Author: sylvia
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The correlation of neutron star radii and the evidence of strong phase transitions in neutron stars
One of the biggest issues in the study of Bayesian inference of neutron star (NS) equations of state (EoSs) is the choice of Bayesian priors. Given today’s measurement accuracy of […]
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Spring 2026 Undergraduate Research Program
Students in the BURN@N3AS undergraduate program work with a scientific mentor to develop their research, and also have a career mentor. Students are directly supported by N3AS, and participate in […]
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Constraints on Symmetric Dark Matter from Neutron Star Capture and Collapse
Dark matter (DM) models with a conserved particle-antiparticle number, $n_\chi-n_{\tilde \chi}$, and the asymmetry in the cosmological abundance $n_\chi\neq n_{\tilde \chi}$, are known to be challenged by the existence of […]
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New Class of Three-Nucleon Forces and Their Implications.
We identify a new class of three-nucleon forces that arises in the low-energy effective theory of nuclear interactions including pions. We estimate their contribution to the energy of neutron and […]
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Bulk viscosity of nuclear matter with pions in the neutrino-trapped regime
Recent work [B. Fore and S. Reddy, Phys. Rev. C 101 035809 (2020)] has shown that the population of thermal pions could modify the equation of state and transport properties […]
