Constraining low scale dark hypercharge symmetry at spallation, reactor, and dark matter direct detection experiments

Coherent elastic neutrino-nucleus (<a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mi>CE</a:mi><a:mi>ν</a:mi><a:mi>NS</a:mi></a:mrow></a:math>) and elastic neutrino-electron scattering (<c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mrow><c:mi mathvariant="normal">E</c:mi><c:mi>ν</c:mi><c:mi>ES</c:mi></c:mrow></c:math>) data are exploited to constrain “chiral” <f:math xmlns:f="http://www.w3.org/1998/Math/MathML" display="inline"><f:mi>U</f:mi><f:mo stretchy="false">(</f:mo><f:mn>1</f:mn><f:msub><f:mo stretchy="false">)</f:mo><f:mi>X</f:mi></f:msub></f:math> gauged models with light vector mediator mass. These models fall under a distinct class of new symmetries called dark hypercharge symmetries. A key feature is the fact that the <j:math xmlns:j="http://www.w3.org/1998/Math/MathML" display="inline"><j:msup><j:mi>Z</j:mi><j:mo>′</j:mo></j:msup></j:math> boson can couple to all Standard Model fermions at tree level, with the <l:math xmlns:l="http://www.w3.org/1998/Math/MathML" display="inline"><l:mi>U</l:mi><l:mo stretchy="false">(</l:mo><l:mn>1</l:mn><l:msub><l:mo stretchy="false">)</l:mo><l:mi>X</l:mi></l:msub></l:math> charges determined by the requirement of anomaly cancellation. Notably, the charges of leptons and quarks can differ significantly depending on the specific anomaly cancellation solution. As a result, different models exhibit distinct phenomenological signatures and can be constrained through various experiments. In this work, we analyze the recent data from the COHERENT experiment, along with results from dark matter (DM) direct detection experiments such as XENONnT, LUX-ZEPLIN, and PandaX-4T, and place new constraints on three benchmark models. Additionally, we set constraints from a performed analysis of TEXONO data and discuss the prospects of improvement in view of the next-generation DM direct detection DARWIN experiment.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-04-16
DOI
https://doi.org/10.1103/physrevd.111.073006
Citations
7
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
13.09

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article

Constraining low scale dark hypercharge symmetry at spallation, reactor, and dark matter direct detection experiments

Dimitrios K. Papoulias, Anirban Majumdar, Rahul Srivastava, Hemant Prajapati
7 citations
Physical review. D/Physical review. D.
Dark Matter and Cosmic Phenomena
13.09
article

Constraining low scale dark hypercharge symmetry at spallation, reactor, and dark matter direct detection experiments

Dimitrios K. Papoulias, Anirban Majumdar, Rahul Srivastava, Hemant Prajapati
article en
7 citations

Abstract

Coherent elastic neutrino-nucleus (<a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mi>CE</a:mi><a:mi>ν</a:mi><a:mi>NS</a:mi></a:mrow></a:math>) and elastic neutrino-electron scattering (<c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mrow><c:mi mathvariant="normal">E</c:mi><c:mi>ν</c:mi><c:mi>ES</c:mi></c:mrow></c:math>) data are exploited to constrain “chiral” <f:math xmlns:f="http://www.w3.org/1998/Math/MathML" display="inline"><f:mi>U</f:mi><f:mo stretchy="false">(</f:mo><f:mn>1</f:mn><f:msub><f:mo stretchy="false">)</f:mo><f:mi>X</f:mi></f:msub></f:math> gauged models with light vector mediator mass. These models fall under a distinct class of new symmetries called dark hypercharge symmetries. A key feature is the fact that the <j:math xmlns:j="http://www.w3.org/1998/Math/MathML" display="inline"><j:msup><j:mi>Z</j:mi><j:mo>′</j:mo></j:msup></j:math> boson can couple to all Standard Model fermions at tree level, with the <l:math xmlns:l="http://www.w3.org/1998/Math/MathML" display="inline"><l:mi>U</l:mi><l:mo stretchy="false">(</l:mo><l:mn>1</l:mn><l:msub><l:mo stretchy="false">)</l:mo><l:mi>X</l:mi></l:msub></l:math> charges determined by the requirement of anomaly cancellation. Notably, the charges of leptons and quarks can differ significantly depending on the specific anomaly cancellation solution. As a result, different models exhibit distinct phenomenological signatures and can be constrained through various experiments. In this work, we analyze the recent data from the COHERENT experiment, along with results from dark matter (DM) direct detection experiments such as XENONnT, LUX-ZEPLIN, and PandaX-4T, and place new constraints on three benchmark models. Additionally, we set constraints from a performed analysis of TEXONO data and discuss the prospects of improvement in view of the next-generation DM direct detection DARWIN experiment.

Physical review. D/Physical review. D.Vol. 111(7)
Universitat de València (ES), Indian Institute of Science Education and Research, Bhopal (IN)
Ministerio de Ciencia, Innovación y Universidades, Generalitat Valenciana, Indian Institute of Science Education and Research Bhopal, Indian Institute of Science Education and Research Mohali, Agencia Estatal de Investigación
Openalex Percentile: Top 2%
Dark Matter and Cosmic Phenomena
13.09
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