$NEUT neutron

Latest papers

1. Prospects for modelling odd and odd-odd nuclei using energy density functionals nucl-th · 14 Oct · 1 hit

   …have an odd number of nucleons. About one quarter more are odd-odd, meaning they have an odd number of neutrons and an odd number of protons. In this context, it is about time to shift the 70-odd-year focus of…

2. Fast Monte Carlo calculation of multiple scattering in resonant neutron capture nucl-th · 14 Oct · 4 hits

   A fast Monte Carlo code has been developed to calculate multiple neutron scattering in a sample. Good agreement with an independent Monte Carlo calculation using SAMMY is…

3. Rotochemical heating of neutron stars in 2D astro-ph.HE · 14 Oct · 2 hits

   The matter inside a spinning-down neutron star (NS) undergoes a slow compression that may drive it out of chemical equilibrium and,…

4. Search for Compact Binary Coalescences with Sub-solar Mass Components in Data from the Second Part of LIGO-Virgo-KAGRA's Fourth Observing Run gr-qc · 14 Oct · 1 hit

   …parts of the observing run to the target sub-solar mass (SSM) black hole (BH) population, as well as to neutron star (NS) binaries with one or more sub-solar component. We place upper limits on the merger rate of…

5. Constraining three-nucleon forces in nuclear lattice effective field theory nucl-th · 14 Oct · 1 hit

   …their coefficients from nuclear binding energies for nuclei in the mass range from $A=3$ to $A=40$ and neutron--alpha finite-volume energies. This allows to work out the minimal three-nucleon force that can be…

6. A practical route to amorphous solid-state electrolyte structures by hybrid reverse Monte Carlo with foundation potentials cond-mat.mtrl-sci · 14 Oct · 1 hit

   …We benchmark both routes and two hybrid schemes on amorphous \ce{Li_{0.9}NbO_{0.9}Cl_{4.1}} against one neutron pair distribution function with one foundation potential. The hybrid schemes put the energy either in…

7. Constraint on particle mass of dark matter based on XTE J1814-338 observation and DANS model astro-ph.HE · 14 Oct · 3 hits

   The small observed radius of neutron star XTE J1814-338 (with mass of $1.21_{-0.05}^{+0.05}$ $M_{\odot}$ and radius of $7_{-0.4}^{+0.4}$…

8. Collective-flow signatures of bubble nuclei in intermediate-energy projectile fragmentation reactions nucl-th · 14 Oct · 1 hit

   …this value, heavy-fragment production plays a significant role, while the directed flow $v_1$ of protons and neutrons remains predominantly negative, indicating preferential emission toward the target side. Above…