Bayesian reconstruction of nuclear matter parameters from the equation of state of neutron star matter
Author:
Funder
Department of Science and Technology, Ministry of Science and Technology
Fundação para a Ciência e a Tecnologia
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.105.015806/fulltext
Reference76 articles.
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2. CONSTRAINING THE SYMMETRY PARAMETERS OF THE NUCLEAR INTERACTION
3. New parametrization for the Lagrangian density of relativistic mean field theory
4. Neutron-Rich Nuclei and Neutron Stars: A New Accurately Calibrated Interaction for the Study of Neutron-Rich Matter
5. Determination of the parameters of a Skyrme type effective interaction using the simulated annealing approach
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