Requiem for a fractionally charged, massive particle

Paul George Langacker, Gary Steigman

Research output: Contribution to journalArticle

36 Scopus citations

Abstract

Fractionally charged massive particles (FCHAMPs) appear in extensions of the standard model, especially those with superstring constructions. The lightest FCHAMP would be absolutely stable and any of them produced during the early evolution of the Universe would be present today. The thermal production, annihilation and, survival of an FCHAMP, a lepton L with electroweak (i.e., U(1)Y) but no strong interactions, of mass mL and charge QL (in units of the charge on the electron) are explored. The FCHAMP relic abundance is determined by the total annihilation cross section which depends on mL, QL and on the available annihilation channels. Since massive (mL≳1GeV) charged particles (Q L≳0.01) behave like baryons (heavy ions), primordial nucleosynthesis and the cosmic background radiation temperature anisotropies limit the FCHAMP relic density. Requiring that ΩL≲Ω B/5 leads to a constraint on the QL-mL relation. Further constraints on QL and mL are provided by the invisible width of the Z (QL>0.16 for mL≤M Z/2) and by accelerator searches for massive, charged particles. Our key result is to exploit the fact that in the early Universe, after L ± freeze-out but prior to e± recombination, the negatively charged L- will combine with the more abundant alpha particles and protons to form tightly bound, positively charged states (fractionally charged heavy ions). The Coulomb barriers between these positively charged L-α and L-p (L-pp, L -αα,⋯) bound states and the free L+ suppresses late-time FCHAMP annihilation in the interstellar medium (ISM) of the Galaxy and on Earth, limiting significantly the late-time reduction of the FCHAMP abundance compared to its relic value. The surviving FCHAMP abundance on Earth is orders of magnitude higher than the limits from terrestrial searches for fractionally charged particles, closing the window on FCHAMPs with Q L≳0.01. However, as QL approaches an integer (e.g., |QL-n|≲0.25) these searches become increasingly insensitive, leaving some potentially unconstrained "islands" in the Q L-mL plane which may be explored by searching for FCHAMPs in the cosmic rays.

Original languageEnglish (US)
Article number065040
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume84
Issue number6
DOIs
StatePublished - Sep 30 2011

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

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