Stefano Gandolfi

6 ta ish

Los Alamos National Laboratory

1. Maximum mass and radius of neutron stars, and the nuclear symmetry energy

   Stefano Gandolfi, J. Carlson, Sanjay Reddy

   MaqolaOAOchiq kirish20125 iqtibos

   ABIABI:AkademIndex/2026.other.164006

2. Connecting Neutron Star Observations to Three-Body Forces in Neutron Matter and to the Nuclear Symmetry Energy

   Andrew W. Steiner, Stefano Gandolfi

   MaqolaOAOchiq kirish20124 iqtibos

   ABIABI:AkademIndex/2026.other.019660

3. Constraints on the symmetry energy and neutron skins from experiments and theory

   M. B. Tsang, J. R. Stone, F. Camera +16

   MaqolaOAOchiq kirish20123 iqtibos

   ABIABI:AkademIndex/2026.other.019671

4. Microscopic calculation of the equation of state of nuclear matter and neutron star structure

   Stefano Gandolfi, A. Yu. Illarionov, S. Fantoni +3

   MaqolaOAOchiq kirish20103 iqtibos

   ABIABI:AkademIndex/2026.other.164015

5. Quantum Monte Carlo calculation of the equation of state of neutron matter

   Stefano Gandolfi, A. Yu. Illarionov, K. E. Schmidt +2

   MaqolaOAOchiq kirish20093 iqtibos

   ABIABI:AkademIndex/2026.other.164024

6. Dense nuclear matter equation of state from heavy-ion collisions

   Agnieszka Sorensen, Kshitij Agarwal, K. W. Brown +97

   Maqola20232 iqtibos

   ABIABI:AkademIndex/2026.other.333512