Cosmic ray electrons and the diffuse gamma ray spectrum

dc.creatorPorter, T. A.
dc.creatorProtheroe, R. J.
dc.date1996-08-28
dc.date1997-03-26
dc.date.accessioned2026-07-07T10:57:48Z
dc.date.available2026-07-07T10:57:48Z
dc.descriptionThe bulk of the diffuse galactic gamma-ray emission above a few tens of GeV has been conventionally ascribed to the decay of neutral pions produced in cosmic-ray interactions with interstellar matter. Cosmic-ray electrons may, however, make a significant contribution to the gamma-ray spectrum at high energies, and even dominate at TeV-PeV energies depending on their injection spectral index and acceleration cut-off energy. If the injection spectrum is flat, the highest energy electrons will also contribute a diffuse hard X-ray/soft gamma-ray flux via synchrotron emission, and this may offer an explanation for the OSSE observation of a steep spectrum below a few MeV from the inner Galaxy. We perform a propagation calculation for cosmic-ray electrons, and use the resulting interstellar electron spectrum to obtain the gamma-ray spectrum due to inverse Compton, synchrotron and bremsstrahlung interactions consistently from MeV to PeV energies. We compare our results with available observations from satellite-borne telescopes, optical Cherenkov telescopes and air shower arrays and place constraints on the injection spectrum of cosmic-ray electrons. With future observations at TeV-PeV energies it should be possible to determine the average interstellar spectrum of cosmic-ray electrons, and hence estimate their spectrum on acceleration.
dc.description28 pages, 10 figures, major revision. Submitted to J. Phys. G: Nucl. Part. Phys
dc.identifierhttps://arxiv.org/abs/astro-ph/9608182
dc.identifierhttp://arxiv.org/abs/astro-ph/9608182
dc.identifierJ.Phys.G23:1765-1784,1997
dc.identifierdoi:10.1088/0954-3899/23/11/022
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186880
dc.subjectAstrophysics
dc.titleCosmic ray electrons and the diffuse gamma ray spectrum
dc.typetext

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