Comment on “A three-loop radiative neutrino mass model with dark matter” [Phys. Lett. B 741 (2015) 163]
We revisit the calculation of the three-loop diagrams for the radiative neutrino mass generation and consider some relevant constraints on the model recently proposed by Jin et al. (2015) [1]. We find that the previous approximation is inappropriate due to the neglect of some important contributions...
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doaj-fa03babb6abc422da2a682ea3d6c3fd52020-11-24T21:39:02ZengElsevierPhysics Letters B0370-26932015-05-017455657Comment on “A three-loop radiative neutrino mass model with dark matter” [Phys. Lett. B 741 (2015) 163]Chao-Qiang Geng0Da Huang1Lu-Hsing Tsai2Chongqing University of Posts & Telecommunications, Chongqing, 400065, China; Department of Physics, National Tsing Hua University, Hsinchu, Taiwan; Physics Division, National Center for Theoretical Sciences, Hsinchu, Taiwan; Corresponding author.Department of Physics, National Tsing Hua University, Hsinchu, Taiwan; Physics Division, National Center for Theoretical Sciences, Hsinchu, TaiwanDepartment of Physics, National Tsing Hua University, Hsinchu, Taiwan; Physics Division, National Center for Theoretical Sciences, Hsinchu, TaiwanWe revisit the calculation of the three-loop diagrams for the radiative neutrino mass generation and consider some relevant constraints on the model recently proposed by Jin et al. (2015) [1]. We find that the previous approximation is inappropriate due to the neglect of some important contributions, and the benchmark point proposed can neither give rise to enough neutrino masses nor accommodate these additional constraints, such as the validity of the perturbation theory, the electroweak precision measurements, and the neutrinoless double beta decays.http://www.sciencedirect.com/science/article/pii/S0370269315002774 |
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DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Chao-Qiang Geng Da Huang Lu-Hsing Tsai |
spellingShingle |
Chao-Qiang Geng Da Huang Lu-Hsing Tsai Comment on “A three-loop radiative neutrino mass model with dark matter” [Phys. Lett. B 741 (2015) 163] Physics Letters B |
author_facet |
Chao-Qiang Geng Da Huang Lu-Hsing Tsai |
author_sort |
Chao-Qiang Geng |
title |
Comment on “A three-loop radiative neutrino mass model with dark matter” [Phys. Lett. B 741 (2015) 163] |
title_short |
Comment on “A three-loop radiative neutrino mass model with dark matter” [Phys. Lett. B 741 (2015) 163] |
title_full |
Comment on “A three-loop radiative neutrino mass model with dark matter” [Phys. Lett. B 741 (2015) 163] |
title_fullStr |
Comment on “A three-loop radiative neutrino mass model with dark matter” [Phys. Lett. B 741 (2015) 163] |
title_full_unstemmed |
Comment on “A three-loop radiative neutrino mass model with dark matter” [Phys. Lett. B 741 (2015) 163] |
title_sort |
comment on “a three-loop radiative neutrino mass model with dark matter” [phys. lett. b 741 (2015) 163] |
publisher |
Elsevier |
series |
Physics Letters B |
issn |
0370-2693 |
publishDate |
2015-05-01 |
description |
We revisit the calculation of the three-loop diagrams for the radiative neutrino mass generation and consider some relevant constraints on the model recently proposed by Jin et al. (2015) [1]. We find that the previous approximation is inappropriate due to the neglect of some important contributions, and the benchmark point proposed can neither give rise to enough neutrino masses nor accommodate these additional constraints, such as the validity of the perturbation theory, the electroweak precision measurements, and the neutrinoless double beta decays. |
url |
http://www.sciencedirect.com/science/article/pii/S0370269315002774 |
work_keys_str_mv |
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