Low scale leptogenesis under neutrino <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>μ</mml:mi><mml:mtext>−</mml:mtext><mml:mi>τ</mml:mi></mml:mrow></mml:math> reflection symmetry

In the literature, the neutrino <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mi>μ</a:mi><a:mo>−</a:mo><a:mi>τ</a:mi></a:math> reflection symmetry (which has the interesting predictions <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:msub><c:mi>θ</c:mi><c:mn>23</c:mn></c:msub><c:mo>=</c:mo><c:mi>π</c:mi><c:mo>/</c:mo><c:mn>4</c:mn></c:math> and <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mi>δ</e:mi><e:mo>=</e:mo><e:mo>±</e:mo><e:mi>π</e:mi><e:mo>/</e:mo><e:mn>2</e:mn></e:math> for the atmospherical neutrino mixing angle and Dirac <g:math xmlns:g="http://www.w3.org/1998/Math/MathML" display="inline"><g:mi>C</g:mi><g:mi>P</g:mi></g:math> phase) is an attractive and widely studied candidate for the flavor symmetries in the neutrino sector. However, it is known that, when the seesaw model is furnished with this symmetry, the leptogenesis mechanism (which provides an elegant explanation for the baryon-antibaryon asymmetry of the Universe) can only work in the two-flavor regime (which only holds for the right-handed neutrino masses in the range <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"><i:msup><i:mn>10</i:mn><i:mn>9</i:mn></i:msup><i:mi>–</i:mi><i:msup><i:mn>10</i:mn><i:mn>12</i:mn></i:msup><i:mtext> </i:mtext><i:mtext> </i:mtext><i:mi>GeV</i:mi></i:math>). This prohibits us to have a low scale seesaw model (which has the potential to be directly accessed by running or upcoming collider experiments) that can have the <k:math xmlns:k="http://www.w3.org/1998/Math/MathML" display="inline"><k:mi>μ</k:mi><k:mo>−</k:mo><k:mi>τ</k:mi></k:math> reflection symmetry and successful leptogenesis simultaneously. In this paper, for the first time, we demonstrate that the successful leptogenesis may also be achieved in low scale seesaw models furnished with the <m:math xmlns:m="http://www.w3.org/1998/Math/MathML" display="inline"><m:mi>μ</m:mi><m:mo>−</m:mo><m:mi>τ</m:mi></m:math> reflection symmetry, by means of the flavor nonuniversality of the conversion efficiencies from the flavored lepton asymmetries to the baryon asymmetry via the sphaleron process. We perform the study in both the resonant leptogenesis regime and the leptogenesis via oscillations (Akhmedov-Rubakov-Smirnov leptogenesis) regime.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-02-12
DOI
https://doi.org/10.1103/physrevd.111.035011
Citations
1
Primary Topic
Particle physics theoretical and experimental studies
Type
article
Field-Weighted Citation Impact
1.87

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article

Low scale leptogenesis under neutrino <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>μ</mml:mi><mml:mtext>−</mml:mtext><mml:mi>τ</mml:mi></mml:mrow></mml:math> reflection symmetry

Zhen-hua Zhao, Yan Shao
1 citations
Physical review. D/Physical review. D.
Particle physics theoretical and experimental studies
1.87
article

Low scale leptogenesis under neutrino <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>μ</mml:mi><mml:mtext>−</mml:mtext><mml:mi>τ</mml:mi></mml:mrow></mml:math> reflection symmetry

Zhen-hua Zhao, Yan Shao
article en
1 citations

Abstract

In the literature, the neutrino <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mi>μ</a:mi><a:mo>−</a:mo><a:mi>τ</a:mi></a:math> reflection symmetry (which has the interesting predictions <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:msub><c:mi>θ</c:mi><c:mn>23</c:mn></c:msub><c:mo>=</c:mo><c:mi>π</c:mi><c:mo>/</c:mo><c:mn>4</c:mn></c:math> and <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mi>δ</e:mi><e:mo>=</e:mo><e:mo>±</e:mo><e:mi>π</e:mi><e:mo>/</e:mo><e:mn>2</e:mn></e:math> for the atmospherical neutrino mixing angle and Dirac <g:math xmlns:g="http://www.w3.org/1998/Math/MathML" display="inline"><g:mi>C</g:mi><g:mi>P</g:mi></g:math> phase) is an attractive and widely studied candidate for the flavor symmetries in the neutrino sector. However, it is known that, when the seesaw model is furnished with this symmetry, the leptogenesis mechanism (which provides an elegant explanation for the baryon-antibaryon asymmetry of the Universe) can only work in the two-flavor regime (which only holds for the right-handed neutrino masses in the range <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"><i:msup><i:mn>10</i:mn><i:mn>9</i:mn></i:msup><i:mi>–</i:mi><i:msup><i:mn>10</i:mn><i:mn>12</i:mn></i:msup><i:mtext> </i:mtext><i:mtext> </i:mtext><i:mi>GeV</i:mi></i:math>). This prohibits us to have a low scale seesaw model (which has the potential to be directly accessed by running or upcoming collider experiments) that can have the <k:math xmlns:k="http://www.w3.org/1998/Math/MathML" display="inline"><k:mi>μ</k:mi><k:mo>−</k:mo><k:mi>τ</k:mi></k:math> reflection symmetry and successful leptogenesis simultaneously. In this paper, for the first time, we demonstrate that the successful leptogenesis may also be achieved in low scale seesaw models furnished with the <m:math xmlns:m="http://www.w3.org/1998/Math/MathML" display="inline"><m:mi>μ</m:mi><m:mo>−</m:mo><m:mi>τ</m:mi></m:math> reflection symmetry, by means of the flavor nonuniversality of the conversion efficiencies from the flavored lepton asymmetries to the baryon asymmetry via the sphaleron process. We perform the study in both the resonant leptogenesis regime and the leptogenesis via oscillations (Akhmedov-Rubakov-Smirnov leptogenesis) regime.

Physical review. D/Physical review. D.Vol. 111(3)
Liaoning Normal University (CN)
National Natural Science Foundation of China, Liaoning Revitalization Talents Program
Openalex Percentile: Top 16%
Particle physics theoretical and experimental studies
1.87
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