Testing the universality of cosmic-ray nuclei from protons to oxygen with AMS-02
arXiv:2112.08381 · doi:10.1103/PhysRevD.105.103033
Abstract
The AMS-02 experiment has provided high-precision measurements of several cosmic-ray (CR) species. The achieved percent-level accuracy gives access to small spectral differences among the different species and, in turn, this allows scrutinizing the universality of CR acceleration, which is expected in the standard scenario of CR shock acceleration. While pre-AMS-02 data already indicated a violation of the universality between protons and helium, it is still an open question if at least helium and heavier nuclei can be reconciled. To address this issue, we performed a joint analysis using the AMS-02 CR measurements of antiprotons, protons, helium, helium 3, boron, carbon, nitrogen, and oxygen. We explore two competing propagation scenarios, one with a break in the diffusion coefficient at a few GVs and no reacceleration, and another one with reacceleration and with a break in the injection spectra of primaries. Furthermore, we explicitly consider the impact of the uncertainties in the nuclear production cross-sections of secondaries by including nuisance parameters in the fit. The resulting parameter space is explored with the help of Monte Carlo methods. We find that, contrary to the naive expectation, in the standard propagation scenarios CR universality is violated also for He, on the one hand, and C, N, and O, on the other hand, i.e., different injection slopes (at the level of ) are required to explain the observed spectra. As an alternative, we explore further propagation scenarios, inspired by non-homogeneous diffusion, which might save universality. Finally, we also investigate the universality of CR propagation, i.e., we compare the propagation properties inferred using only light nuclei (, p, He, He) with the ones inferred using only heavier nuclei (B, C, N, O).
25 pages, 9 figures; v2: results and conclusion unchanged; expanded introduction and discussion; matches accepted version by PRD
References in corpus (18)
- Discrepant hardening observed in cosmic-ray elemental spectra
- Galactic cosmic rays after the AMS-02 observations
- AMS-02 beryllium data and its implication for cosmic ray transport
- Scrutinizing the evidence for dark matter in cosmic-ray antiprotons
- Cosmic-ray transport from AMS-02 B/C data: benchmark models and interpretation
- Cosmic Ray Antiprotons at High Energies
- New calculation of antiproton production by cosmic ray protons and nuclei
- GeV-TeV cosmic-ray spectral anomaly as due to re-acceleration by weak shocks in the Galaxy
- Galactic cosmic-ray propagation in the light of AMS-02: I. Analysis of protons, helium, and antiprotons
- Galactic halo size in the light of recent AMS-02 data
- Dark matter or correlated errors: Systematics of the AMS-02 antiproton excess
- Power requirements for cosmic ray propagation models involving diffusive reacceleration; estimates and implications for the damping of interstellar turbulence
- Implications of current nuclear cross sections on secondary cosmic rays with the upcoming DRAGON2 code
- Implications of Lithium to Oxygen AMS-02 spectra on our understanding of cosmic-ray diffusion
- Stochastic Fluctuations of Low-Energy Cosmic Rays and the Interpretation of Voyager Data
- Constraints on the spatially dependent cosmic-ray propagation model from Bayesian Analysis
- Intermediate mass and heavy Galactic cosmic-ray nuclei: the case of new AMS-02 measurements
- Origin of hardening and universality of cosmic rays spectra in GV-PV rigidity region
Cited by in corpus (6)
- FLUKA cross sections for cosmic-ray interactions with the DRAGON2 code
- New determination of the production cross section for secondary positrons and electrons in the Galaxy
- Pulsars Do Not Produce Sharp Features in the Cosmic-Ray Electron and Positron Spectra
- Weighing the Local Interstellar Medium using Gamma Rays and Dust
- A Simple Sub-Grid Model For Cosmic Ray Effects on Galactic Scales
- Transport parameters from AMS-02 F/Si data and fluorine source abundance