Toward UV models of kinetic mixing and portal matter. VII. A light dark photon in the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mn>3</mml:mn><mml:mi>c</mml:mi></mml:msub><mml:msub><mml:mn>3</mml:mn><mml:

The kinetic mixing (KM) portal, by which the Standard Model (SM) photon mixes with a light dark photon arising from a new <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mi>U</a:mi><a:mo stretchy="false">(</a:mo><a:mn>1</a:mn><a:msub><a:mo stretchy="false">)</a:mo><a:mi>D</a:mi></a:msub></a:math> gauge group, allows for the possibility of viable scenarios of sub-GeV thermal dark matter with appropriately suppressed couplings to the SM. This KM can only occur if particles having both SM and dark quantum numbers, here termed portal matter, also exist. The presence of such types of states and the strong suggestion of a need to embed <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mi>U</e:mi><e:mo stretchy="false">(</e:mo><e:mn>1</e:mn><e:msub><e:mo stretchy="false">)</e:mo><e:mi>D</e:mi></e:msub></e:math> into a non-Abelian gauge structure not too far above the TeV scale based on the renormalization-group equation running of the <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"><i:mi>U</i:mi><i:mo stretchy="false">(</i:mo><i:mn>1</i:mn><i:msub><i:mo stretchy="false">)</i:mo><i:mi>D</i:mi></i:msub></i:math> gauge coupling is potentially indicative of an enlarged group linking together the visible and dark sectors. The gauge group <m:math xmlns:m="http://www.w3.org/1998/Math/MathML" display="inline"><m:mi>G</m:mi><m:mo>=</m:mo><m:mi>S</m:mi><m:mi>U</m:mi><m:mo stretchy="false">(</m:mo><m:mn>3</m:mn><m:msub><m:mo stretchy="false">)</m:mo><m:mi>c</m:mi></m:msub><m:mo>×</m:mo><m:mi>S</m:mi><m:mi>U</m:mi><m:mo stretchy="false">(</m:mo><m:mn>3</m:mn><m:msub><m:mo stretchy="false">)</m:mo><m:mi>L</m:mi></m:msub><m:mo>×</m:mo><m:mi>U</m:mi><m:mo stretchy="false">(</m:mo><m:mn>1</m:mn><m:msub><m:mo stretchy="false">)</m:mo><m:mi>A</m:mi></m:msub><m:mo>×</m:mo><m:mi>U</m:mi><m:mo stretchy="false">(</m:mo><m:mn>1</m:mn><m:msub><m:mo stretchy="false">)</m:mo><m:mi>B</m:mi></m:msub><m:mo>=</m:mo><m:msub><m:mn>3</m:mn><m:mi>c</m:mi></m:msub><m:msub><m:mn>3</m:mn><m:mi>L</m:mi></m:msub><m:msub><m:mn>1</m:mn><m:mi>A</m:mi></m:msub><m:msub><m:mn>1</m:mn><m:mi>B</m:mi></m:msub></m:math> is perhaps the simplest setup wherein the SM and dark interactions are partially unified in a non-Abelian fashion that is not a simple product group of the form <w:math xmlns:w="http://www.w3.org/1998/Math/MathML" display="inline"><w:mi>G</w:mi><w:mo>=</w:mo><w:msub><w:mi>G</w:mi><w:mi>SM</w:mi></w:msub><w:mo>×</w:mo><w:msub><w:mi>G</w:mi><w:mi>D</w:mi></w:msub></w:math> encountered frequently in earlier work. The present paper describes the implications and phenomenology of this type of setup.

