Parameterization of the antiproton inclusive production cross section on nuclei
arXiv:astro-ph/0305274 · doi:10.1103/PhysRevD.68.094017
Abstract
A new parameterization of the antiproton inclusive production cross section in proton-proton and proton-nucleus collisions is proposed. A sample of consistent pA->pbar X$ experimental data sets measured on 1<A<208 nuclei, from 12 GeV up to 400 GeV incident energy, have been used to constrain the parameters. A broader energy domain is covered for the pp->pbar X reaction with a simplified functional form used in the fits. The agreement obtained with the data is good. The results are discussed.
10 pages, 11 figures, 7 tables, submitted to Phys. Rev. D
References in corpus (5)
- Antiprotons from primordial black holes
- Cosmic-Ray Antiprotons from Neutralino Annihilation into Gluons
- Proton and Antiproton Distributions at Mid-Rapidity in Proton-Nucleus and Sulphur-Nucleus Collisions
- Antideuteron production in proton-proton and proton-nucleus collisions
- Secondary antiproton flux induced by cosmic ray interactions with the atmosphere
Cited by in corpus (33)
- Possible dark matter annihilation signal in the AMS-02 antiproton data
- A Robust Excess in the Cosmic-Ray Antiproton Spectrum: Implications for Annihilating Dark Matter
- Heavy Wino-like Neutralino Dark Matter Annihilation into Antiparticles
- The galactic antiproton spectrum at high energies: background expectation vs. exotic contributions
- Flux of light antimatter nuclei near earth, induced by Cosmic Rays in the Galaxy and in the atmosphere
- A new evaluation of the antiproton production cross section for cosmic ray studies
- Prospects to verify a possible dark matter hint in cosmic antiprotons with antideuterons and antihelium
- Cosmic Ray Antiprotons at High Energies
- 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
- AMS-02 Antiprotons Reloaded
- The Cosmic Ray Antiproton Background for AMS-02
- Constraining the origin of the rising cosmic ray positron fraction with the boron-to-carbon ratio
- Revisit of cosmic ray antiprotons from dark matter annihilation with updated constraints on the background model from AMS-02 and collider data
- Determination of the Cosmic Antideuteron Flux in a Monte Carlo approach
- Investigating the dark matter signal in the cosmic ray antiproton flux with the machine learning method
- Possible Evidence for the Stochastic Acceleration of Secondary Antiprotons by Supernova Remnants
- Prescriptions on antiproton cross section data for precise theoretical antiproton flux predictions
- A systematic study on the cosmic ray antiproton flux
- Dark Matter after BESS-Polar II
- Galactic cosmic-ray model in the light of AMS-02 nuclei data
- Sub-GeV galactic cosmic-ray antiprotons from primordial black holes in the Randall-Sundrum braneworld
- Bayesian analysis of the break in DAMPE lepton spectra
- Deuteron and Antideuteron Production Simulation in Cosmic-ray Interactions
- Large-scale Simulations of Antihelium Production in Cosmic-ray Interactions
- Cosmic-ray antiprotons in the AMS-02 era: A sensitive probe of dark matter
- Prospects of detecting dark matter through cosmic-ray antihelium with the antiproton constraints
- A simple and natural interpretations of the DAMPE cosmic-ray electron/positron spectrum within two sigma deviations
- Some new hints on cosmic-ray propagation from AMS-02 nuclei spectra
- A model for A=3 antinuclei production in proton-nucleus collisions
- Implementation of antiproton generator in Geant4
- Combined analyses of the antiproton production from cosmic-ray interactions and its possible dark matter origin