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).
arXiv comment25 pages, 9 figures; v2: results and conclusion unchanged; expanded introduction and discussion; matches accepted version by PRD
References in corpus (59)
- MultiNest: an efficient and robust Bayesian inference tool for cosmology and particle physics
- Cosmic-ray propagation and interactions in the Galaxy
- PAMELA Measurements of Cosmic-ray Proton and Helium Spectra
- Limits and Confidence Intervals in the Presence of Nuisance Parameters
- Diffuse continuum gamma rays from the Galaxy
- Development of the Model of Galactic Interstellar Emission for Standard Point-Source Analysis of Fermi Large Area Telescope Data
- Discrepant hardening observed in cosmic-ray elemental spectra
- Cosmic-Ray Nuclei, Antiprotons and Gamma-rays in the Galaxy: a New Diffusion Model
- Novel dark matter constraints from antiprotons in the light of AMS-02
- Bayesian analysis of cosmic-ray propagation: evidence against homogeneous diffusion
- Testing the Origin of High-Energy Cosmic Rays
- Galactic cosmic rays after the AMS-02 observations
- A Markov Chain Monte Carlo technique to sample transport and source parameters of Galactic cosmic rays: II. Results for the diffusion model combining B/C and radioactive nuclei
- Radial distribution of the diffuse gamma-ray emissivity in the galactic disk
- PICARD: A novel code for the Galactic Cosmic Ray propagation problem
- AMS-02 beryllium data and its implication for cosmic ray transport
- Scrutinizing the evidence for dark matter in cosmic-ray antiprotons
- Current status and desired accuracy of the isotopic production cross sections relevant to astrophysics of cosmic rays I. Li, Be, B, C, N
- Constraints on the distribution of supernova remnants with Galactocentric radius
- Spectra of Cosmic Ray Protons and Helium Produced in Supernova Remnants
- Inference of the Local Interstellar Spectra of Cosmic Ray Nuclei Z<=28 with the GalProp-HelMod Framework
- Cosmic-ray transport from AMS-02 B/C data: benchmark models and interpretation
- Cosmic Ray Antiprotons at High Energies
- Constraining heavy dark matter with cosmic-ray antiprotons
- Production cross sections of cosmic antiprotons in the light of new data from the NA61 and LHCb experiments
- Cosmic-ray propagation with DRAGON2: II. Nuclear interactions with the interstellar gas
- 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
- Proton-Helium Spectral Anomaly as a Signature of Cosmic Ray Accelerator
- The Three-Dimensional Spatial Distribution of Interstellar Gas in the Milky Way: Implications for Cosmic Rays and High-Energy Gamma-Ray Emissions
- Galactic cosmic-ray propagation in the light of AMS-02: I. Analysis of protons, helium, and antiprotons
- Deciphering the local Interstellar spectra of secondary nuclei with GALPROP/HelMod framework and a hint for primary lithium in cosmic rays
- Constraining Galactic cosmic-ray parameters with Z<=2 nuclei
- Measurement of antiproton production in collisions at GeV
- Galactic halo size in the light of recent AMS-02 data
- Probing dark matter annihilation in the Galaxy with antiprotons and gamma rays
- Combined analysis of AMS-02 (Li,Be,B)/C, N/O, 3He, and 4He data
- Chemical Enhancements in Shock-accelerated Particles: Ab-initio Simulations
- Dark matter or correlated errors: Systematics of the AMS-02 antiproton excess
- AMS-02 antiprotons' consistency with a secondary astrophysical origin
- USINE: semi-analytical models for Galactic cosmic-ray propagation
- Deciphering the local Interstellar spectra of primary cosmic ray species with HelMod
- Solar and nuclear physics uncertainties in cosmic-ray propagation
- Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the PAMELA experiment
- Power requirements for cosmic ray propagation models involving diffusive reacceleration; estimates and implications for the damping of interstellar turbulence
- Implications of Lithium to Oxygen AMS-02 spectra on our understanding of cosmic-ray diffusion
- Implications of current nuclear cross sections on secondary cosmic rays with the upcoming DRAGON2 code
- Origin of the Proton-to-Helium Ratio Anomaly in Cosmic Rays
- Revisiting Spatial-Dependent Propagation Model with Latest Observations of Cosmic Ray Nuclei
- Stochastic Fluctuations of Low-Energy Cosmic Rays and the Interpretation of Voyager Data
- Production of secondary particles and nuclei in cosmic rays collisions with the interstellar gas using the FLUKA code
- Prescriptions on antiproton cross section data for precise theoretical antiproton flux predictions
- On the progressive hardening of the cosmic-ray proton spectrum in the inner Galaxy
- Acceleration of Cosmic Rays in Supernova Shocks: elemental selectivity of the injection mechanism
- Constraints on the spatially dependent cosmic-ray propagation model from Bayesian Analysis
- Revisit cosmic ray propagation by using H, H, He and He
- Intermediate mass and heavy Galactic cosmic-ray nuclei: the case of new AMS-02 measurements
- Testing universality of cosmic-ray acceleration with proton/helium data from AMS and Voyager-1
- Origin of hardening and universality of cosmic rays spectra in GV-PV rigidity region
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- 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