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Compton polarimeter as a focal plane detector for hard X-ray telescope: sensitivity estimation with Geant4 simulations

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dc.contributor.author Chattopadhyay, T. en_US
dc.contributor.author Vadawale, S. V. en_US
dc.contributor.author PENDHARKAR, J. en_US
dc.date.accessioned 2020-10-19T09:00:10Z
dc.date.available 2020-10-19T09:00:10Z
dc.date.issued 2013-04 en_US
dc.identifier.citation Experimental Astronomy, 35(3), 391-412. en_US
dc.identifier.issn 0922-6435 en_US
dc.identifier.issn 1572-9508 en_US
dc.identifier.uri http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5199
dc.identifier.uri https://doi.org/10.1007/s10686-012-9312-3 en_US
dc.description.abstract X-ray polarimetry can be an important tool for investigating various physical processes as well as their geometries at the celestial X-ray sources. However, X-ray polarimetry has not progressed much compared to the spectroscopy, timing and imaging mainly due to the extremely photon-hungry nature of X-ray polarimetry leading to severely limited sensitivity of X-ray polarimeters. The great improvement in sensitivity in spectroscopy and imaging was possible due to focusing X-ray optics which is effective only at the soft X-ray energy range. Similar improvement in sensitivity of polarisation measurement at soft X-ray range is expected in near future with the advent of GEM based photoelectric polarimeters. However, at energies >10 keV, even spectroscopic and imaging sensitivities of X-ray detector are limited due to lack of focusing optics. Thus hard X-ray polarimetry so far has been largely unexplored area. On the other hand, typically the polarisation degree is expected to increase at higher energies as the radiation from non-thermal processes is dominant fraction. So polarisation measurement in hard X-ray can yield significant insights into such processes. With the recent availability of hard X-ray optics (e.g. with upcoming NuSTAR, Astro-H missions) which can focus X-rays from 5 KeV to 80 KeV, sensitivity of X-ray detectors in hard X-ray range is expected to improve significantly. In this context we explore feasibility of a focal plane hard X-ray polarimeter based on Compton scattering having a thin plastic scatterer surrounded by cylindrical array scintillator detectors. We have carried out detailed Geant4 simulation to estimate the modulation factor for 100 % polarized beam as well as polarimetric efficiency of this configuration. We have also validated these results with a semi-analytical approach. Here we present the initial results of polarisation sensitivities of such focal plane Compton polarimeter coupled with the reflection efficiency of present era hard X-ray optics. en_US
dc.language.iso en en_US
dc.publisher Springer Nature en_US
dc.subject Hard X-ray polarimetry en_US
dc.subject X-ray instrumentation en_US
dc.subject Compton polarimetry en_US
dc.subject X-ray detectors en_US
dc.subject 2013 en_US
dc.title Compton polarimeter as a focal plane detector for hard X-ray telescope: sensitivity estimation with Geant4 simulations en_US
dc.type Article en_US
dc.contributor.department Dept. of Physics en_US
dc.identifier.sourcetitle Experimental Astronomy en_US
dc.publication.originofpublisher Foreign en_US


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