On atmospheric neutrino mass-squared difference in the precision era

Abstract

With the measurement of the small parameter ${\sin }^2{\theta }_{13}$ experiments on the study of neutrino oscillations enter into a high precision era. I discuss here the problem of the definition of the atmospheric mass-squared difference which will be important for analysis of data of future experiments.

6 pages, LaTeX: the text was partly changed

References in corpus (2)

• Updated fit to three neutrino mixing: status of leptonic CP violation
• Some comments on high precision study of neutrino oscillations

Cited by in corpus (1)

• Neutrino masses and mixings: Status of known and unknown $3\nu$ parameters