New Gogny interaction suitable for astrophysical applications
The D1 family of parametrizations of the Gogny interaction commonly suffers from a rather soft neutron matter equation of state that leads to maximal masses of neutron stars well below the observational value of two solar masses. We propose a reparametrization scheme that preserves the good properti...
Main Authors: | C. Gonzalez-Boquera, M. Centelles, X. Viñas, L.M. Robledo |
---|---|
Format: | Article |
Language: | English |
Published: |
Elsevier
2018-04-01
|
Series: | Physics Letters B |
Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269318301047 |
Similar Items
-
Unified Equation of State for Neutron Stars Based on the Gogny Interaction
by: Xavier Viñas, et al.
Published: (2021-09-01) -
GW170817 constraints analyzed with Gogny forces and momentum-dependent interactions
by: O. Lourenço, et al.
Published: (2020-04-01) -
Isovector and pairing properties of the gogny interaction in the context of neutron stars
by: Sellahewa, R.
Published: (2016) -
Nouvelles paramétrisations de l'interaction nucléaire effective de Gogny
by: Chappert, Frédéric
Published: (2007) -
Microscopic mean field approximation and beyond with the Gogny force
by: Péru S., et al.
Published: (2014-03-01)