Neutrino masses and leptonic CP violation

Sin Kyu Kang; C. S. Kim; J. D. Kim

doi:10.1103/PhysRevD.62.073011

Neutrino masses and leptonic CP violation

Sin Kyu Kang, C. S. Kim, J. D. Kim

School of Natural Sciences

Research output: Contribution to journal › Article › peer-review

15 Scopus citations

Abstract

Neutrino oscillations as solutions of the solar neutrino problems and the atmospheric neutrino deficits may restrict neutrino mass squared differences and mixing angles in the three-neutrino mixing scheme. Currently we have several solutions depending on the interpretation of the solar neutrino problem. Combining the neutrino oscillation solutions and a mass matrix ansatz, we investigate the neutrino mass bounds and find a possible leptonic CP-violating rephasing-invariant quantity J_CP^l≤0.012 for the large mixing angle MSW and just-so vacuum oscillation solutions, and J_CP^l≤0.0013 for the small mixing angle MSW solution.

Original language	English
Article number	073011
Pages (from-to)	1-7
Number of pages	7
Journal	Physical Review D
Volume	62
Issue number	7
DOIs	https://doi.org/10.1103/PhysRevD.62.073011
State	Published - 1 Oct 2000

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10.1103/PhysRevD.62.073011

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abstract = "Neutrino oscillations as solutions of the solar neutrino problems and the atmospheric neutrino deficits may restrict neutrino mass squared differences and mixing angles in the three-neutrino mixing scheme. Currently we have several solutions depending on the interpretation of the solar neutrino problem. Combining the neutrino oscillation solutions and a mass matrix ansatz, we investigate the neutrino mass bounds and find a possible leptonic CP-violating rephasing-invariant quantity JCPl≤0.012 for the large mixing angle MSW and just-so vacuum oscillation solutions, and JCPl≤0.0013 for the small mixing angle MSW solution.",

author = "Kang, \{Sin Kyu\} and Kim, \{C. S.\} and Kim, \{J. D.\}",

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N2 - Neutrino oscillations as solutions of the solar neutrino problems and the atmospheric neutrino deficits may restrict neutrino mass squared differences and mixing angles in the three-neutrino mixing scheme. Currently we have several solutions depending on the interpretation of the solar neutrino problem. Combining the neutrino oscillation solutions and a mass matrix ansatz, we investigate the neutrino mass bounds and find a possible leptonic CP-violating rephasing-invariant quantity JCPl≤0.012 for the large mixing angle MSW and just-so vacuum oscillation solutions, and JCPl≤0.0013 for the small mixing angle MSW solution.

AB - Neutrino oscillations as solutions of the solar neutrino problems and the atmospheric neutrino deficits may restrict neutrino mass squared differences and mixing angles in the three-neutrino mixing scheme. Currently we have several solutions depending on the interpretation of the solar neutrino problem. Combining the neutrino oscillation solutions and a mass matrix ansatz, we investigate the neutrino mass bounds and find a possible leptonic CP-violating rephasing-invariant quantity JCPl≤0.012 for the large mixing angle MSW and just-so vacuum oscillation solutions, and JCPl≤0.0013 for the small mixing angle MSW solution.

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Neutrino masses and leptonic CP violation

Abstract

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