Kavli Affiliate: Shunsaku Horiuchi | Summary:Sterile neutrinos can be produced through mixing with active neutrinos in the hot, dense core of a core-collapse supernova (SN). The standard bounds on the active-sterile mixing ($sin^2 θ$) from SN arise from SN1987A energy-loss, requiring $E_textloss<10^52~rm erg$. In this work, we discuss a novel bound on sterile neutrino parameter […]
Continue.. Low-Energy Supernovae Bounds on Sterile Neutrinos