A new universal cosmic-ray knee near the magnetic rigidity 10 TV with the NUCLEON space observatory
arXiv:1805.07119 · doi:10.1134/S0021364018130015
Abstract
Data from the NUCLEON space observatory give a strong indication of the existence of a new universal cosmic ray "knee", which is observed in all groups of nuclei, including heavy nuclei, near a magnetic rigidity of about 10\,TV. Universality means the same position of the knee in the magnetic rigidity scale for all groups of nuclei. The knee is observed by both methods of measurement of particles energy implemented in the NUCLEON observatory---the calorimetric method and the kinematic method KLEM. This new cosmic ray "knee" is probably connected with the limit of acceleration of cosmic rays by some generic or nearby source of cosmic rays.
arXiv comment12 pages, 4 figures, 4 pages of Supplemental material (pictures). References improved
References in corpus (9)
- PAMELA Measurements of Cosmic-ray Proton and Helium Spectra
- On the knee in the energy spectrum of cosmic rays
- Discrepant hardening observed in cosmic-ray elemental spectra
- Cosmic-Ray Proton and Helium Spectra from the First CREAM Flight
- Proton and Helium Spectra from the CREAM-III Flight
- Measurements of Primary and Atmospheric Cosmic-Ray Spectra with the BESS-TeV Spectrometer
- Three component model of cosmic ray spectra from 10 GeV to 100 PeV
- The Cosmic-Ray Proton and Helium Spectra measured with the CAPRICE98 balloon experiment
- First results of the cosmic ray NUCLEON experiment
Cited by in corpus (39)
- Measurement of the cosmic-ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite
- Direct Measurement of the Cosmic-Ray Proton Spectrum from 50 GeV to 10 TeV with the Calorimetric Electron Telescope on the International Space Station
- Inference of the Local Interstellar Spectra of Cosmic Ray Nuclei Z<=28 with the GalProp-HelMod Framework
- Observation of Spectral Structures in the Flux of Cosmic-Ray Protons from 50 GeV to 60 TeV with the Calorimetric Electron Telescope on the International Space Station
- Cosmic Ray Models
- The shape of the cosmic ray proton spectrum
- Galactic diffuse gamma rays meet the PeV frontier
- Direct Measurement of the Cosmic-Ray Helium Spectrum from 40 GeV to 250 TeV with the Calorimetric Electron Telescope on the International Space Station
- Indication of nearby source signatures of cosmic rays from energy spectra and anisotropies
- Gamma rays as probes of cosmic-ray propagation and interactions in galaxies
- Revisiting Spatial-Dependent Propagation Model with Latest Observations of Cosmic Ray Nuclei
- Constraining light dark matter upscattered by ultrahigh-energy cosmic rays
- Anisotropies of different mass compositions of cosmic rays
- The TeV Cosmic Ray Bump: a Message from Epsilon Indi or Epsilon Eridani Star?
- Galactic diffuse gamma-ray emission from GeV to PeV energies in light of up-to-date cosmic ray measurements
- Nearby source interpretation of differences among light and medium composition spectra in cosmic rays
- Cosmic ray spectrum of protons plus helium nuclei between 6 TeV and 158 TeV from HAWC data
- Where are Milky Way's Hadronic PeVatrons?
- On the origin of observed cosmic ray spectrum below 100 TV
- Implications on the origin of cosmic rays in light of 10 TV spectral softenings
- DAMPE proton spectrum indicates a slow-diffusion zone in the nearby ISM
- A diffusive origin for the cosmic-ray spectral hardening reveals signatures of a nearbysource in the leptons and protons data
- A deep learning method for the trajectory reconstruction of cosmic rays with the DAMPE mission
- Correction Method for the Readout Saturation of the DAMPE Calorimeter
- A Three-component Model for Cosmic-ray Spectrum and Dipole Anisotropy
- Statistically study the optimal local sources for cosmic ray nuclei and electron
- Precise measurements of the cosmic ray proton energy spectrum in the "knee'' region
- Local interstellar spectra and solar modulation of cosmic ray electrons and positrons
- Implications of a Possible Spectral Structure of Cosmic-ray Protons Unveiled by the DAMPE
- Explanation of nearby SNRs for primary electron excess and proton spectral bump
- Injection spectra of different species of cosmic rays from AMS-02, ACE-CRIS and Voyager-1
- Escape of cosmic rays from perpendicular shocks in the circumstellar magnetic field
- Galactic diffuse emission from radio to ultra-high-energy gamma rays in light of up-to-date cosmic ray measurements
- A new break near 10 TeV in the energy spectrum of protons according to data from space-based instruments: astrophysical interpretation
- LHAASO Galactic Plane -rays Strongly Constrain Heavy Dark Matter
- Joint constraint on the propagation origin of the cosmic-ray spectral knee from energy spectrum and anisotropy observations
- Research on electron and positron spectrum in the high-energy region based on the gluon condensation model
- Escape of cosmic rays from perpendicular shocks in the interstellar magnetic field
- Deciphering the spectral bumps of Galactic cosmic rays through gamma-ray observations of nearby molecular clouds