Neutrinos from Cosmic Accelerators including Magnetic Field and Flavor Effects
Author
Source
Advances in High Energy Physics
Issue
Vol. 2012, Issue 2012 (31 Dec. 2012), pp.1-41, 41 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2012-06-13
Country of Publication
Egypt
No. of Pages
41
Main Subjects
Abstract EN
We review the particle physics ingredients affecting the normalization, shape, and flavor composition of astrophysical neutrinos fluxes, such as different production modes, magnetic field effects on the secondaries (muons, pions, and kaons), and flavor mixing, where we focus on pγ interactions.
We also discuss the interplay with neutrino propagation and detection, including the possibility to detect flavor and its application in particle physics, and the use of the Glashow resonance to discriminate pγ from pp interactions in the source.
We illustrate the implications on fluxes and flavor composition with two different models: (1) the target photon spectrum is dominated by synchrotron emission of coaccelerated electrons and (2) the target photon spectrum follows the observed photon spectrum of gamma-ray bursts.
In the latter case, the multimessenger extrapolation from the gamma-ray fluence to the expected neutrino flux is highlighted.
American Psychological Association (APA)
Winter, Walter. 2012. Neutrinos from Cosmic Accelerators including Magnetic Field and Flavor Effects. Advances in High Energy Physics،Vol. 2012, no. 2012, pp.1-41.
https://search.emarefa.net/detail/BIM-482943
Modern Language Association (MLA)
Winter, Walter. Neutrinos from Cosmic Accelerators including Magnetic Field and Flavor Effects. Advances in High Energy Physics No. 2012 (2012), pp.1-41.
https://search.emarefa.net/detail/BIM-482943
American Medical Association (AMA)
Winter, Walter. Neutrinos from Cosmic Accelerators including Magnetic Field and Flavor Effects. Advances in High Energy Physics. 2012. Vol. 2012, no. 2012, pp.1-41.
https://search.emarefa.net/detail/BIM-482943
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-482943