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Related papers: Kaon Condensation in Dense Stellar Matter

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This article combines two talks given by the authors and is based on works done in collaboration with G.E. Brown and D.-P. Min on kaon condensation in dense baryonic medium treated in chiral perturbation theory using heavy-baryon formalism.…

High Energy Physics - Phenomenology · Physics 2009-10-28 Chang-Hwan Lee , Mannque Rho

The critical density for kaon condensation in ``nuclear star" matter is computed up to two-loop order {\it in medium} (corresponding to next-to-next-to-leading order in chiral perturbation theory in free space) with a heavy-baryon effective…

High Energy Physics - Phenomenology · Physics 2009-10-28 Chang-Hwan Lee , G. E. Brown , Mannque Rho

An effective chiral Lagrangian in heavy-fermion formalism whose parameters are constrained by kaon-nucleon and kaon-nuclear interactions next to the leading order in chiral expansion is used to describe kaon condensation in dense ``neutron…

High Energy Physics - Phenomenology · Physics 2011-07-19 G. E. Brown , C. -H. Lee , M. Rho , V. Thorsson

We address the possibility of the appearance of a charged kaon condensate in neutron star cores described within a generalized Skyrme model. Our treatment of strange degrees of freedom is based on the Bound State Approach by Callan and…

We point out that the problem of kaon condensation in dense hadronic matter can be addressed in perturbative QCD. Indeed, perturbative calculations suggest that negative kaons are condensed in high density quark matter if the electroweak…

Nuclear Theory · Physics 2008-11-26 Thomas Schaefer

The recent measurement of the mass of neutron stars (PSR J1614 - 2230, PSR J0348 + 0432, MSP J0740 + 6620) restricts the lower limit $\sim 2M_{\odot}$ of the maximum mass of such compact stars, making it possible for dense matter to exist…

Nuclear Theory · Physics 2022-02-08 Fu Ma , Wenjun Guo , Chen Wu

We formulate kaon condensation in dense baryonic matter with anti-kaons fluctuating from the Fermi-liquid fixed point. This entails that in the Wilsonian RG approach, the decimation is effectuated in the baryonic sector to the Fermi surface…

Nuclear Theory · Physics 2015-01-14 Won-Gi Paeng , Mannque Rho

Based on the Kaplan-Nelson Lagrangian, we investigate kaon condensation in dense neutron star matter allowing for the explicit presence of hyperons. Using various models we find that the condensate threshold is sensitive to the behavior of…

Nuclear Theory · Physics 2016-09-08 Paul J. Ellis , Roland Knorren , Madappa Prakash

Using the Callan-Klebanov bound state model for hyperons simulated on crystal lattice to describe strange baryonic matter, we argue that to ${\cal O} (1)$ in the large $N_c$ counting to which the theory is robust, hyperons can figure only…

Nuclear Theory · Physics 2013-01-03 Hyun Kyu Lee , Mannque Rho

We investigate the possibility of kaon condensation in the dense interior of neutron stars through the s--wave interaction of kaons with nucleons. We include nucleon--nucleon interactions by using simple parametrizations of realistic…

Nuclear Theory · Physics 2009-10-22 V. Thorsson , M. Prakash , J. M. Lattimer

We discuss the equation of state of neutron stars in the dense interior considering hyperons and the possible onset of kaon condensation within the relativistic mean field model. We find that hyperons are favoured in dense matter and that…

Nuclear Theory · Physics 2022-02-23 J. Schaffner , J. Bondorf , I. N. Mishustin

We examine the presence of strangeness-bearing components, hyperons and kaons, in dense neutron star matter. Calculations are performed using relativistic mean field models, in which both the baryon-baryon and kaon-baryon interactions are…

Nuclear Theory · Physics 2009-09-25 R. Knorren , M. Prakash , P. J. Ellis

Dense hadronic matter at low temperature is expected to be in crystal and at high density make a transition to a {\em chirally restored but color-confined} state which is a novel phase hitherto unexplored. This phase transition is predicted…

High Energy Physics - Phenomenology · Physics 2010-04-06 Byung-Yoon Park , Joon-Il Kim , Mannque Rho

Kaon polarization operator in dense baryonic matter of arbitrary isotopic composition is calculated including s- and p-wave kaon-baryon interactions. The regular part of the polarization operator is extracted from the realistic kaon-nucleon…

Nuclear Theory · Physics 2009-11-07 E. E. Kolomeitsev , D. N. Voskresensky

Recent measurements of neutron star mass from several candidates (PSR J$1614-2230$, PSR J$0348+0432$, MSP J$0740+6620$) set the lower bound on the maximum possible mass for this class of compact objects $\sim 2$ M$_\odot$. Existence of…

High Energy Astrophysical Phenomena · Physics 2020-12-04 Vivek Baruah Thapa , Monika Sinha

We discuss three different ways to arrive at kaon condensation at n_c = 3 n_0 where n_0 is nuclear matter density: (1) Fluctuating around the n=0 vacuum in chiral perturbation theory, (2) fluctuating around n_VM near the chiral restoration…

High Energy Physics - Phenomenology · Physics 2008-11-26 Gerald E. Brown , Chang-Hwan Lee , Mannque Rho

The core of neutron-star matter is supposed to be at a much higher density than the normal nuclear matter density for which various possibilities have been suggested such as, for example, meson or hyperon condensation and/or deconfined…

High Energy Astrophysical Phenomena · Physics 2011-10-07 Kyungmin Kim , Hyun Kyu Lee , Mannque Rho

We investigate $K^-$ and $\bar K^0$ condensation in $\beta$-equilibrated hyperonic matter within a density dependent hadron field theoretical model. In this model, baryon-baryon and (anti)kaon-baryon interactions are mediated by the…

Astrophysics · Physics 2009-11-07 Sarmistha Banik , Debades Bandyopadhyay

The variation of kaon mass in dense, charge-neutral baryonic matter at beta-equilibrium has been investigated. The baryon interaction has been included by means of nonlinear Walecka model, with and without hyperons and the interaction of…

Nuclear Theory · Physics 2009-10-30 Abhijit Bhattacharyya , Sanjay K. Ghosh , S. C. Phatak , Sibaji Raha

We use the modified quark-meson coupling and the quantum hadrodynamics models to study the properties of neutron star. Coupling constants of both models are adjusted to reproduce the same saturation properties. The onset of kaon…

Nuclear Theory · Physics 2007-05-23 S. W. Hong , C. H. Hyun , C. Y. Ryu
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