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相关论文: Chiral thermodynamics of nuclear matter

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We calculate the equation of state of nuclear matter for arbitrary isospin-asymmetry up to three loop order in the free energy density in the framework of in-medium chiral perturbation theory. In our approach 1\pi- and 2\pi-exchange…

核理论 · 物理学 2012-03-06 Salvatore Fiorilla , Norbert Kaiser , Wolfram Weise

The density and temperature dependence of the nuclear symmetry free energy is investigated using microscopic two- and three-body nuclear potentials constructed from chiral effective field theory. The nuclear force models and many-body…

核理论 · 物理学 2016-03-23 Corbinian Wellenhofer , Jeremy W. Holt , Norbert Kaiser

The temperature dependence of the chiral condensate in isospin-symmetric nuclear matter at varying baryon density is investigated using thermal in-medium chiral effective field theory. This framework provides a realistic approach to the…

核理论 · 物理学 2015-06-04 Salvatore Fiorilla , Norbert Kaiser , Wolfram Weise

Based on a chiral approach to nuclear matter, we calculate the quartic term in the expansion of the equation of state of isospin-asymmetric nuclear matter. The contributions to the quartic isospin asymmetry energy $A_4(k_f)$ arising from…

核理论 · 物理学 2015-04-03 N. Kaiser

The temperature dependence of the chiral condensate in isospin-symmetric nuclear matter at varying baryon densities is investigated starting from a realistic free energy density of the correlated nuclear many-body system. The framework is…

核理论 · 物理学 2011-04-15 S. Fiorilla , N. Kaiser , W. Weise

We extend a recent three-loop calculation of nuclear matter in the systematic framework of chiral perturbation theory to finite temperatures T. The contributions from one- and two-pion exchange diagrams which cause nuclear binding and…

核理论 · 物理学 2009-11-07 S. Fritsch , N. Kaiser , W. Weise

The computation of the thermodynamic properties of nuclear matter is a central task of theoretical nuclear physics. The nuclear equation of state is an essential quantity in nuclear astrophysics and governs the properties of neutron stars…

核理论 · 物理学 2017-10-31 Corbinian Wellenhofer

We calculate the equation of state of isospin-symmetric nuclear matter in the three-loop approximation of chiral perturbation theory. The contributions to the energy per particle $\bar E(k_f)$ from one- and two-pion exchange diagrams are…

核理论 · 物理学 2009-11-07 N. Kaiser , S. Fritsch , W. Weise

We extend a recent three-loop calculation of nuclear matter in chiral perturbation theory by including the effects from two-pion exchange with single and double virtual $\Delta(1232)$-isobar excitation. Regularization dependent short-range…

核理论 · 物理学 2009-11-10 S. Fritsch , N. Kaiser , W. Weise

We investigate the thermodynamic equation of state of isospin-symmetric nuclear matter with microscopic nuclear forces derived within the framework of chiral effective field theory. Two- and three-body nuclear interactions constructed at…

核理论 · 物理学 2015-08-07 Corbinian Wellenhofer , Jeremy W. Holt , Norbert Kaiser , Wolfram Weise

This study uses classical molecular dynamics to simulate infinite nuclear matter and study the effect of isospin asymmetry on bulk properties such as energy per nucleon, pressure, saturation density, compressibility and symmetry energy. The…

核理论 · 物理学 2014-02-26 J. A. López , E. Ramírez-Homs , R. González , R. Ravelo

We calculate the equation of state of asymmetric nuclear matter at finite temperature based on chiral effective field theory interactions to next-to-next-to-next-to-leading order. Our results assess the theoretical uncertainties from the…

核理论 · 物理学 2023-02-21 J. Keller , K. Hebeler , A. Schwenk

We calculate the properties of isospin-asymmetric nuclear matter based on chiral nucleon-nucleon (NN) and three-nucleon (3N) interactions. To this end, we develop an improved normal-ordering framework that allows to include general 3N…

核理论 · 物理学 2016-12-12 Christian Drischler , Kai Hebeler , Achim Schwenk

We calculate the density-dependent spin-asymmetry energy $S(k_f)$ of isospin-symmetric nuclear matter in the three-loop approximation of chiral perturbation theory. The interaction contributions to $S(k_f)$ originate from one-pion exchange,…

核理论 · 物理学 2009-11-10 N. Kaiser

We calculate the density-dependent spin-isospin asymmetry energy $J(k_f)$ of nuclear matter in the three-loop approximation of chiral perturbation theory. The interaction contributions to $J(k_f)$ originate from one-pion exchange, iterated…

核理论 · 物理学 2009-11-11 N. Kaiser

This presentation reviews an approach to nuclear many-body systems based on the spontaneously broken chiral symmetry of low-energy QCD. In the low-energy limit, for energies and momenta small compared to a characteristic symmetry breaking…

核理论 · 物理学 2015-06-15 J. W. Holt , N. Kaiser , W. Weise

We compute the density dependence of in-medium pion properties, such as mass, wave function renormalization, and decay constant in the correlation function approach, and how they change under the influence of isospin-asymmetric nuclear…

核理论 · 物理学 2025-07-03 Kihong Kwon , Yamato Suda , Stephan Hübsch , Daisuke Jido

Thermal properties of asymmetric nuclear matter, including the temperature dependence of the symmetry energy, single-particle properties, and differential isospin fractionation, are investigated with different neutron-proton effective mass…

核理论 · 物理学 2015-01-23 Jun Xu , Lie-Wen Chen , Bao-An Li

The isospin-asymmetry dependence of the nuclear matter equation of state obtained from microscopic chiral two- and three-body interactions in second-order many-body perturbation theory is examined in detail. The quadratic, quartic and…

核理论 · 物理学 2016-05-11 Corbinian Wellenhofer , Jeremy W. Holt , Norbert Kaiser

We consider isospin-asymmetric matter in the parity-doublet model within an extended mean-field calculation, increasing continuously the neutron excess all the way to pure neutron matter. We compute the liquid-gas and the chiral phase…

核理论 · 物理学 2024-08-05 Jürgen Eser , Jean-Paul Blaizot
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