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 |