Abstract
The scattering of soft protons inside the Wolter-type optics of X-ray observatories has been proven to concentrate these particles onto the focal plane instruments. The funneling of these protons increases the instrumental background and can also contribute to the degrading of the detectors. The instrumental background and degradation of the detector’s performance experienced by Chandra and XMM-Newton is significantly larger than what was expected on the basis of previous Monte Carlo simulations. For Chandra the main issue is the degradation of the energy resolution due to lattice displacements in the detectors. For XMM the contribution to the instrumental background is more significant. In between, new laboratory measurements as well as a revision of the theory are needed to correctly assess the impact of the environmental radiation for future missions. In this publication we present a Geant4 class that will allow future users to select between either theoretical models or measured data to simulate the scattering of soft protons at grazing angles. To develop this method, we revisit the theory of elastic scattering of protons on polished surfaces and implement these approaches into Geant4. We also implemented recently performed measurements using parts of eROSITA (extended ROentgen Survey with an Imaging Telescope Array) mirror shells as scattering targets as another scattering model to be used within the Geant4 toolkit.
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Acknowledgements
The AHEAD project (grant agreement n. 654215) which is part of the EU-H2020 programm is acknowledged for partial support.
The research leading to these results has received funding from the European Union’s Horizon 2020 Programme under the AHEAD project (grant agreement n. 654215). This work was partially supported by the Bundesministerium für Wirtschaft und Energie through the Deutsche Zentrum für Luft- und Raumfahrt e.V. (DLR) under the grant 50QR0702.
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Guzmán, A., Perinati, E., Diebold, S. et al. A revision of soft proton scattering at grazing incidence and its implementation in the geant4 toolkit. Exp Astron 44, 401–411 (2017). https://doi.org/10.1007/s10686-017-9537-2
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DOI: https://doi.org/10.1007/s10686-017-9537-2