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- W1641922018 abstract "For a strong understanding of astrophysical annihilation radiation, especially that observed from the galactic center direction, the interaction of positrons with the ambient medium must be carefully investigated. Although hot, ionized regions may be important sources of annihilation radiation, in this report I will examine mainly the simpler processes occurring in low‐temperature neutral hydrogen gas. The goal is to set limits on conditions in the annihilation region by using the predictions of atomic theory compared with the observed γ‐ray line width, continuum strength and time dependence." @default.
- W1641922018 created "2016-06-24" @default.
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- W1641922018 date "1983-01-01" @default.
- W1641922018 modified "2023-09-27" @default.
- W1641922018 title "Low-temperature positron annihilation" @default.
- W1641922018 doi "https://doi.org/10.1063/1.34095" @default.
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