Author: sylvia

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  Large and massive neutron stars: Implications for the sound speed in dense QCD

  How big are neutron stars? Precise measurements of the size of neutron stars are required for having a solid grasp on the state of the densest material in their interiors, and for differentiating between theoretical models.

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  Collective neutrino oscillations with tensor networks using a time-dependent variational principle

  A system of oscillating neutrinos at high densities, wherein neutrino-neutrino coherent forward scatterings are non-negligible, represents a many-body problem engendered by the weak interaction. Whether an interplay between the one-body […]

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  North Carolina State REU Program: Computational and Data Science in Astrophysics

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  Dense Nuclear Matter Equation of State from Heavy-Ion Collisions

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  Parton Distributions and Nucleon Structure