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Fotis Koutroulis, Eugenio Megías, Stefan Pokorski | Physical review. D/Physical review. D. | (2024)
Abstract
We propose a setup for the origin of dark matter based on spacetime with a warped extra dimension and three branes: the Planck brane, the TeV brane, at a (few) TeV scale <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:msub><a:mrow><a:mi>ρ</a:mi></a:mrow><a:mrow><a:mi>T</a:mi></a:mrow></a:msub></a:mrow></a:math>, and a dark brane, at a (sub-)GeV scale <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:msub><c:mi>ρ</c:mi><c:mn>1</c:mn></c:msub><c:mo>≲</c:mo><c:mn>100</c:mn><c:mtext> </c:mtext><c:mtext> </c:mtext><c:mrow><c:mi>GeV</c:mi></c:mrow><c:mo>≪</c:mo><c:msub><c:mi>ρ</c:mi><c:mi>T</c:mi></c:msub></c:math>. The Standard Model (SM) is localized in the TeV brane, thus solving the Higgs hierarchy problem, while the dark matter <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mi>χ</e:mi></e:math>, a Dirac fermion with mass <g:math xmlns:g="http://www.w3.org/1998/Math/MathML" display="inline"><g:msub><g:mi>m</g:mi><g:mi>χ</g:mi></g:msub><g:mo><</g:mo><g:msub><g:mi>ρ</g:mi><g:mn>1</g:mn></g:msub></g:math>, is localized in the dark brane. The radion, with mass <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"><i:msub><i:mi>m</i:mi><i:mi>r</i:mi></i:msub><i:mo><</i:mo><i:msub><i:mi>m</i:mi><i:mi>χ</i:mi></i:msub></i:math>, interacts strongly [<k:math xmlns:k="http://www.w3.org/1998/Math/MathML" display="inline"><k:mrow><k:mo>∼</k:mo><k:msub><k:mrow><k:mi>m</k:mi></k:mrow><k:mrow><k:mi>χ</k:mi></k:mrow></k:msub><k:mo>/</k:mo><k:msub><k:mrow><k:mi>ρ</k:mi></k:mrow><k:mrow><k:mn>1</k:mn></k:mrow></k:msub><k:mo>∼</k:mo><k:mi mathvariant="script">O</k:mi><k:mo stretchy="false">(</k:mo><k:mn>1</k:mn><k:mo stretchy="false">)</k:mo></k:mrow></k:math>] with dark matter and very weakly (<p:math xmlns:p="http://www.w3.org/1998/Math/MathML" display="inline"><p:mo>∼</p:mo><p:msub><p:mi>m</p:mi><p:mi>f</p:mi></p:msub><p:msub><p:mi>ρ</p:mi><p:mn>1</p:mn></p:msub><p:mo>/</p:mo><p:msubsup><p:mi>ρ</p:mi><p:mi>T</p:mi><p:mn>2</p:mn></p:msubsup><p:mo>≪</p:mo><p:mn>1</p:mn></p:math>) with the Standard Model matter <r:math xmlns:r="http://www.w3.org/1998/Math/MathML" display="inline"><r:mi>f</r:mi></r:math>. The generic conflict between the bounds on its detection signatures and its proper relic abundance is avoided as dark matter annihilation is <t:math xmlns:t="http://www.w3.org/1998/Math/MathML" display="inline"><t:mi>p</t:mi></t:math>-wave suppressed. The former is determined by its very weak interactions with the SM and the latter by its much stronger annihilation into radions. Therefore, there is a vast range in the dark matter’s parameter space where the correct relic abundance is achieved consistently with the existing bounds. Moreover, for the dark brane with <v:math xmlns:v="http://www.w3.org/1998/Math/MathML" display="inline"><v:msub><v:mi>ρ</v:mi><v:mn>1</v:mn></v:msub><v:mo>≲</v:mo><v:mn>3</v:mn><v:mtext> </v:mtext><v:mtext> </v:mtext><v:mi>GeV</v:mi></v:math>, a confinement/deconfinement first order phase transition, where the radion condensates, produces a stochastic gravitational wave background at the nanohertz frequencies, which can be identified with the signal detected by the Pulsar Timing Array (PTA) experiments. In the PTA window, for <x:math xmlns:x="http://www.w3.org/1998/Math/MathML" display="inline"><x:mn>0.15</x:mn><x:mo>≲</x:mo><x:msub><x:mi>m</x:mi><x:mi>χ</x:mi></x:msub><x:mo>≲</x:mo><x:mn>2</x:mn><x:mtext> </x:mtext><x:mtext> </x:mtext><x:mi>GeV</x:mi></x:math> the relic abundance is reproduced and all constraints are satisfied. Published by the American Physical Society 2024
Tags
Sample Definition And Size
The study proposes a theoretical model involving a warped extra-dimensional spacetime with three branes: the Planck brane, the TeV brane (at a few TeV scale), and a dark brane (at sub-GeV to ~100 GeV scale). Dark matter is modeled as a Dirac fermion χ localized on the dark brane, with mass m_χ < ρ₁. No empirical sample size is involved, as this is a theoretical physics model rather than an experimental or observational study. The paper is not a meta-analysis or literature review.
Study Type
This is a theoretical model-building study in high-energy physics, specifically proposing a new framework for dark matter within a warped extra-dimensional scenario involving three branes. It includes analytical derivations and phenomenological implications.
Conflicts Of Interest
No conflicts of interest are declared in the publication. The article is published under the Creative Commons Attribution 4.0 International license and funded by SCOAP³, with no competing interests noted.
Results Summary
Key findings include: (1) Dark matter annihilation is p-wave suppressed, allowing consistency between relic abundance and detection constraints due to strong annihilation into radions and very weak interactions with Standard Model matter. (2) For dark brane scale ρ₁ ≲ 3 GeV, a first-order confinement/deconfinement phase transition produces a stochastic gravitational wave background at nanohertz frequencies, potentially matching signals observed by Pulsar Timing Array experiments. (3) In the PTA window, for 0.15 GeV ≲ m_χ ≲ 2 GeV, the model reproduces the correct relic abundance while satisfying all constraints. No explicit numerical p-values, effect sizes, or confidence intervals are provided, as the results are theoretical and qualitative/parametric in nature.
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