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Electron backscattering simulation in Geant4 / Dondero, Paolo (SWHARD S.R.L., Genoa) ; Mantero, Alfonso (SWHARD S.R.L., Genoa) ; Ivanchencko, Vladimir (CERN ; Geant4 Assoc. ; Tomsk State U.) ; Lotti, Simone (INAF, IAPS, Rome) ; Mineo, Teresa (IASF, Palermo) ; Fioretti, Valentina (IASF, Bologna)
The backscattering of electrons is a key phenomenon in several physics applications which range from medical therapy to space including AREMBES, the new ESA simulation framework for radiation background effects. The importance of properly reproducing this complex interaction has grown considerably in the last years and the Geant4 Monte Carlo simulation toolkit, recently upgraded to the version 10.3, is able to comply with the AREMBES requirements in a wide energy range. [...]
2018 - 8 p. - Published in : Nucl. Instrum. Methods Phys. Res., B 425 (2018) 18-25 Fulltext: PDF;

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Validation of Geant4 10.3 simulation of proton interaction for space radiation effects / Ivanchenko, Vladimir (CERN ; Tomsk State U.) ; Dondero, Paolo (SWHARD SRL, Genova) ; Fioretti, Valentina (IASF, Bologna) ; Ivantchenko, Anton (Geant4 Assoc.) ; Lei, Fan (RadMod Reserach, Hampshire) ; Lotti, Simone (INAF, Rome) ; Mantero, Alfonso (SWHARD SRL, Genova) ; Mineo, Teresa (IASF, Palermo)
Monte Carlo simulation of space radiation effects induced by protons is important for design of space missions. Geant4 is a well established toolkit for Monte Carlo simulation focused on high energy physics applications. [...]
2017 - 14 p. - Published in : Exp. Astron. 44 (2017) 437-450

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Geant4 simulations of soft proton scattering in X-ray optics / Fioretti, Valentina (IASF, Bologna) ; Mineo, Teresa (IASF, Palermo) ; Bulgarelli, Andrea (IASF, Bologna) ; Dondero, Paolo (SWHARD srl, Genova) ; Ivanchenko, Vladimir (CERN ; Geant4 Assoc. ; Tomsk State U.) ; Lei, Fan (RadMod Research, Camberley) ; Lotti, Simone (IAS, Rome) ; Macculi, Claudio (IAS, Rome) ; Mantero, Alfonso (SWHARD srl, Genova) /Alfonso Mantero for the AREMBES Collaboration
Low energy protons (< 300 keV) can enter the field of view of X-ray space telescopes, scatter at small incident angles, and deposit energy on the detector, causing intense background flares at the focal plane or in the most extreme cases, damaging the X-ray detector. A correct modelization of the physics process responsible for the grazing angle scattering processes is mandatory to evaluate the impact of such events on the performance of future X-ray telescopes as the ESA ATHENA mission. [...]
arXiv:1707.02221.- 2017-10-28 - 23 p. - Published in : Exp. Astron. 44 (2017) 413-435 Preprint: PDF;

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