Author: sylvia

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  Cooling of the Cassiopeia A neutron star and superfluid implications

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  Towards Probing the Diffuse Supernova Neutrino Background in All Flavors

  Fully understanding the average core-collapse supernova requires detecting the diffuse supernova neutrino background (DSNB) in all flavors. While the DSNB $\bar{\nu}_e$ flux is near detection, and the DSNB $\nu_e$ flux […]

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  Neutrino Fast Flavor Instability in Three Dimensions

  Core-collapse supernovae and neutron star mergers are profligate producers of neutrinos that would be observable at neutrino observatories on Earth if they occur sufficiently close.

• research-publ

  Neutrino Fast Flavor Instability in Three Dimensions

  Neutrino flavor instabilities have the potential to shuffle neutrinos between electron, mu, and tau flavor states, modifying the core-collapse supernova mechanism and the heavy elements ejected from neutron star mergers. […]

• research-publ

  Statistical significance of the sterile-neutrino hypothesis in the context of reactor and gallium data

  We evaluate the statistical significance of the 3+1 sterile-neutrino hypothesis using $\nu_e$ and $\bar\nu_e$ disappearance data from reactor, solar and gallium radioactive source experiments. Concerning the latter, we investigate the […]