HEP-Astro Seminar | Collective Neutrino Oscillations: Challenges and Future Directions
Shashank Shalgar (University of New Mexico)
The large neutrino flux emitted during core-collapse supernovae leads to non-negligible neutrino self-interactions. The presence of neutrino self-interaction is the cause of interesting non-linear evolution of neutrino flavor. This offers a unique probe for neutrino properties. Collective neutrino oscillations are also essential for understanding some aspects of the physics of supernovae. Due to the non-linear nature of the equations of motion, there are challenges involved in the computation of flavor evolution even in the simplest case. I will discuss the physics impact of supernova neutrinos, the challenges involved, and what the future holds for the study of supernova neutrinos.
Building: | West Hall |
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Event Type: | Workshop / Seminar |
Tags: | Culture, Free, Graduate, Physics, Science, Talk, Undergraduate |
Source: | Happening @ Michigan from HEP - Astro Seminars, Department of Physics |