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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

Abstract

Not provided.

Authors:
; ; ;
Publication Date:
Research Org.:
Univ. of California, Santa Cruz, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1541174
DOE Contract Number:  
SC0010107
Resource Type:
Journal Article
Journal Name:
Physical Review D
Additional Journal Information:
Journal Volume: 97; Journal Issue: 12; Journal ID: ISSN 2470-0010
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
Astronomy & Astrophysics; Physics

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: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:10.1103/physrevd.97.123008.
@article{osti_1541174,
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 = {Not provided.},
doi = {10.1103/physrevd.97.123008},
journal = {Physical Review D},
issn = {2470-0010},
number = 12,
volume = 97,
place = {United States},
year = {2018},
month = {6}
}

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