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Possible evidence for the stochastic acceleration of secondary antiprotons by supernova remnants

Journal Article · · Physical Review D
 [1];  [2];  [3]
  1. The Johns Hopkins Univ., Baltimore, MD (United States)
  2. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, Chicago, IL (United States)
  3. The Ohio State Univ., Columbus, OH (United States)
In this paper, the antiproton-to-proton ratio in the cosmic-ray spectrum is a sensitive probe of new physics. Using recent measurements of the cosmic-ray antiproton and proton fluxes in the energy range of 1–1000 GeV, we study the contribution to the $$\bar{p}$$/p ratio from secondary antiprotons that are produced and subsequently accelerated within individual supernova remnants. We consider several well-motivated models for cosmic-ray propagation in the interstellar medium and marginalize our results over the uncertainties related to the antiproton production cross section and the time-, charge-, and energy-dependent effects of solar modulation. We find that the increase in the $$\bar{p}$$/p ratio observed at rigidities above ~100 GV cannot be accounted for within the context of conventional cosmic-ray propagation models, but is consistent with scenarios in which cosmic-ray antiprotons are produced and subsequently accelerated by shocks within a given supernova remnant. In light of this, the acceleration of secondary cosmic rays in supernova remnants is predicted to substantially contribute to the cosmic-ray positron spectrum, accounting for a significant fraction of the observed positron excess.
Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE; USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
Grant/Contract Number:
AC02-07CH11359; SC0009924
OSTI ID:
1345609
Alternate ID(s):
OSTI ID: 1363982
Report Number(s):
FERMILAB-PUB--17-010-A; arXiv:1701.04406; 1509337
Journal Information:
Physical Review D, Journal Name: Physical Review D Journal Issue: 12 Vol. 95; ISSN PRVDAQ; ISSN 2470-0010
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

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Cited By (5)

Constraining heavy dark matter with cosmic-ray antiprotons journal April 2018
HAWC observations strongly favor pulsar interpretations of the cosmic-ray positron excess journal November 2017
A robust excess in the cosmic-ray antiproton spectrum: Implications for annihilating dark matter journal May 2019
HAWC Observations Strongly Favor Pulsar Interpretations of the Cosmic-Ray Positron Excess text January 2017
A Robust Excess in the Cosmic-Ray Antiproton Spectrum: Implications for Annihilating Dark Matter text January 2019

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