Linear sigma dark matter

Abstract We present a model of self-interacting dark matter based on QCD-like theories and inspired by the proximity of a 0(980 ± 20) to the K K ¯ $$ K\overline{K} $$ (990) threshold. Dark matter is comprised of dark pions which self-scatter via the σ resonance close to the ππ threshold. While the l...

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Main Authors: Dan Kondo, Robert McGehee, Tom Melia, Hitoshi Murayama
Format: Article
Language:English
Published: SpringerOpen 2022-09-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP09(2022)041
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author Dan Kondo
Robert McGehee
Tom Melia
Hitoshi Murayama
author_facet Dan Kondo
Robert McGehee
Tom Melia
Hitoshi Murayama
author_sort Dan Kondo
collection DOAJ
description Abstract We present a model of self-interacting dark matter based on QCD-like theories and inspired by the proximity of a 0(980 ± 20) to the K K ¯ $$ K\overline{K} $$ (990) threshold. Dark matter is comprised of dark pions which self-scatter via the σ resonance close to the ππ threshold. While the linear sigma model serves as a qualitative guide, a fully unitary description of the scattering in the strongly coupled regime is given by effective range theory. The introduction of a kinetically mixed dark photon allows the dark pion to either freeze-out or -in. We study the viable parameter space which explains the observed relic abundance while evading all current constraints. Searches for dark matter self interactions at different scales, (in)direct detection signals, and (in)visibly-decaying dark photons will test this model in the near future.
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spelling doaj.art-fab866ee25144f7a9a1dfbb31fa2f0d92022-12-22T03:12:56ZengSpringerOpenJournal of High Energy Physics1029-84792022-09-012022913610.1007/JHEP09(2022)041Linear sigma dark matterDan Kondo0Robert McGehee1Tom Melia2Hitoshi Murayama3Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, University of TokyoLeinweber Center for Theoretical Physics, Department of Physics, University of MichiganKavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, University of TokyoKavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, University of TokyoAbstract We present a model of self-interacting dark matter based on QCD-like theories and inspired by the proximity of a 0(980 ± 20) to the K K ¯ $$ K\overline{K} $$ (990) threshold. Dark matter is comprised of dark pions which self-scatter via the σ resonance close to the ππ threshold. While the linear sigma model serves as a qualitative guide, a fully unitary description of the scattering in the strongly coupled regime is given by effective range theory. The introduction of a kinetically mixed dark photon allows the dark pion to either freeze-out or -in. We study the viable parameter space which explains the observed relic abundance while evading all current constraints. Searches for dark matter self interactions at different scales, (in)direct detection signals, and (in)visibly-decaying dark photons will test this model in the near future.https://doi.org/10.1007/JHEP09(2022)041Effective Field Theories of QCDParticle Nature of Dark MatterSigma Models
spellingShingle Dan Kondo
Robert McGehee
Tom Melia
Hitoshi Murayama
Linear sigma dark matter
Journal of High Energy Physics
Effective Field Theories of QCD
Particle Nature of Dark Matter
Sigma Models
title Linear sigma dark matter
title_full Linear sigma dark matter
title_fullStr Linear sigma dark matter
title_full_unstemmed Linear sigma dark matter
title_short Linear sigma dark matter
title_sort linear sigma dark matter
topic Effective Field Theories of QCD
Particle Nature of Dark Matter
Sigma Models
url https://doi.org/10.1007/JHEP09(2022)041
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AT robertmcgehee linearsigmadarkmatter
AT tommelia linearsigmadarkmatter
AT hitoshimurayama linearsigmadarkmatter