1999/11/30 by Peter Milne, P. A. Milne, M. D. Leising +4
Medicine · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Nuclear Physics and Applications #Nuclear physics research studies #Radiation Therapy and Dosimetry #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9911517
8 pages, 2 figures. To appear in "Astronomy with Radioactivities", Ringberg, Germany, Sept. 1999
arxiv created 1999/11/30 · openalex publication_date 1999/11/30 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The energy deposition into the ejecta of type Ia supernovae is dominated at late times by the slowing of positrons produced in the β+ decays of 56Co. Fits of model-generated light curves to observations of type Ia supernovae suggest that a significant number of positrons escape the ejecta and annihilate as a delayed emission. In this work, the isotopic yields of the β+ decay unstable nuclei, 56Co, 44Ti & 26Al are combined with the delayed annihilation fractions of each isotope for types Ia, Ib, II supernovae to generate an estimate of the positron production rate due to supernovae. It is shown that SN produced positrons can explain a sizeable fraction of the galactic positron annihilation radiation, as measured at 511 keV by the CGRO/OSSE, SMM and TGRS instruments.