Three-body calculation of the level shift in kaonic deuterium with realistic potentials
J. Révai
Phys. Rev. C 94, 054001 (2016) - Published 9 November, 2016
Nucleon-nucleon interaction with one-pion exchange and instanton-induced interactions
C. S. Vanamali and K. B. Vijaya Kumar
Phys. Rev. C 94, 054002 (2016) - Published 11 November, 2016
Longitudinal asymmetry and proton spin rotation in scattering with pionless effective field theory
N. Mahboubi, S. Bayegan, H. Nematollahi, and M. Moeini Arani
Phys. Rev. C 94, 054003 (2016) - Published 15 November, 2016
reaction with pionless effective field theory
H. Nematollahi, S. Bayegan, N. Mahboubi, and M. Moeini Arani
Phys. Rev. C 94, 054004 (2016) - Published 15 November, 2016
Quantum Monte Carlo calculations of two neutrons in finite volume
P. Klos, J. E. Lynn, I. Tews, S. Gandolfi, A. Gezerlis, H.-W. Hammer, M. Hoferichter, and A. Schwenk
Phys. Rev. C 94, 054005 (2016) - Published 18 November, 2016
Role of correlations in spin-polarized neutron matter
Isaac Vidaña, Artur Polls, and Victoria Durant
Phys. Rev. C 94, 054006 (2016) - Published 28 November, 2016
This paper uses Brueckner theory in its accepted modern form to definitively establish that neutron matter, in the density regime relevant to neutron stars, does not suffer any ferromagnetic instability. This result shows that a ferromagnetic transition cannot be the origin of the magnetic fields in neutron stars.
Local chiral potentials with -intermediate states and the structure of light nuclei
M. Piarulli, L. Girlanda, R. Schiavilla, A. Kievsky, A. Lovato, L. E. Marcucci, Steven C. Pieper, M. Viviani, and R. B. Wiringa
Phys. Rev. C 94, 054007 (2016) - Published 28 November, 2016







