Open Access
30 March 2018 High-energy photon polarimeter for astrophysics
Maxim Eingorn, Lakma Fernando, Branislav Vlahovic, Cosmin Ilie, Bogdan Wojtsekhowski, Guido Maria Urciuoli, Fulvio De Persio, Franco Meddi, Vladimir Nelyubin
Author Affiliations +
Abstract
A high-energy photon polarimeter for astrophysics studies in the energy range from 10 to 800 MeV is considered. The proposed concept uses a stack of silicon microstrip detectors, where they play the roles of both a converter and a tracker. The purpose of this paper is to outline the parameters of such a polarimeter and to estimate the productivity of measurements. Our study, supported by a Monte Carlo simulation, shows that with a 1-year observation period the polarimeter will provide 6% accuracy of the polarization degree for photon energies above 100 MeV, which would be a significant advance relative to the currently explored energy range of a few MeV. The proposed polarimeter design could easily be adjusted to the specific photon energy range to maximize efficiency if needed.
CC BY: © The Authors. Published by SPIE under a Creative Commons Attribution 4.0 Unported License. Distribution or reproduction of this work in whole or in part requires full attribution of the original publication, including its DOI.
Maxim Eingorn, Lakma Fernando, Branislav Vlahovic, Cosmin Ilie, Bogdan Wojtsekhowski, Guido Maria Urciuoli, Fulvio De Persio, Franco Meddi, and Vladimir Nelyubin "High-energy photon polarimeter for astrophysics," Journal of Astronomical Telescopes, Instruments, and Systems 4(1), 011006 (30 March 2018). https://doi.org/10.1117/1.JATIS.4.1.011006
Received: 28 November 2017; Accepted: 9 March 2018; Published: 30 March 2018
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CITATIONS
Cited by 9 scholarly publications.
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KEYWORDS
Polarimetry

Polarization

Photon polarization

Sensors

Astrophysics

Pulsars

Silicon

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