Axionless strong <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math> problem solution: The spontaneous <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"

We propose an alternative to the axion mechanism for addressing the charge parity (<a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mi>C</a:mi><a:mi>P</a:mi></a:math>) problem in QCD. Our approach involves imposing <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mi>C</c:mi><c:mi>P</c:mi></c:math> as an inherent symmetry of the Lagrangian, which is then spontaneously broken. To generate the correct texture for the Yukawa matrices, we introduce a discrete <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> symmetry that is softly broken by the scalar potential. By identifying a benchmark point for the Yukawa couplings that aligns with the measured quark masses, the Cabibbo-Kobayashi-Maskawa matrix, and low-energy flavor-changing constraints, our findings suggest that this model offers a viable solution to the <h:math xmlns:h="http://www.w3.org/1998/Math/MathML" display="inline"><h:mi>C</h:mi><h:mi>P</h:mi></h:math> problem.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-04-23
DOI
https://doi.org/10.1103/physrevd.111.073009
Citations
1
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
1.87

Funders

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article

Axionless strong <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math> problem solution: The spontaneous <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"

Stefano Morisi, Rodolfo Ferro-Hernández, Eduardo Peinado
1 citations
Physical review. D/Physical review. D.
Dark Matter and Cosmic Phenomena
1.87
article

Axionless strong <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:mrow></mml:math> problem solution: The spontaneous <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"

Stefano Morisi, Rodolfo Ferro-Hernández, Eduardo Peinado
article en
1 citations

Abstract

We propose an alternative to the axion mechanism for addressing the charge parity (<a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mi>C</a:mi><a:mi>P</a:mi></a:math>) problem in QCD. Our approach involves imposing <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mi>C</c:mi><c:mi>P</c:mi></c:math> as an inherent symmetry of the Lagrangian, which is then spontaneously broken. To generate the correct texture for the Yukawa matrices, we introduce a discrete <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> symmetry that is softly broken by the scalar potential. By identifying a benchmark point for the Yukawa couplings that aligns with the measured quark masses, the Cabibbo-Kobayashi-Maskawa matrix, and low-energy flavor-changing constraints, our findings suggest that this model offers a viable solution to the <h:math xmlns:h="http://www.w3.org/1998/Math/MathML" display="inline"><h:mi>C</h:mi><h:mi>P</h:mi></h:math> problem.

Physical review. D/Physical review. D.Vol. 111(7)
Istituto Nazionale di Fisica Nucleare, Sezione di Napoli (IT), Instituto Politécnico Nacional (MX), Centro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional (MX), University of Naples Federico II (IT), Universidad Nacional Autónoma de México (MX)
Fundación Marcos Moshinsky, Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México
Openalex Percentile: Top 14%
Dark Matter and Cosmic Phenomena
1.87
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