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Autor(en) / Beteiligte
Titel
Stealth dark matter: Dark scalar baryons through the Higgs portal
Ist Teil von
  • Physical review. D, Particles, fields, gravitation, and cosmology, 2015-10, Vol.92 (7), Article 075030
Ort / Verlag
United States: American Physical Society (APS)
Erscheinungsjahr
2015
Quelle
PROLA - Physical Review Online Archive
Beschreibungen/Notizen
  • We present a new model of "Stealth Dark Matter": a composite baryonic scalar of an SU(ND) strongly coupled theory with even ND ≥ 4. All mass scales are technically natural, and dark matter stability is automatic without imposing an additional discrete or global symmetry. Constituent fermions transform in vectorlike representations of the electroweak group that permit both electroweak-breaking and electroweak-preserving mass terms. This gives a tunable coupling of stealth dark matter to the Higgs boson independent of the dark matter mass itself. We specialize to SU(4), and investigate the constraints on the model from dark meson decay, electroweak precision measurements, basic collider limits, and spin-independent direct detection scattering through Higgs exchange. We exploit our earlier lattice simulations that determined the composite spectrum as well as the effective Higgs coupling of stealth dark matter in order to place bounds from direct detection, excluding constituent fermions with dominantly electroweak-breaking masses. A lower bound on the dark baryon mass mB ≳ 300 GeV is obtained from the indirect requirement that the lightest dark meson not be observable at LEP II. Furthermore, we briefly survey some intriguing properties of stealth dark matter that are worthy of future study, including collider studies of dark meson production and decay; indirect detection signals from annihilation; relic abundance estimates for both symmetric and asymmetric mechanisms; and direct detection through electromagnetic polarizability, a detailed study of which will appear in a companion paper.
Sprache
Englisch
Identifikatoren
ISSN: 1550-7998
eISSN: 1550-2368
DOI: 10.1103/PhysRevD.92.075030
Titel-ID: cdi_osti_scitechconnect_1224653
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