no code implementations • 19 Feb 2021 • Reed Essick, Ingo Tews, Philippe Landry, Achim Schwenk
The symmetry energy and its density dependence are crucial inputs for many nuclear physics and astrophysics applications, as they determine properties ranging from the neutron-skin thickness of nuclei to the crust thickness and the radius of neutron stars.
Gaussian Processes Nuclear Theory High Energy Astrophysical Phenomena Nuclear Experiment
1 code implementation • 27 Aug 2019 • Collin D. Capano, Ingo Tews, Stephanie M. Brown, Ben Margalit, Soumi De, Sumit Kumar, Duncan A. Brown, Badri Krishnan, Sanjay Reddy
The properties of neutron stars are determined by the nature of the matter that they contain.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology High Energy Physics - Phenomenology Nuclear Theory