What do the highest-energy cosmic-ray data suggest about possible new physics around 50 TeV?
Abstract
The latest observations of extensive air showers (EASs) induced by ultrahigh-energy cosmic rays appear to indicate, prima facie, a transition to heavy primaries at the highest energies. However, this interpretation is based on extrapolations of the Standard Model (SM) to ultra-LHC energies. We consider the alternative that after some energy threshold, the first collision of the primary in the atmosphere results in a state, the decay of which leads to a considerably increased shower particle multiplicity, so that light-primary EASs appear heavy-like. We show that a minimal implementation of such a model yields predictions for the average EAS depth and shower-to-shower fluctuations that are consistent with each other, and an excellent fit to Auger data. If such an effect indeed takes place, we predict that (a) the center-of-momentum (c.m.) energy threshold for the effect is of order 50 TeV; (b) the probability with which the effect occurs is high, and it will be detected easily by next-generation accelerators; (c) the increase in multiplicity compared to the SM prediction grows with c.m. energy roughly as ∼ECM; and (d) the cosmic-ray composition at the highest energies is light. Remarkably, if the latter is confirmed electromagnetically, this would necessitate the existence of new physics by these energies.
- Publication:
-
Physical Review D
- Pub Date:
- June 2019
- DOI:
- 10.1103/PhysRevD.99.123016
- arXiv:
- arXiv:1802.04806
- Bibcode:
- 2019PhRvD..99l3016P
- Keywords:
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- Astrophysics - High Energy Astrophysical Phenomena;
- High Energy Physics - Phenomenology
- E-Print:
- 5 pages, 2 figures