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2020

Analytic solutions for neutrino-light curves of core-collapse supernovae

Suwa, Yudai, Harada, Akira, Nakazato, Ken'ichiro et al.

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Neutrinos are a guaranteed signal from supernova explosions in the Milky Way, and a most valuable messenger that can provide us with information about the deepest parts of supernovae.

In particular, neutrinos will provide us with physical quantities, such as the radius and mass of protoneutron stars (PNS), which are the central engine of supernovae.
This requires a theoretical model that connects observables such as neutrino luminosity and average energy with physical quantities.
Here, we show analytic solutions for the neutrino-light curve derived from the neutrino radiation transport equation by employing the diffusion approximation and the analytic density solution of the hydrostatic equation for a PNS.

Analytic solutions for neutrino-light curves of core-collapse supernovae · Around

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