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Journal
Physical review. D/Physical review. D.
Published
2025-04-14
DOI
https://doi.org/10.1103/physrevd.111.075018
Citations
2
Primary Topic
Dark Matter and Cosmic Phenomena
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article
Field-Weighted Citation Impact
3.74

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article

Toward UV models of kinetic mixing and portal matter. VII. A light dark photon in the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mn>3</mml:mn><mml:mi>c</mml:mi></mml:msub><mml:msub><mml:mn>3</mml:mn><mml:

Thomas G. Rizzo
2 citations
Physical review. D/Physical review. D.
Dark Matter and Cosmic Phenomena
3.74
article

Toward UV models of kinetic mixing and portal matter. VII. A light dark photon in the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mn>3</mml:mn><mml:mi>c</mml:mi></mml:msub><mml:msub><mml:mn>3</mml:mn><mml:

Thomas G. Rizzo
article en
2 citations

Abstract

The kinetic mixing (KM) portal, by which the Standard Model (SM) photon mixes with a light dark photon arising from a new <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mi>U</a:mi><a:mo stretchy="false">(</a:mo><a:mn>1</a:mn><a:msub><a:mo stretchy="false">)</a:mo><a:mi>D</a:mi></a:msub></a:math> gauge group, allows for the possibility of viable scenarios of sub-GeV thermal dark matter with appropriately suppressed couplings to the SM. This KM can only occur if particles having both SM and dark quantum numbers, here termed portal matter, also exist. The presence of such types of states and the strong suggestion of a need to embed <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mi>U</e:mi><e:mo stretchy="false">(</e:mo><e:mn>1</e:mn><e:msub><e:mo stretchy="false">)</e:mo><e:mi>D</e:mi></e:msub></e:math> into a non-Abelian gauge structure not too far above the TeV scale based on the renormalization-group equation running of the <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"><i:mi>U</i:mi><i:mo stretchy="false">(</i:mo><i:mn>1</i:mn><i:msub><i:mo stretchy="false">)</i:mo><i:mi>D</i:mi></i:msub></i:math> gauge coupling is potentially indicative of an enlarged group linking together the visible and dark sectors. The gauge group <m:math xmlns:m="http://www.w3.org/1998/Math/MathML" display="inline"><m:mi>G</m:mi><m:mo>=</m:mo><m:mi>S</m:mi><m:mi>U</m:mi><m:mo stretchy="false">(</m:mo><m:mn>3</m:mn><m:msub><m:mo stretchy="false">)</m:mo><m:mi>c</m:mi></m:msub><m:mo>×</m:mo><m:mi>S</m:mi><m:mi>U</m:mi><m:mo stretchy="false">(</m:mo><m:mn>3</m:mn><m:msub><m:mo stretchy="false">)</m:mo><m:mi>L</m:mi></m:msub><m:mo>×</m:mo><m:mi>U</m:mi><m:mo stretchy="false">(</m:mo><m:mn>1</m:mn><m:msub><m:mo stretchy="false">)</m:mo><m:mi>A</m:mi></m:msub><m:mo>×</m:mo><m:mi>U</m:mi><m:mo stretchy="false">(</m:mo><m:mn>1</m:mn><m:msub><m:mo stretchy="false">)</m:mo><m:mi>B</m:mi></m:msub><m:mo>=</m:mo><m:msub><m:mn>3</m:mn><m:mi>c</m:mi></m:msub><m:msub><m:mn>3</m:mn><m:mi>L</m:mi></m:msub><m:msub><m:mn>1</m:mn><m:mi>A</m:mi></m:msub><m:msub><m:mn>1</m:mn><m:mi>B</m:mi></m:msub></m:math> is perhaps the simplest setup wherein the SM and dark interactions are partially unified in a non-Abelian fashion that is not a simple product group of the form <w:math xmlns:w="http://www.w3.org/1998/Math/MathML" display="inline"><w:mi>G</w:mi><w:mo>=</w:mo><w:msub><w:mi>G</w:mi><w:mi>SM</w:mi></w:msub><w:mo>×</w:mo><w:msub><w:mi>G</w:mi><w:mi>D</w:mi></w:msub></w:math> encountered frequently in earlier work. The present paper describes the implications and phenomenology of this type of setup.

Physical review. D/Physical review. D.Vol. 111(7)
SLAC National Accelerator Laboratory (US)
U.S. Department of Energy, Brookhaven National Laboratory
Openalex Percentile: Top 8%
Dark Matter and Cosmic Phenomena
3.74
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