N3AS Newscenter
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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 […]
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Neutrinos Join Forces to Shed Light on Dark Matter
Neutrinos can “talk” to each other much more than expected within the Standard Model, and this can provide an experimentally testable solution to the dark matter puzzle of the Universe. Can […]