Speaker
Sayan Ghosh
(Purdue University)
Description
In this talk I would discuss the potential detection sensitivity of XLZD towards supernova neutrino CE$\nu$NS. In addition, I would also talk on the limitations, to this detection, caused by charged current (CC) interaction of the supernova neutrinos. I would try to show that the CC interaction may in fact present a lower limit in the supernova distance that a large xenon detector can be sensitive to, without being blinded by the high energy electrons produced in the CC interactions.
Primary author
Sayan Ghosh
(Purdue University)
