Author: sylvia

• 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 […]

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  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 […]

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  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 [...]

• event

  Dark photons and supernovae: Lessons from astrophysics

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  post

  Sandblasting the r-Process: Spallation of Ejecta from Neutron Star Mergers

  Abundances in the third peak (180<A<200) of the r-process pattern produced with PRISM calculation of disk wind conditions of a neutron star merger event, before (blue line) and after spallation […]