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   <dc:title>On the relativistic impulse approximation for the calculation of Compton scattering cross sections and photon interaction coefficients used in kV dosimetry</dc:title>
   <dc:creator>Wang, X.J.</dc:creator>
   <dc:creator>Miguel, Beatriz</dc:creator>
   <dc:creator>Seuntjens, J.</dc:creator>
   <dc:creator>Fernández Varea, José María</dc:creator>
   <dc:subject>Fotons</dc:subject>
   <dc:subject>Dosimetria (Radiació)</dc:subject>
   <dc:subject>Transferència d'energia</dc:subject>
   <dc:subject>Grafit</dc:subject>
   <dc:subject>Photons</dc:subject>
   <dc:subject>Radiation dosimetry</dc:subject>
   <dc:subject>Energy transfer</dc:subject>
   <dc:subject>Graphite</dc:subject>
   <dc:description>&lt;p>We calculate differential and integrated cross sections for the Compton interaction as well as mass&lt;/p>&lt;p>attenuation (μC/ρ), mass energy-transfer (μC&lt;/p>&lt;p>tr/ρ), and mass energy-absorption (μen/ρ)&lt;/p>&lt;p>coefficients, within the relativistic impulse approximation (RIA) using Compton profiles (CPs)&lt;/p>&lt;p>obtained from unrestricted Hartree–Fock electron densities. We investigate the impact of using&lt;/p>&lt;p>molecular as opposed to atomic CPs on dosimetric photon interaction coefficients for air, water&lt;/p>&lt;p>and graphite, and compare our cross sections to the simpler Waller–Hartree (WH) and&lt;/p>&lt;p>Klein–Nishina (KN) formalisms. We find that differences in μC/ρ and μC&lt;/p>&lt;p>tr/ρ resulting from the&lt;/p>&lt;p>choice of CPs within the RIA are small relative to the differences between the RIA, WH, and KN&lt;/p>&lt;p>calculations. Surprisingly, although the WH binding corrections seem accurate when considering&lt;/p>&lt;p>μC/ρ, there are significant discrepancies between the WH and RIA results when we look at μC&lt;/p>&lt;p>tr/ρ.&lt;/p>&lt;p>The WH theory can differ substantially from the predictions of KN and the RIA in the tens of keV&lt;/p>&lt;p>range (e.g. 6%–10% at 20 keV), when Compton scattering becomes the dominant interaction&lt;/p>&lt;p>mechanism. For lower energies, the disagreement further grows to about one order of magnitude&lt;/p>&lt;p>at 1 keV. However, since the photoelectric effect transfers more energy than the Compton&lt;/p>&lt;p>interaction in the tens of keV range and below, the differences in the total μen/ρ values resulting&lt;/p>&lt;p>from the choice of Compton models (KN, WH, or RIA) are not larger than 0.4%, and the&lt;/p>&lt;p>differences between WH and the other two theories are no longer prominent.&lt;/p></dc:description>
   <dc:date>2026-01-29T13:14:29Z</dc:date>
   <dc:date>2026-01-29T13:14:29Z</dc:date>
   <dc:date>2020-01-01</dc:date>
   <dc:date>2026-01-29T13:14:29Z</dc:date>
   <dc:type>info:eu-repo/semantics/article</dc:type>
   <dc:type>info:eu-repo/semantics/acceptedVersion</dc:type>
   <dc:identifier>0031-9155</dc:identifier>
   <dc:identifier>https://hdl.handle.net/2445/226403</dc:identifier>
   <dc:identifier>712759</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:relation>Versió postprint del document publicat a: https://doi.org/10.1088/1361-6560/ab8108</dc:relation>
   <dc:relation>Physics in Medicine and Biology, 2020, vol. 65, p. 125010-1-125010-16</dc:relation>
   <dc:relation>https://doi.org/10.1088/1361-6560/ab8108</dc:relation>
   <dc:rights>(c) ART AMB B, 2020</dc:rights>
   <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
   <dc:format>16 p.</dc:format>
   <dc:format>application/pdf</dc:format>
   <dc:publisher>ART AMB B</dc:publisher>
   <dc:source>Articles publicats en revistes (Física Quàntica i Astrofísica)</dc:source>
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