Author: sylvia

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  Neutrinoless double beta decay in effective field theory

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  Multi-messenger astronomy with high-energy neutrinos

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  Properties of the neutron star crust: Quantifying and correlating uncertainties with improved nuclear physics

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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 […]