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相关论文: Specific viscosity of neutron-rich nuclear matter …

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We calculate the electron shear viscosity (determined by Coulomb electron collisions) for a dense matter in a wide range of parameters typical for white dwarf cores and neutron star crusts. In the density range from ~10^3 g cm^-3 to…

天体物理学 · 物理学 2009-11-13 A. I. Chugunov , D. G. Yakovlev

The radii of nucleon distribution, bulk density, and neutron skin in nuclei beyond the \beta-stability line are studied within the direct variational method. We evaluate the partial equation of state of finite nuclei and demonstrate that…

核理论 · 物理学 2012-03-22 V. M. Kolomietz , S. V. Lukyanov , A. I. Sanzhur

We present a numerical study of shear viscosity and thermal conductivity of symmetric nuclear matter, pure neutron matter and $\beta$-stable nuclear matter, in the framework of the Brueckner theory. The calculation of in-medium cross…

太阳与恒星天体物理 · 物理学 2014-11-21 H. F. Zhang , U. Lombardo , W. Zuo

The transport property of cold and dense nucleon matter is important for nuclear physics but is relatively less studied than that at finite temperatures. In this paper, we present a primary study of bulk and shear viscosities in the limit…

核理论 · 物理学 2025-04-09 Jianing Li , Weiyao Ke

We clarify how the weak-interaction-driven bulk viscosity $\zeta$ and the bulk relaxation time $\tau_\Pi$ of neutrino-transparent $npe$ matter depend on the nuclear symmetry energy. We show that, at saturation density, the equation-of-state…

核理论 · 物理学 2025-11-11 Yumu Yang , Mauricio Hippert , Enrico Speranza , Jorge Noronha

For beta-equilibrated nuclear matter we estimate the contribution to the bulk viscosity from purely leptonic processes, namely the conversion of electrons to and from muons. For oscillation frequencies in the kiloHertz range, we find that…

核理论 · 物理学 2010-12-02 Mark G. Alford , Gerald Good

Various kinds of isovector nucleon effective masses are used in the literature to characterize the momentum/energy dependence of the nucleon symmetry potential or self-energy due to the space/time non-locality of the underlying isovector…

核理论 · 物理学 2018-02-21 Bao-An Li , Bao-Jun Cai , Lie-Wen Chen , Jun Xu

Heavy-ion reactions induced by neutron-rich nuclei provide a unique means to investigate the equation of state of isospin-asymmetric nuclear matter, especially the density dependence of the nuclear symmetry energy. In particular, recent…

核理论 · 物理学 2009-09-29 Lie-Wen Chen , Che Ming Ko , Bao-An Li , Gao-Chan Yong

The history and recent progresses in the study of bulk viscosity in nuclear and quark matter are reviewed. The constraints from baryon number conservation and electric neutrality in quark matter on particle densities and fluid velocity…

天体物理学 · 物理学 2008-11-26 Hui Dong , Nan Su , Qun Wang

Including nucleon-nucleon correlations due to both Fermi statistics and nuclear forces, we have developed a general formalism for calculating the neutral-current neutrino-nucleon opacities in nuclear matter. We derive corrections to the…

天体物理学 · 物理学 2008-11-26 Adam Burrows , R. F. Sawyer

The in-medium neutron-proton, proton-proton (neutron-neutron) elastic scattering cross sections ($\sigma_{np}^{*}$, $\sigma_{pp(nn)}^{*}$) are studied based on the effective Lagrangian of density dependent relativistic hadron theory in…

核理论 · 物理学 2009-11-10 Qingfeng Li , Zhuxia Li , Enguang Zhao

The symmetry energy expansion is a useful way to parametrize the properties of dense matter near nuclear saturation density, and much work has been done to connect physical quantities like the neutron star radius and the core-crust…

核理论 · 物理学 2025-09-26 Steven P Harris

We have calculated microscopically bulk viscosity of hadronic matter, where equilibrium thermodynamics for all hadrons in medium are described by Hadron Resonance Gas (HRG) model. Considering pions and nucleons as abundant medium…

核理论 · 物理学 2016-12-20 Sabyasachi Ghosh , Sandeep Chatterjee , Bedangdas Mohanty

We investigate the shear viscosity of neutron star matter in the presence of an antikaon condensate. The electron and muon number densities are reduced due to the appearance of a $K^-$ condensate in neutron star matter, whereas the proton…

太阳与恒星天体物理 · 物理学 2010-04-23 Rana Nandi , Sarmistha Banik , Debades Bandyopadhyay

Transitions of nuclear compositions in the crust of a neutron star induced by stellar spin-down are evaluated at zero temperature. We construct a compressible liquid-drop model for the energy of nuclei immersed in a neutron gas, including…

天体物理学 · 物理学 2016-08-30 Kei Iida , Katsuhiko Sato

We study varying forms of viscous dark matter and try to address the intriguing tensions of the standard model of cosmology with recent cosmological data, including the Hubble and $S_8$ tensions. We note that by assuming the dark matter…

宇宙学与河外天体物理 · 物理学 2023-12-15 Amjad Ashoorioon , Zahra Davari

The specific shear viscosity $\bar\eta$ of a classically rotating system of nucleons that interact via a monopole pairing interaction is calculated including the effects of thermal fluctuations and coupling to pair vibrations within the…

核理论 · 物理学 2015-06-05 N. Quang Hung , N. Dinh Dang

Data on stopping in intermediate-energy central heavy-ion collisions are analyzed following transport theory based on the Boltzmann equation. In consequence, values of nuclear shear viscosity are inferred. The inferred values are…

核理论 · 物理学 2009-06-12 P. Danielewicz , B. Barker , L. Shi

The existence of a dark baryon that mixes with the neutron leads to the possibility of neutron decay into a dark sector. Such dark decays have been studied as possibly relevant for the neutron decay anomaly and for their potential impacts…

高能天体物理现象 · 物理学 2026-04-20 Steven P. Harris , C. J. Horowitz

We present a comprehensive and pedagogic discussion of the properties of photons in cold and dense nuclear matter based on the resummed one-loop photon self energy. Correlations between electrons, muons, protons and neutrons in beta…

高能天体物理现象 · 物理学 2018-04-18 Stephan Stetina , Ermal Rrapaj , Sanjay Reddy