Lessons from HAWC pulsar wind nebulae observations: The diffusion constant is not a constant; pulsars remain the likeliest sources of the anomalous positron fraction; cosmic rays are trapped for long periods of time in pockets of inefficient diffusion
- Authors:
- Publication Date:
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1454363
- Grant/Contract Number:
- de-sc0010107
- Resource Type:
- Publisher's Accepted Manuscript
- Journal Name:
- Physical Review D
- Additional Journal Information:
- Journal Name: Physical Review D Journal Volume: 97 Journal Issue: 12; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society
- Country of Publication:
- United States
- Language:
- English
Citation Formats
Profumo, Stefano, Reynoso-Cordova, Javier, Kaaz, Nicholas, and Silverman, Maya. Lessons from HAWC pulsar wind nebulae observations: The diffusion constant is not a constant; pulsars remain the likeliest sources of the anomalous positron fraction; cosmic rays are trapped for long periods of time in pockets of inefficient diffusion. United States: N. p., 2018.
Web. doi:10.1103/PhysRevD.97.123008.
Profumo, Stefano, Reynoso-Cordova, Javier, Kaaz, Nicholas, & Silverman, Maya. Lessons from HAWC pulsar wind nebulae observations: The diffusion constant is not a constant; pulsars remain the likeliest sources of the anomalous positron fraction; cosmic rays are trapped for long periods of time in pockets of inefficient diffusion. United States. doi:https://doi.org/10.1103/PhysRevD.97.123008
Profumo, Stefano, Reynoso-Cordova, Javier, Kaaz, Nicholas, and Silverman, Maya. Fri .
"Lessons from HAWC pulsar wind nebulae observations: The diffusion constant is not a constant; pulsars remain the likeliest sources of the anomalous positron fraction; cosmic rays are trapped for long periods of time in pockets of inefficient diffusion". United States. doi:https://doi.org/10.1103/PhysRevD.97.123008.
@article{osti_1454363,
title = {Lessons from HAWC pulsar wind nebulae observations: The diffusion constant is not a constant; pulsars remain the likeliest sources of the anomalous positron fraction; cosmic rays are trapped for long periods of time in pockets of inefficient diffusion},
author = {Profumo, Stefano and Reynoso-Cordova, Javier and Kaaz, Nicholas and Silverman, Maya},
abstractNote = {},
doi = {10.1103/PhysRevD.97.123008},
journal = {Physical Review D},
number = 12,
volume = 97,
place = {United States},
year = {2018},
month = {6}
}
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DOI: https://doi.org/10.1103/PhysRevD.97.123008
DOI: https://doi.org/10.1103/PhysRevD.97.123008
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