Results 21 to 30 of about 80,385 (278)
Flow probe of symmetry energy in relativistic heavy-ion reactions [PDF]
, 2013 Flow observables in heavy-ion reactions at incident energies up to about 1 GeV per nucleon have been shown to be very useful for investigating the reaction dynamics and for determining the parameters of reaction models based on transport theory.
Cozma, M. D. +7 more
core +2 more sources
EPJ Web of Conferences, 2016 Eigenvalues are obtained for one-dimensional steady-state neutron transport equation in slab geometry using Henyey-Greenstein (HG) phase function. Firstly, HG phase function is inserted into neutron transport equation then eigenvalues are calculated for ...
Bülbül Ahmet
doaj +1 more source
COMPARISON OF CHEBYSHEV AND ANDERSON ACCELERATIONS FOR THE NEUTRON TRANSPORT EQUATION [PDF]
EPJ Web of Conferences, 2021 This work focuses on the k-eigenvalue problem of the neutron transport equation. The variables of interest are the largest eigenvalue (keff) and the corresponding eigenmode is called the fundamental mode.
Calloo Ansar +2 more
doaj +1 more source
PARTIAL NEUTRON TRANSPORT EQUATIONS
PROBLEMS OF ATOMIC SCIENCE AND TECHNOLOGY. SERIES: NUCLEAR AND REACTOR CONSTANTS, 2019 To analyze the spatial kinetics of the reactor, a system of equations for the spatial kinetics of the reactor, consisting of two equations, is usually used. One of them describes the behavior of the neutron flux density, and the second describes the behavior of the precursors of delayed neutrons.
I Chernova, V Bereznev, E Seleznev
openaire +1 more source
Energies, 2022 The shielding calculation of neutron streaming problems with ducts is characterized by the strong anisotropy of angular flux, which poses a challenge for the analysis of nuclear installations.
Xinyu Wang +3 more
doaj +1 more source
Numerical analysis of the neutron multigroup $SP_N$ equations
Comptes Rendus. Mathématique, 2021 The multigroup neutron $SP_N$ equations, which are an approximation of the neutron transport equation, are used to model nuclear reactor cores. In their steady state, these equations can be written as a source problem or an eigenvalue problem.
Jamelot, Erell, Madiot, François
doaj +1 more source
Electrical conductivity tensor of dense plasma in magnetic fields [PDF]
, 2016 Electrical conductivity of finite-temperature plasma in neutron star crusts is studied for applications in magneto-hydrodynamical description of compact stars.
Harutyunyan, Arus, Sedrakian, Armen
core +1 more source
Proton Differential Elliptic Flow and the Isospin-Dependence of the Nuclear Equation of State [PDF]
, 2001 Within an isospin-dependent transport model for nuclear reactions involving neutron-rich nuclei, we study the first-order direct transverse flow of protons and their second-order differential elliptic flow as a function of transverse momentum.
A. Akmal +53 more
core +3 more sources
A new multigroup method for cross-sections that vary rapidly in energy
, 2016 We present a numerical method for solving the time-independent thermal radiative transfer (TRT) equation or the neutron transport (NT) equation when the opacity or cross-section varies rapidly in energy (frequency).
Ahrens, C. +4 more
core +1 more source
Low mass binary neutron star mergers : gravitational waves and neutrino emission [PDF]
, 2016 Neutron star mergers are among the most promising sources of gravitational waves for advanced ground-based detectors. These mergers are also expected to power bright electromagnetic signals, in the form of short gamma-ray bursts, infrared/optical ...
Duez, Matthew D. +9 more
core +3 more sources