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Gamma-ray line emission from $^7$Li and $^7$Be production by cosmic-rays

Abstract : We calculate the total gamma-ray line emission at ~450 keV that accompanies 7-Li and 7-Be production by cosmic-ray interactions, including the delayed line emission at 0.478 MeV from 7-Be radioactive decay. We present a new gamma-ray spectroscopic test which has the potential to give direct information on the nature of the interstellar regions into which 7-Be ions propagate and decay. Finally, we evaluate the intensity of the predicted diffuse emission from the central radian of the Galaxy.
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Contributor : Jocelyne Lorgeril Connect in order to contact the contributor
Submitted on : Monday, July 17, 2006 - 2:13:32 PM
Last modification on : Thursday, October 21, 2021 - 5:10:50 AM

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V. Tatischeff, J.P. Thibaud, M. Casse, E. Vangioni-Flam. Gamma-ray line emission from $^7$Li and $^7$Be production by cosmic-rays. Integral Workshop : Exploring the Gamma-Ray Universe 4, Sep 2000, Alicante, Spain. pp.105-108. ⟨in2p3-00011207⟩



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