2011/09/06 by Nicolas M. Barrière, Barrière, Nicolas M., Lorenzo Natalucci +5
Physics and Astronomy · #Astrophysical Phenomena and Observations #FOS: Physical sciences #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Nuclear Physics and Applications #Particle Detector Development and Performance #astro-ph.IM
paper · pdf · doi:10.48550/arxiv.1109.1313
Published in the proceedings of the conference " The coming of age of X-ray polarimetry" held in Rome on April 27th-30th 2009; 'X-ray Polarimetry, a new window in astrophysics', Cambridge University Press, June 2010, p. 88
arxiv created 2011/09/06 · openalex publication_date 2011/09/06 · arxiv updated 2011/09/08 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Hard X / soft gamma-ray polarimetric analysis can be performed efficiently by the study of Compton scattering anisotropy in a detector composed of fine pixels. But in the energy range above 100 keV where sources flux are extremely weak and instrumental background very strong, such delicate measurement is actually very difficult to perform. Laue lens is an emerging technology based on diffraction in crystals allowing the concentration of soft gamma rays. This kind of optics can be applied to realize an efficient high-sensitivity and high-angular resolution telescope, at the cost of a field of view reduced to a few arcmin though. A 20 m focal length telescope concept focusing in the 100 keV - 600 keV energy range is taken as example here to show that recent progresses in the domain of high-reflectivity crystals can lead to very appealing performance. The Laue lens being fully transparent to polarization, this kind of telescope would be well suited to perform polarimetric studies since the ideal focal plan is a stack of finely pixelated planar detectors - in order to reconstruct the point spread function - which is also ideal to perform Compton tracking of events.