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The impact of the symmetry energy on the properties of compact stars is analyzed considering constraints from nuclear physics and astrophysics. A compact star can be a neutron star composed only of nuclear matter or a hybrid star with a…

Nuclear Theory · Physics 2026-01-27 H. Güven , K. Bozkurt , E. Khan , J. Margueron

We investigate the influence of charged kaon condensation in hadronic sector on the formation of the electron-free charge neutral quark matter of equipartition of three light flavors, i.e., a phenomenon called ``enforced electrical…

High Energy Physics - Phenomenology · Physics 2007-05-23 Youngman Kim , Dong-Pil Min , Mannque Rho

In this work we present a study of magnetars composed of hadronic and quark matter, under the influence of strong magnetic fields. We present our results for hadronic matter taking into account the effects that the inclusion of anomalous…

Solar and Stellar Astrophysics · Physics 2015-02-24 R. Casali , L. B. Castro , D. P. Menezes

Kaon condensation in hyperon-mixed matter [($Y$+$K$) phase], which may be realized in neutron stars, is discussed on the basis of chiral symmetry. With the use of the effective chiral Lagrangian for kaon--baryon and kaon--kaon interactions;…

Nuclear Theory · Physics 2025-02-20 Takumi Muto , Toshiki Maruyama , Toshitaka Tatsumi

We study the consequences of the hadron-quark deconfinement phase transition in stellar compact objects when finite size effects between the deconfined quark phase and the hadronic phase are taken into account. We show that above a…

Astrophysics · Physics 2014-10-13 Ignazio Bombaci , Irene Parenti , Isaac Vidaña

Coulomb impurity of charge $Ze$ is known to destabilize the ground state of undoped graphene with respect to creation of screening space charge if $Z$ exceeds a critical value of $1/2\alpha$ set by material's fine structure constant…

Mesoscale and Nanoscale Physics · Physics 2024-02-19 Eugene B. Kolomeisky , Joseph P. Straley

We study the hadron-quark phase transition, taking into account the finite-size effects for neutron star matter. For the hadron phase, we adopt a realistic equation of state within the framework of the Brueckner-Hartree-Fock theory. For the…

High Energy Astrophysical Phenomena · Physics 2018-07-25 Nobutoshi Yasutake , Huan Chen , Toshiki Maruyama , Toshitaka Tatsumi

One of the most promising possibilities may be the appearance of quark matter in astrophysical phenomena in the light of recent progress in observations. The mechanism of deconfinement is not well understood, but the thermodynamical aspects…

High Energy Astrophysical Phenomena · Physics 2013-09-10 Nobutoshi Yasutake , Tsuneo Noda , Hajime Sotani , Toshiki Maruyama , Toshitaka Tatsumi

We give a general thermodynamical argument showing that in neutron stars, the Coulomb structured mixed phase is always favored for any first order phase transition involving systems in equilibrium with baryon number and electric charge as…

Astrophysics · Physics 2007-05-23 Michael B. Christiansen , Norman K. Glendenning

We have studied the mechanical and chemical instabilities as well as the liquid-gas-like phase transition in isospin asymmetric quark matter based on the NJL and the pNJL model. Areas of the mechanical instability region and the liquid-gas…

Nuclear Theory · Physics 2021-10-11 Lu-Meng Liu , Wen-Hao Zhou , Jun Xu , Guang-Xiong Peng

Influences of nonlinear screening on effective interactions between spherical macroions in charged colloids are described via response theory. Nonlinear screening, in addition to generating effective many-body interactions, is shown to…

Soft Condensed Matter · Physics 2007-05-23 A. R. Denton

We study the quark-hadron mixed phase in proto-neutron stars with the finite-size effects. In the calculations of pasta structures appeared in the mixed phase, the Gibbs conditions require the pressure balance and chemical equilibrium…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Nobutoshi Yasutake , Toshiki Maruyama , Toshitaka Tatsumi

We study the influence of strong magnetic fields in hybrid stars, composed by hadrons and a pure quark matter core, and analyse their structure and stability as well as some possible evolution channels due to the magnetic field decay. Using…

High Energy Astrophysical Phenomena · Physics 2019-09-30 Mauro Mariani , Milva G. Orsaria , Ignacio F. Ranea-Sandoval , Germán Lugones

We study the rotational properties of inverted hybrid stars (also termed cross stars), which have been recently proposed as a possible new class of compact stars characterized by an outer layer of quark matter and a core of hadrons, in an…

High Energy Astrophysical Phenomena · Physics 2025-04-10 Rodrigo Negreiros , Chen Zhang , Renxin Xu

In this work, we consider the properties of compact stars in which quark matter has low- and high-density phases that are separated by a first-order phase transition. Thus, unlike the commonly considered case of a single phase transition…

High Energy Astrophysical Phenomena · Physics 2023-03-27 Jia Jie Li , Armen Sedrakian , Mark Alford

By assuming that ultra dense hybrid neutron stars are endowed with a distribution of electric charge, we study the corresponding twin star solutions and their properties resulting from a sharp first order transition from confined hadronic…

High Energy Physics - Phenomenology · Physics 2022-02-16 V. P. Goncalves , J. C. Jimenez , L. Lazzari

We study structures of general relativistic compact stars with exotic matter. Our study is based on axisymetric and stationary formalism including purely toroidal magnetic field. We also study the finite size effects of quark-hadron mixed…

High Energy Astrophysical Phenomena · Physics 2014-11-18 Nobutoshi Yasutake , Toshiki Maruyama , Toshitaka Tatsumi , Kenta Kiuchi , Kei Kotake

We study the properties of strange quark matter in equilibrium with normal nuclear matter. Instead of using the conventional bag model in quark sector, we achieve the confinement by a density-dependent quark mass derived from in-medium…

Astrophysics · Physics 2008-11-26 G. X. Peng , A. Li , U. Lombardo

In a galaxy merger, the stars tidally stripped from the satellite and accreted onto the host galaxy undergo phase mixing and form finely-grained structures in the phase space. However, these fragile structures may be destroyed in the…

Astrophysics of Galaxies · Physics 2023-03-06 Elliot Y. Davies , Adam M. Dillamore , Eugene Vasiliev , Vasily Belokurov

The equation of state for quark matter is derived for a nonlocal, chiral quark model within the mean field approximation. Special emphasis is on the occurrence of a diquark condensate which signals a phase transition to color…

Astrophysics · Physics 2009-11-07 H. Grigorian , D. Blaschke , D. N. Aguilera