Linear Polarimetry with γ→e+e− Conversions

Linear Polarimetry with γ→e+e− Conversions

γ -rays are emitted by cosmic sources by non-thermal processes that yield either non-polarized photons, such as those from π 0 decay in hadronic interactions, or linearly polarized photons from synchrotron radiation and the inverse-Compton up-shifting of these on high-energy charged partic...

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Bibliographic Details
Main Author: Denis Bernard
Format: Article
Language:English
Published: MDPI AG 2017-11-01
Series:Galaxies
Subjects:
gamma-ray astronomy
gamma-ray polarimetry
pair conversion
time projection chamber
gas detector
optimal methods
Kalman filter
Bayesian method
Online Access:https://www.mdpi.com/2075-4434/5/4/72

Internet

https://www.mdpi.com/2075-4434/5/4/72

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