Speaker
Melanie Zaidel
(Ohio State University)
Description
In the coming age of precision neutrino physics, neutrinos from the Sun become robust probes of the conditions of the solar core. Here, we focus on $^8$B neutrinos, for which there are already high precision measurements by the Sudbury Neutrino Observatory and Super-Kamiokande. Using only basic physical principles and straightforward statistical tools, we calculate projected constraints on the temperature and density of the $^8$B neutrino production zone compared to a reference solar model. We outline how to better understand the astrophysics of the solar interior using forthcoming neutrino data and solar models. Our code is publicly available on Github.
Author
Melanie Zaidel
(Ohio State University)
Co-author
Dr
John Beacom
(Ohio State University)