Change search
ReferencesLink to record
Permanent link

Direct link
Separation of electrons and protons in the GAMMA-400 gamma-ray telescope
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.ORCID iD: 0000-0003-0065-2933
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.ORCID iD: 0000-0001-7011-7229
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.ORCID iD: 0000-0002-9769-8016
Show others and affiliations
Number of Authors: 65
2015 (English)In: Advances in Space Research, ISSN 0273-1177, E-ISSN 1879-1948, Vol. 56, no 7, 1538-1545 p.Article in journal (Refereed) Published
Abstract [en]

The GAMMA-400 telescope will measure the fluxes of gamma rays and cosmic-ray electrons and positrons in the energy range from 100 MeV to several TeV. These measurements will allow it to achieve the following scientific objectives: search for signatures of dark matter, investigation of gamma-ray point-like and extended sources, study of the energy spectrum of the Galactic and extragalactic diffuse emission, study of gamma-ray bursts and gamma-ray emission from the active Sun, together with high-precision measurements of the high-energy electrons and positrons spectra, protons and nuclei up to the knee. The bulk of cosmic rays are protons and helium nuclei, whereas the lepton component in the total flux is similar to 10(-3) at high energy. In the present paper, the simulated capability of the GAMMA-400 telescope to distinguish electrons and positrons from protons in cosmic rays is addressed. The individual contribution to the proton rejection from each detector system of GAMMA-400 is studied separately. The use of the combined information from all detectors allows us to reach a proton rejection of the order of similar to 4 x 10(5) for vertical incident particles and similar to 3 x 10(5) for particles with initial inclination of 30 degrees in the electron energy range from 50 GeV to 1 TeV. (C) 2015 COSPAR. Published by Elsevier Ltd. All rights reserved.

Place, publisher, year, edition, pages
Elsevier, 2015. Vol. 56, no 7, 1538-1545 p.
Keyword [en]
Gamma-ray telescope, Hadron and electromagnetic showers, Gamma rays, Cosmic rays, Space experiments
National Category
Astronomy, Astrophysics and Cosmology Subatomic Physics
URN: urn:nbn:se:kth:diva-176852DOI: 10.1016/j.asr.2015.06.040ISI: 000361402300023ScopusID: 2-s2.0-84954053061OAI: diva2:868363

QC 20151110

Available from: 2015-11-10 Created: 2015-11-10 Last updated: 2015-11-10Bibliographically approved

Open Access in DiVA

No full text

Other links

Publisher's full textScopus

Search in DiVA

By author/editor
Larsson, JosefinPearce, MarkRyde, Felix
By organisation
Particle and Astroparticle Physics
In the same journal
Advances in Space Research
Astronomy, Astrophysics and CosmologySubatomic Physics

Search outside of DiVA

GoogleGoogle Scholar
The number of downloads is the sum of all downloads of full texts. It may include eg previous versions that are now no longer available

Altmetric score

Total: 44 hits
ReferencesLink to record
Permanent link

Direct link