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DC Field | Value | Language |
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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 |
Appears in Collections: | JOURNAL ARTICLES |
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