Author: sylvia
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Mu-Tau Neutrinos: Influencing Fast Flavor Conversions in Supernovae
Neutrinos in a core-collapse supernova can undergo fast flavor conversions with a possible impact on the explosion mechanism and nucleosynthesis. We perform the first nonlinear simulations of fast conversions in […]
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Inference of neutrino flavor evolution through data assimilation and neural differential equations
The evolution of neutrino flavor in dense environments such as core-collapse supernovae and binary compact object mergers constitutes an important and unsolved problem. Its solution has potential implications for the […]
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Mapping dynamical ejecta and disk masses from numerical relativity simulations of neutron star mergers
We present fitting formulae for the dynamical ejecta properties and remnant disk masses from a large sample of numerical relativity simulations. The considered data include some of the latest simulations […]
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Gravitational Waves from Core-Collapse Supernovae
We summarize our current understanding of gravitational wave emission from core-collapse supernovae. We review the established results from multi-dimensional simulations and, wherever possible, provide back-of-the-envelope calculations to highlight the underlying […]
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Intimate Relationship Between Sterile Neutrino Dark Matter and ΔNeff
The self-interacting neutrino hypothesis is well motivated for addressing the tension between the origin of sterile neutrino dark matter and indirect detection constraints. It can also result in a number […]