Class in charge of generating electrons from Electron-electron_Neutrino Elastic Scattering (ENES) nu_e+e -> nu_e+e of supernova antineutrino interactions.
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Supported by OMSimSNTools, this class generates the corresponding electrons after the ENES and weights the interactions corresponding to the cross section and the generated volume
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| OMSimENES (G4ParticleGun *) |
| Constructor of OMSimENES class.
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Public Member Functions inherited from SNBaseParticleGenerator |
| SNBaseParticleGenerator (G4ParticleGun *) |
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void | GeneratePrimaries (G4Event *anEvent) |
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Protected Member Functions inherited from SNBaseParticleGenerator |
void | initialiseDistribution (int column, int targets) |
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G4double | calculateNeutrinoEnergy () |
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G4ThreeVector | calculateMomentumDirection (G4double pNeutrinoEnergy) |
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G4double | calculateWeight (G4double pNuEnergy) |
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Protected Attributes inherited from SNBaseParticleGenerator |
G4ParticleGun * | m_particleGun |
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OMSimSNTools | m_SNToolBox |
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const G4double | m_Gf = 1.166e-5 * 1e-6 / (MeV * MeV) |
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const G4double | m_Consg = 1.26 |
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const G4double | m_deltaMass = neutron_mass_c2 - proton_mass_c2 |
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const G4double | m_massSquaredDifference = (pow(m_deltaMass, 2) - pow(electron_mass_c2, 2)) / 2. |
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G4double | m_NrTargets |
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DistributionSampler | m_timeDistribution |
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DistributionSampler | m_meanEnergyDistribution |
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DistributionSampler | m_meanEnergySquaredDistribution |
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◆ OMSimENES()
OMSimENES::OMSimENES |
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G4ParticleGun * |
p_gun | ) |
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- Parameters
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p_gun | Pointer to the particle p_gun object used for simulation. |
◆ angularDistribution()
This function calculates the angular distribution for electrons scattered by neutrinos. The foundation for this computation is taken from the reference: "Carlo Giunti and Chung W.Kim (2007), Fundamentals of Neutrino Physics and Astrophysics, Oxford University Press, Chapter 5, eq. 5.29".
- Parameters
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p_energy | The energy of the incident neutrino. |
Implements SNBaseParticleGenerator.
◆ calculateSecondaryParticleEnergy()
G4double OMSimENES::calculateSecondaryParticleEnergy |
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G4double |
p_NuEnergy, |
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G4double |
p_cosTheta |
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privatevirtual |
The computation utilizes the formula for the energy of the electron as a function of incident neutrino energy and the scatter angle, based on the formula provided in the reference: "Carlo Giunti and Chung W.Kim (2007), Fundamentals of Neutrino Physics and Astrophysics, Oxford University Press, Chapter 5, eq. 5.27".
- Parameters
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p_NuEnergy | The energy of the incident neutrino. |
p_cosTheta | The cosine of the scattering angle. |
- Returns
- Calculated energy value of the electron post scattering.
Implements SNBaseParticleGenerator.
◆ initialiseParticle()
void OMSimENES::initialiseParticle |
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privatevirtual |
◆ totalCrossSection()
G4double OMSimENES::totalCrossSection |
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G4double |
p_energy | ) |
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privatevirtual |
This function determines the total cross-section for the scattering of neutrinos with electrons given a specific incident neutrino energy. The computational foundation is derived from: "M. Buchkremer, Electroweak Interactions: Neutral currents in neutrino-lepton elastic scattering experiments,
Université Catholique de Louvain /CP3, 2011."
- Parameters
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p_energy | The energy of the incident neutrino. |
- Returns
- Calculated total cross-section value for the given energy.
Implements SNBaseParticleGenerator.
The documentation for this class was generated from the following files: