demonstrated how in the absence of solutions for QCD under conditions deep inside compact stars an equation of state can be obtained within a model that is built on the basic symmetries of the QCD Lagrangian, in particular chiral…

高能天体物理现象 · 物理学 2014-10-07 David Blaschke

We investigate the influence of spatially inhomogeneous chiral symmetry-breaking condensates in a magnetic field background on the equation of state for compact stellar objects. After building a hybrid star composed of nuclear and quark…

核理论 · 物理学 2015-11-18 S. Carignano , E. J. Ferrer , V. de la Incera , L. Paulucci

In this letter, we discuss a novel method to search for inhomogeneous chiral symmetry breaking in theories with fermions. The prime application we have in mind is QCD, but the method is also applicable for other theories, including…

高能物理 - 唯象学 · 物理学 2025-03-26 Theo F. Motta , Julian Bernhardt , Michael Buballa , Christian S. Fischer

The chiral condensate, which is constant in vacuum, may become spatially modulated at moderately high densities where in the traditional picture of the QCD phase diagram a first-order chiral phase transition occurs. We review the current…

高能物理 - 唯象学 · 物理学 2015-06-19 Michael Buballa , Stefano Carignano

We use a variational procedure to study finite density QCD in an approximation in which the interaction between quarks is modelled by that induced by instantons. We find that uniform states with conventional chiral symmetry breaking have…

高能物理 - 唯象学 · 物理学 2008-11-26 Krishna Rajagopal

We investigate the effects of isospin asymmetry on inhomogeneous chiral symmetry breaking phases within the two-flavor NJL model. After introducing a plane-wave ansatz for each quark-flavor condensate, we find that, as long as their…

高能物理 - 唯象学 · 物理学 2015-06-18 Daniel Nowakowski , Michael Buballa , Stefano Carignano , Jochen Wambach

We use a variational procedure to study finite density QCD in an approximation in which the interaction between quarks is modelled by that induced by instantons. We find that uniform states with conventional chiral symmetry breaking have…

高能物理 - 唯象学 · 物理学 2009-10-30 M. Alford , K. Rajagopal , F. Wilczek

Recent lattice QCD studies at vanishing density exhibit the parity-doubling structure for the low-lying baryons around the chiral crossover temperature. This finding is likely an imprint of the chiral symmetry restoration in the baryonic…

核理论 · 物理学 2018-12-21 Michał Marczenko , David Blaschke , Krzysztof Redlich , Chihiro Sasaki

Cold and dense matter may break rotational symmetry spontaneously and thus form an anisotropic phase in the interior of neutron stars. We consider the concrete example of an anisotropic chiral condensate in the form of a chiral density…

核理论 · 物理学 2025-01-22 Orestis Papadopoulos , Andreas Schmitt

Based on a baryonic extended linear sigma model including explicit chiral symmetry breaking effect, the structure of neutron star with the emergence of hyperons is investigated using the relativistic mean field approximation. It's found…

核理论 · 物理学 2025-12-30 Yao Ma , Yong-Liang Ma , Lu-Qi Zhang

Inhomogeneous superconductors and inhomogeneous superfluids appear in a variety of contexts including quark matter at extreme densities, fermionic systems of cold atoms, type-II cuprates, and organic superconductors. In the present review…

We investigate the existence of inhomogeneous chiral phases in the quark-meson model with explicit chiral-symmetry breaking. We find that the inhomogeneous region shrinks with increasing pion masses but survives for the physical value of…

高能物理 - 唯象学 · 物理学 2021-01-18 Michael Buballa , Stefano Carignano , Lennart Kurth

We discuss the possible influence of fundamental QCD properties such as spontaneous chiral symmetry breaking and nucleon substructure on nuclear matter properties. We propose a chiral version of the relativistic $\sigma-\omega$ model in…

核理论 · 物理学 2011-07-19 G. Chanfray , M. Ericsson , E. Massot

We explore a possible phase where chiral $SU(2)_L \times SU(2)_R$ symmetry is spontaneously broken while its center $Z_2$ symmetry remains unbroken and its consequence on thermal quantities. In this phase, chiral symmetry breaking is driven…

高能物理 - 唯象学 · 物理学 2010-02-04 M. Harada , C. Sasaki , S. Takemoto

The effect of explicit chiral-symmetry breaking on inhomogeneous chiral phases is studied within a Nambu-Jona-Lasinio model with nonzero current quark mass. Generalizing an earlier result obtained in the chiral limit, we show within a…

高能物理 - 唯象学 · 物理学 2020-06-04 Michael Buballa , Stefano Carignano

While chiral symmetry breaking in the QCD vacuum is attributed to nonzero chiral condensate, an alternative symmetry breaking pattern with no chiral condensate is also possible, as pointed out by Stern. This hypothetical phase was excluded…

高能物理 - 唯象学 · 物理学 2015-10-06 Takuya Kanazawa

The modern phase diagram of strongly interacting matter reveals a rich structure at high-densities due to phase transitions related to the chiral symmetry of quantum chromodynamics (QCD) and the phenomenon of color superconductivity. These…

天体物理学 · 物理学 2009-06-23 J. Schaffner-Bielich
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