Author: sylvia

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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 ΔN_eff

  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 […]

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  High-accuracy waveforms for black hole-neutron star systems with spinning black holes

  The availability of accurate numerical waveforms is an important requirement for the creation and calibration of reliable waveform models for gravitational wave astrophysics. For black hole-neutron star binaries, very few […]