Author: sylvia

  • Illustration of magnetic field lines of a neutron star.

    post

    Oscillations of Highly Magnetized Non-Rotating Neutron Stars

    Neutron stars are probably the most compact and extreme magnetised astrophysical objects in the universe. These stars are the composite of the most extreme physics within only a few kilometres in diameter.

  • Yellow leaves in front of UC Berkeley Music Library.

    post

    Fall 2023 Undergraduate Research Program

    Application deadline: September 4, 2023. Students in the N3AS undergraduate program work with a scientific mentor to develop their research, and also have a career mentor.

  • research-publ

    Neutrinos and Nucleosynthesis of Elements

    Neutrinos are known to play important roles in many astrophysical scenarios from the early period of the big bang to current stellar evolution being a unique messenger of the fusion […]

  • research-publ

    Inelastic Freeze-in

    Dark matter (DM) could be a nonthermal relic that freezes in from extremely weak, sub-Hubble annihilation and decay of Standard Model (SM) particles. The case of Dirac DM freezing in […]

  • research-publ

    Impact of the equation of state on f- and p- mode oscillations of neutron stars

    We investigate the impact of the neutron-star matter equation of state on the f- and p1-mode oscillations of neutron stars obtained within the Cowling approximation and linearized general relativity. The […]