Translating Neutron Star Observations to Nuclear Symmetry Energy via Deep Neural Networks

One of the most significant challenges involved in efforts to understand the equation of state of dense neutron-rich matter is the uncertain density dependence of the nuclear symmetry energy. In particular, the nuclear symmetry energy is still rather poorly constrained, especially at high densities....

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Bibliographic Details
Main Author: Plamen G. Krastev
Format: Article
Language:English
Published: MDPI AG 2022-01-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/10/1/16