Author: sylvia

  • research-publ

    A Detailed Comparison of Multidimensional Boltzmann Neutrino Transport Methods in Core-Collapse Supernovae

    The mechanism driving core-collapse supernovae is sensitive to the interplay between matter and neutrino radiation. However, neutrino radiation transport is very difficult to simulate, and several radiation transport methods of […]

  • research-publ

    FRIB and the GW170817 Kilonova

    In July 2018 an FRIB Theory Alliance program was held on the implications of GW170817 and its associated kilonova for r-process nucleosynthesis. Topics of discussion included the astrophysical and nuclear […]

  • research-publ

    An optimization-based approach to calculating neutrino flavor evolution

    We assess the utility of an optimization-based data assimilation (D.A.) technique for treating the problem of nonlinear neutrino flavor transformation in core collapse supernovae. D.A. uses measurements obtained from a […]

  • Jeff Berryman

    fellow

    Jeff Berryman

    Jeff completed his Ph.D. in 2017 at Northwestern University, where he worked with André de Gouvêa on neutrino and dark matter phenomenology. After his first postdoc at Virginia Tech working […]

  • Computer simulation of merger of two neutron stars with purple cones on either side of green concentric circles

    post

    N3AS: New center to focus on physics of ultra-dense neutron stars

    By Robert Sanders, Media relations, UC Berkeley. The National Science Foundation (NSF) has awarded UC Berkeley $10.9 million over five years to expand research on the exotic state of matter inside neutron stars [...]

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