Neutrino Masses in Astrophysics and Cosmology
Georg G. Raffelt
Abstract
Astrophysical and cosmological arguments and observations give us the most restrictive constraints on neutrino masses, electromagnetic couplings, and other properties. Conversely, massive neutrinos would contribute to the cosmic dark-matter density and would play an important role for the formation of structure in the universe. Neutrino oscillations may well solve the solar neutrino problem, and can have a significant impact on supernova physics.
Create a lesson
Related papers
Theoretical calculations for t tH production
Nikolaos Kidonakis, Nodoka Yamanaka
BSMScanner: a lightweight framework for beyond-the-Standard-Model global fits
Mohamed Belfkir
Chiral mass corrections to decuplet hidden-charm pentaquark states
Yu-Quan Guo, Hao-Song Li
Probing eV-scale sterile neutrinos with neutrinoless double-beta decay and beta decay
Ruisha Yang, Jiajun Liao
χc0 production in Λn scattering process
Quan-Yun Guo, Zhuo Yu, Dian-Yong Chen
Mixed leptogenesis sources and low-energy neutrino portals
Yingnan Xu