Physics – Optics
Scientific paper
Jul 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010spie.7732e.151i&link_type=abstract
Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray. Edited by Arnaud, Monique; Murray, Stephen S.; Takahashi,
Physics
Optics
Scientific paper
We report a development of a bent crystal for use of X-ray polarimeter. A Si(100) crystal sheet was deposited with DLC (Diamond-Like Carbon) and bent by the difference in the internal stress between the DLC and Si. An angular reflectivity of the crystal was measured at 8 keV (Cu-Kα). The center of the reflection peak appeared at the Bragg angle expected for the (400) plane of Si(100). With the bending of the crystal, the angular width of the peak is broadened. A sample indicated the angular width of 2 degree, which is equivalent to the energy width of 0.5 keV. The modulation factor was measured to be more than 0.9 for 8 keV energy emission. If the energy of the X-ray emission is at Fe-K lines (~7 keV), which are very important for X-ray astronomy, the Bragg angle becomes more close to 45 degree. It means that higher sensitivity for the polarization would be expected for these lines. The sensitivity in wide energy band with the high modulation factor indicates that the bent crystal can be a new tool for the X-ray polarimeter. A preliminary design of the polarimetric optics composed by the Si(100) crystal and a small-size detector (e.g. X-ray CCD camera) is proposed. For celestial objects with large spatial extent with large emitting energy band, our optics could collect X-rays much more efficiently than existing optics with high signal to noise ratio. Any kind of crystals can be bent with our method, and then a combination of different crystals will further improve the performance of the polarimetric optics.
Akasaka Hiroki
Iizuka Ryo
Kusunoki Shingo
Misumi Kazuyoshi
Ohtake Naoto
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