Golden Littlest Seesaw
Golden Littlest Seesaw
We propose and analyse a new class of Littlest Seesaw models, with two right-handed neutrinos in their diagonal mass basis, based on preserving the first column of the Golden Ratio mixing matrix. We perform an exhaustive analysis of all possible remnant symmetries of the group $A_5$ which can be used to enforce various vacuum alignments for the flavon controlling solar mixing, for two simple cases of the atmospheric flavon vacuum alignment. The solar and atmospheric flavon vacuum alignments are enforced by {\em different} remnant symmetries. We examine the phenomenological viability of each of the possible Littlest Seesaw alignments in $A_5$, which preserve the first column of the Golden ratio mixing matrix, using figures and extensive tables of benchmark points and comparing our predictions to a recent global analysis of neutrino data. We also repeat the analysis for an alternative form of Golden Ratio mixing matrix.
hep-ph
470-499
Ding, Gui-Jun
65280d32-40be-4950-a54f-f130e4f8699a
King, Stephen F.
f8c616b7-0336-4046-a943-700af83a1538
Li, Cai-Chang
477970e9-f18d-42db-91f5-ab9099be6705
December 2017
Ding, Gui-Jun
65280d32-40be-4950-a54f-f130e4f8699a
King, Stephen F.
f8c616b7-0336-4046-a943-700af83a1538
Li, Cai-Chang
477970e9-f18d-42db-91f5-ab9099be6705
Abstract
We propose and analyse a new class of Littlest Seesaw models, with two right-handed neutrinos in their diagonal mass basis, based on preserving the first column of the Golden Ratio mixing matrix. We perform an exhaustive analysis of all possible remnant symmetries of the group $A_5$ which can be used to enforce various vacuum alignments for the flavon controlling solar mixing, for two simple cases of the atmospheric flavon vacuum alignment. The solar and atmospheric flavon vacuum alignments are enforced by {\em different} remnant symmetries. We examine the phenomenological viability of each of the possible Littlest Seesaw alignments in $A_5$, which preserve the first column of the Golden ratio mixing matrix, using figures and extensive tables of benchmark points and comparing our predictions to a recent global analysis of neutrino data. We also repeat the analysis for an alternative form of Golden Ratio mixing matrix.
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Accepted/In Press date: 25 October 2017
e-pub ahead of print date: 31 October 2017
Published date: December 2017
Keywords:
hep-ph
Identifiers
Local EPrints ID: 416411
URI: http://eprints.soton.ac.uk/id/eprint/416411
ISSN: 0550-3213
PURE UUID: af502ca7-3270-4164-aecc-991e3016187b
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Date deposited: 15 Dec 2017 17:30
Last modified: 15 Mar 2024 17:20
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Author:
Gui-Jun Ding
Author:
Cai-Chang Li
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