Argonne family potentials and neutron star matter equation of state
Department of Physics, University of Zanjan, 45371-38791, Zanjan, Iran
* e-mail: email@example.com
Accepted: 23 June 2019
Published online: 6 September 2019
Properties of neutron star matter are studied using different microscopic equation of states, derived from the lowest order constrained variational (LOCV) many-body theory using the two-body nuclear force AV8' , and AV6' and also implementing the three-nucleon interaction in AV18, AV8' , and AV6' . The maximum mass configuration of the neutron star is obtained, , with AV18+TNI, AV8' +TNI and AV6' +TNI, respectively, which is an excellent agreement with the accepted maximum mass of non-rotating neutron star range .
© Società Italiana di Fisica / Springer-Verlag GmbH Germany, part of Springer Nature, 2019