Cosmic-ray transport and gamma-ray emission in M31
Abstract
Here we study the possibility that an extended cosmic-ray leptonic and/or hadronic halo is at the origin of the large-scale gamma-ray emission detected from the Andromeda galaxy (M31). We consider a broad ensemble of nonhomogeneous diffusion scenarios and of cosmic-ray injection sources. We find that cosmic-ray electrons and protons could be, and very likely are, responsible for part, or all, of the gamma-ray emission from M31, including out to more than 100 kpc from the center of the galaxy. We also simulate possible emission from pulsars in M31 and consider the effect of regions of highly inefficient diffusion around cosmic-ray acceleration sites, as suggested by recent TeV halo observations with Cherenkov telescopes.
- Authors:
-
- University of California, Santa Cruz, CA (United States)
- Kinard Lab of Physics, Clemson, SC (United States)
- University of California, Santa Cruz, CA (United States); Santa Cruz Institute for Particle Physics, Santa Cruz, CA (United States)
- Publication Date:
- Research Org.:
- Univ. of California, Santa Cruz, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1979972
- Grant/Contract Number:
- SC0010107; A00-1465-001
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review. D.
- Additional Journal Information:
- Journal Volume: 104; Journal Issue: 12; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; 79 ASTRONOMY AND ASTROPHYSICS; cosmic ray propagation; cosmic ray sources; dark matter; gamma ray astronomy
Citation Formats
Do, Audrey, Duong, Matthew, McDaniel, Alex, O’Connor, Collin, Profumo, Stefano, Rafael, Justine, Sweeney, Connor, and Vera III, Washington. Cosmic-ray transport and gamma-ray emission in M31. United States: N. p., 2021.
Web. doi:10.1103/physrevd.104.123016.
Do, Audrey, Duong, Matthew, McDaniel, Alex, O’Connor, Collin, Profumo, Stefano, Rafael, Justine, Sweeney, Connor, & Vera III, Washington. Cosmic-ray transport and gamma-ray emission in M31. United States. https://doi.org/10.1103/physrevd.104.123016
Do, Audrey, Duong, Matthew, McDaniel, Alex, O’Connor, Collin, Profumo, Stefano, Rafael, Justine, Sweeney, Connor, and Vera III, Washington. Wed .
"Cosmic-ray transport and gamma-ray emission in M31". United States. https://doi.org/10.1103/physrevd.104.123016. https://www.osti.gov/servlets/purl/1979972.
@article{osti_1979972,
title = {Cosmic-ray transport and gamma-ray emission in M31},
author = {Do, Audrey and Duong, Matthew and McDaniel, Alex and O’Connor, Collin and Profumo, Stefano and Rafael, Justine and Sweeney, Connor and Vera III, Washington},
abstractNote = {Here we study the possibility that an extended cosmic-ray leptonic and/or hadronic halo is at the origin of the large-scale gamma-ray emission detected from the Andromeda galaxy (M31). We consider a broad ensemble of nonhomogeneous diffusion scenarios and of cosmic-ray injection sources. We find that cosmic-ray electrons and protons could be, and very likely are, responsible for part, or all, of the gamma-ray emission from M31, including out to more than 100 kpc from the center of the galaxy. We also simulate possible emission from pulsars in M31 and consider the effect of regions of highly inefficient diffusion around cosmic-ray acceleration sites, as suggested by recent TeV halo observations with Cherenkov telescopes.},
doi = {10.1103/physrevd.104.123016},
journal = {Physical Review. D.},
number = 12,
volume = 104,
place = {United States},
year = {Wed Dec 08 00:00:00 EST 2021},
month = {Wed Dec 08 00:00:00 EST 2021}
}
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