Updated Constraints on the Injection Energy of Positrons Generating the Galactic 511 keV gamma-ray line
astro-ph.HE, astro-ph.GA, hep-ph
Submitted: 2025-06-01
Updated: 2026-08-10
Comments: v2: 12+28 pages, 3+28 figures; Accepted for publication in Physical Review Letters
Journal ref: Phys. Rev. Lett. 137, 111003 (2026)
DOI: 10.1103/7v14-g7tf
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Astrophysical constraints from gamma-ray spectroscopy
- The 511 keV emission from positron annihilation in the Galaxy
- Positron Annihilation in the Galaxy
- The Positron Puzzle
- Gamma-ray spectroscopy of Positron Annihilation in the Milky Way
- Early SPI/INTEGRAL contraints on the morphology of the 511 keV line emission in the 4th galactic quadrant
- The all-sky distribution of 511 keV electron-positron annihilation emission
- The sky distribution of positronium annihilation continuum emission measured with SPI/INTEGRAL
- On the intensity and spatial morphology of the 511 keV emission in the Milky Way
- On the morphology of the electron-positron annihilation emission as seen by SPI/INTEGRAL
- Diffuse Galactic antimatter from faint thermonuclear supernovae in old stellar populations
- Galactic Positrons from Thermonuclear Supernovae
- Positron transport in the interstellar medium
- The Galactic Positron Annihilation Radiation & The Propagation of Positrons in the Interstellar Medium
- Is There a Dark Matter Signal in the Galactic Positron Annihilation Radiation?
- Positron Annihilation in the Nuclear Outflows of the Milky Way
- Measuring the smearing of the Galactic 511 keV signal: positron propagation or supernova kicks?
- Importance of cosmic ray propagation on sub-GeV dark matter constraints
- Could electron-positron annihilation lines in the Galactic center result from pulsar winds?
- Cosmic Rays from Microquasars: a Narrow Component to the CR Spectrum?
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