N3AS Newscenter
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Studying the Impact of Dark Photon Emission on Massive Star Evolution
Dark matter represents more than 80% of the matter density of the universe and remains one of the biggest mysteries in physics. In many models currently under investigation, it could […]
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Investigating neutrino collective flavor oscillations with machine learning
During the explosion of a massive dying star — a supernova — millions of tiny subatomic particles called neutrinos are emitted. These neutrinos are emitted from deep inside the star, […]
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Mu-Tau Neutrinos: Influencing Fast Flavor Conversions in Supernovae
Mysteries involving the interplay of tiny neutrinos and huge supernova explosions become more intriguing! During the cataclysmic explosion of a dying star — a supernova — millions of tiny subatomic […]
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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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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 […]