Radiative generation of non-zero <mml:math altimg="si1.gif" overflow="scroll" xmlns:xocs="http://www.elsevier.com/xml/xocs/dtd" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.elsevier.com/xml/ja/dtd" xmlns:ja="http://www.elsevier.com/xml/ja/dtd" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:tb="http://www.elsevier.com/xml/common/table/dtd" xmlns:sb="http://www.elsevier.com/xml/common/struct-bib/dtd" xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:cals="http://www.elsevier.com/xml/common/cals/dtd" xmlns:sa="http://www.elsevier.com/xml/common/struct-aff/dtd"><mml:msub><mml:mrow><mml:mi>θ</mml:mi></mml:mrow><mml:mrow><mml:mn>13</mml:mn></mml:mrow></mml:msub></mml:math> in MSSM with broken <mml:math altimg="si2.gif" overflow="scroll" xmlns:xocs="http://www.elsevier.com/xml/xocs/dtd" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.elsevier.com/xml/ja/dtd" xmlns:ja="http://www.elsevier.com/xml/ja/dtd" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:tb="http://www.elsevier.com/xml/common/table/dtd" xmlns:sb="http://www.elsevier.com/xml/common/struct-bib/dtd" xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:cals="http://www.elsevier.com/xml/common/cals/dtd" xmlns:sa="http://www.elsevier.com/xml/common/struct-aff/dtd"><mml:msub><mml:mrow><mml:mi>A</mml:mi></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow></mml:msub></mml:math> flavor symmetry-Reference-Cited by-同舟云学术

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Radiative generation of non-zero θ13 in MSSM with broken A4 flavor symmetry

Published:2014-08 Issue: Volume:885 Page:76-96
ISSN:0550-3213
Container-title:Nuclear Physics B
language:en
Short-container-title:Nuclear Physics B

Author:

Borah Manikanta,Borah Debasish,Das Mrinal Kumar

Funder

UGC

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference81 articles.

1. Constraints on Neutrino Oscillations Using 1258 Days of Super-Kamiokande Solar Neutrino Data

2. Solar models and solar neutrino oscillations

3. Review of Particle Physics

Cited by 4 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Common origin of θ13 and dark matter within the flavor symmetric scoto-seesaw framework;Journal of High Energy Physics;2022-11-14

2. Radiative generation of realistic neutrino mixing with A4;Nuclear Physics B;2021-02

3. Nonzeroθ13inSO(3)→A4lepton models;Physical Review D;2015-04-08

4. Nonzeroθ13and leptogenesis in a type-I seesaw model withA4symmetry;Physical Review D;2015-01-14

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