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File indexing completed on 2026-09-08 09:05:35
0001 //------------------------------ -*- C++ -*- -------------------------------// 0002 // Copyright Celeritas contributors: see top-level COPYRIGHT file for details 0003 // SPDX-License-Identifier: (Apache-2.0 OR MIT) 0004 //---------------------------------------------------------------------------// 0005 //! \file celeritas/em/interactor/detail/PhysicsConstants.hh 0006 //---------------------------------------------------------------------------// 0007 #pragma once 0008 0009 #include "corecel/Macros.hh" 0010 #include "corecel/Types.hh" 0011 #include "corecel/math/Algorithms.hh" 0012 #include "corecel/math/Constant.hh" 0013 #include "corecel/math/UnitUtils.hh" 0014 #include "celeritas/Constants.hh" 0015 #include "celeritas/UnitTypes.hh" 0016 0017 namespace celeritas 0018 { 0019 namespace detail 0020 { 0021 //---------------------------------------------------------------------------// 0022 //! Special partly-natural unit [MeV / len] 0023 using MevPerLen = RealQuantity<UnitDivide<units::Mev, units::Native>>; 0024 0025 //! Migdal's constant used for Bremsstrahlung [len^3] 0026 CELER_CONSTEXPR_FUNCTION Constant migdal_constant() 0027 { 0028 using namespace constants; 0029 0030 return 4 * pi * r_electron * ipow<2>(lambdabar_electron); 0031 } 0032 0033 //---------------------------------------------------------------------------// 0034 /*! 0035 * Landau-Pomeranchuk-Migdal constant [MeV / len]. 0036 * 0037 * This is used to calculate the LPM characteristic energy, defined as 0038 * \f$ E_\textrm{LPM} = \frac{\alpha m^2 X_0}{2 h c} \f$, where 0039 * \f$ X_0 \f$ is the radiation length of the material. Note that some papers 0040 * define \f$ E_\textrm{LPM} \f$ as a factor of two smaller and others as a 0041 * factor of 8 larger: see \cite{klein-lpm-1999}. 0042 * The Geant4 Physics Reference Manual (Eq. 10.17) \cite{g4prm} has 0043 * an extra factor of two in the denominator. 0044 */ 0045 CELER_CONSTEXPR_FUNCTION MevPerLen lpm_constant() 0046 { 0047 using namespace constants; 0048 0049 constexpr auto electron_mass_csq = electron_mass * ipow<2>(c_light); 0050 0051 return native_value_to<MevPerLen>(alpha_fine_structure 0052 * ipow<2>(electron_mass_csq) 0053 / (2 * h_planck * c_light)); 0054 } 0055 0056 //---------------------------------------------------------------------------// 0057 // Constant functions for model limits 0058 //---------------------------------------------------------------------------// 0059 0060 //! Maximum energy for EM models to be valid 0061 CELER_CONSTEXPR_FUNCTION units::MevEnergy high_energy_limit() 0062 { 0063 return units::MevEnergy{1e8}; //! 100 TeV 0064 } 0065 0066 //---------------------------------------------------------------------------// 0067 } // namespace detail 0068 } // namespace celeritas
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