Noninvertible symmetry as a solution to the strong <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>C</mml:mi> <mml:mi>P</mml:mi> </mml:math> problem in a GUT-inspired standard model

We propose a three-zero texture for the down-quark mass matrix within a <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mi>S</a:mi> <a:mi>U</a:mi> <a:mo stretchy="false">(</a:mo> <a:mn>5</a:mn> <a:mo stretchy="false">)</a:mo> </a:math> grand unified theory (GUT)-inspired Standard Model, enforced by a noninvertible selection rule originating from <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"> <e:msub> <e:mi mathvariant="double-struck">Z</e:mi> <e:mn>2</e:mn> </e:msub> </e:math> gauging of <h:math xmlns:h="http://www.w3.org/1998/Math/MathML" display="inline"> <h:msub> <h:mi mathvariant="double-struck">Z</h:mi> <h:mi>N</h:mi> </h:msub> </h:math> symmetries. Assuming <k:math xmlns:k="http://www.w3.org/1998/Math/MathML" display="inline"> <k:mi>C</k:mi> <k:mi>P</k:mi> </k:math> invariance at the high-energy scale, our framework solves the strong <m:math xmlns:m="http://www.w3.org/1998/Math/MathML" display="inline"> <m:mi>C</m:mi> <m:mi>P</m:mi> </m:math> problem while reproducing a realistic quark mass matrix. The <o:math xmlns:o="http://www.w3.org/1998/Math/MathML" display="inline"> <o:mi>C</o:mi> <o:mi>P</o:mi> </o:math> symmetry is spontaneously broken down at an intermediate scale via complex vacuum expectation values of new scalar fields <q:math xmlns:q="http://www.w3.org/1998/Math/MathML" display="inline"> <q:msub> <q:mi>η</q:mi> <q:mi>i</q:mi> </q:msub> </q:math> , which generate the <s:math xmlns:s="http://www.w3.org/1998/Math/MathML" display="inline"> <s:mi>C</s:mi> <s:mi>P</s:mi> </s:math> phase in the Cabibbo-Kobayashi-Maskawa matrix without inducing the quantum chromodynamics (QCD) <u:math xmlns:u="http://www.w3.org/1998/Math/MathML" display="inline"> <u:mover accent="true"> <u:mi>θ</u:mi> <u:mo stretchy="false">¯</u:mo> </u:mover> </u:math> term. The present model incorporates three generations of matter, Higgs, and additional scalars with a common structure under the noninvertible symmetry, which may be naturally embedded into <y:math xmlns:y="http://www.w3.org/1998/Math/MathML" display="inline"> <y:mi>S</y:mi> <y:mi>O</y:mi> <y:mo stretchy="false">(</y:mo> <y:mn>10</y:mn> <y:mo stretchy="false">)</y:mo> </y:math> GUTs at high energies.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2026-02-02
DOI
https://doi.org/10.1103/vbd5-5cp3
Citations
2
Primary Topic
Particle physics theoretical and experimental studies
Type
article
Field-Weighted Citation Impact
55.92
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article

Noninvertible symmetry as a solution to the strong <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>C</mml:mi> <mml:mi>P</mml:mi> </mml:math> problem in a GUT-inspired standard model

Hajime Otsuka, Anonymous, Tsutomu T. Yanagida
2 citations
Physical review. D/Physical review. D.
Particle physics theoretical and experimental studies
55.92
article

Noninvertible symmetry as a solution to the strong <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>C</mml:mi> <mml:mi>P</mml:mi> </mml:math> problem in a GUT-inspired standard model

Hajime Otsuka, Anonymous, Tsutomu T. Yanagida
article en
2 citations

Abstract

We propose a three-zero texture for the down-quark mass matrix within a <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mi>S</a:mi> <a:mi>U</a:mi> <a:mo stretchy="false">(</a:mo> <a:mn>5</a:mn> <a:mo stretchy="false">)</a:mo> </a:math> grand unified theory (GUT)-inspired Standard Model, enforced by a noninvertible selection rule originating from <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"> <e:msub> <e:mi mathvariant="double-struck">Z</e:mi> <e:mn>2</e:mn> </e:msub> </e:math> gauging of <h:math xmlns:h="http://www.w3.org/1998/Math/MathML" display="inline"> <h:msub> <h:mi mathvariant="double-struck">Z</h:mi> <h:mi>N</h:mi> </h:msub> </h:math> symmetries. Assuming <k:math xmlns:k="http://www.w3.org/1998/Math/MathML" display="inline"> <k:mi>C</k:mi> <k:mi>P</k:mi> </k:math> invariance at the high-energy scale, our framework solves the strong <m:math xmlns:m="http://www.w3.org/1998/Math/MathML" display="inline"> <m:mi>C</m:mi> <m:mi>P</m:mi> </m:math> problem while reproducing a realistic quark mass matrix. The <o:math xmlns:o="http://www.w3.org/1998/Math/MathML" display="inline"> <o:mi>C</o:mi> <o:mi>P</o:mi> </o:math> symmetry is spontaneously broken down at an intermediate scale via complex vacuum expectation values of new scalar fields <q:math xmlns:q="http://www.w3.org/1998/Math/MathML" display="inline"> <q:msub> <q:mi>η</q:mi> <q:mi>i</q:mi> </q:msub> </q:math> , which generate the <s:math xmlns:s="http://www.w3.org/1998/Math/MathML" display="inline"> <s:mi>C</s:mi> <s:mi>P</s:mi> </s:math> phase in the Cabibbo-Kobayashi-Maskawa matrix without inducing the quantum chromodynamics (QCD) <u:math xmlns:u="http://www.w3.org/1998/Math/MathML" display="inline"> <u:mover accent="true"> <u:mi>θ</u:mi> <u:mo stretchy="false">¯</u:mo> </u:mover> </u:math> term. The present model incorporates three generations of matter, Higgs, and additional scalars with a common structure under the noninvertible symmetry, which may be naturally embedded into <y:math xmlns:y="http://www.w3.org/1998/Math/MathML" display="inline"> <y:mi>S</y:mi> <y:mi>O</y:mi> <y:mo stretchy="false">(</y:mo> <y:mn>10</y:mn> <y:mo stretchy="false">)</y:mo> </y:math> GUTs at high energies.

Physical review. D/Physical review. D.Vol. 113(5)
Kyushu University (JP), Kavli Institute for the Physics and Mathematics of the Universe (JP), Shanghai Jiao Tong University (CN), Hokkaido University (JP), The University of Tokyo (JP)
Openalex Percentile: Top 0%
Particle physics theoretical and experimental studies
55.92
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