Chiral Dark Sector

Raymond T. Co, Keisuke Harigaya, Yasunori Nomura

Research output: Contribution to journalArticlepeer-review

17 Scopus citations

Abstract

We present a simple and natural dark sector model in which dark matter particles arise as composite states of hidden strong dynamics and their stability is ensured by accidental symmetries. The model has only a few free parameters. In particular, the gauge symmetry of the model forbids the masses of dark quarks, and the confinement scale of the dynamics provides the unique mass scale of the model. The gauge group contains an Abelian symmetry U(1)D, which couples the dark and standard model sectors through kinetic mixing. This model, despite its simple structure, has rich and distinctive phenomenology. In the case where the dark pion becomes massive due to U(1)D quantum corrections, direct and indirect detection experiments can probe thermal relic dark matter which is generically a mixture of the dark pion and the dark baryon, and the Large Hadron Collider can discover the U(1)D gauge boson. Alternatively, if the dark pion stays light due to a specific U(1)D charge assignment of the dark quarks, then the dark pion constitutes dark radiation. The signal of this radiation is highly correlated with that of dark baryons in dark matter direct detection.

Original languageEnglish (US)
Article number101801
JournalPhysical review letters
Volume118
Issue number10
DOIs
StatePublished - Mar 7 2017
Externally publishedYes

Bibliographical note

Funding Information:
This work was supported in part by the Director, Office of Science, Office of High Energy and Nuclear Physics, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231, by the National Science Foundation under Grants No.PHY-1316783 and No. PHY-1521446, and by MEXT KAKENHI Grant No. 15H05895.

Publisher Copyright:
© 2017 American Physical Society.

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