---

CrProtonReentrant.cxx File Reference

#include <math.h>
#include <CLHEP/Random/RandomEngine.h>
#include <CLHEP/Random/RandGeneral.h>
#include <CLHEP/Random/JamesRandom.h>
#include "CrProtonReentrant.h"

Go to the source code of this file.

Functions
G4double	beta (G4double E )
G4double	rigidity (G4double E )
G4double	energy (G4double rigidity )
G4double	reentrantCRspec (G4double E , G4double cor , G4double phi )
G4double	reentrantCRenvelope (G4double E , G4double cor , G4double phi )
G4double	reentrantCRenvelope_integral (G4double E , G4double cor , G4double phi )
G4double	reentrantCRenvelope_integral_inv (G4double value, G4double cor , G4double phi )
G4double	reentrantCRenergy (HepRandomEngine* engine, G4double cor, G4double solarPotential)
Variables
const G4double	lowE_reentrant = 0.1
const G4double	highE_reentrant = 10.0
const G4double	INTEGRAL_reentrant = 26.449
const G4double	A_reentrant = 3.0e-3
	Generate a random distribution of secondary cosmic ray protons: j(E) = A * E**-a * exp(-pow(energy/LOW_CUTOFF,-1)) A = 3.0e-03 a = 2.5 LOW_CUTOFF = 0.16 References: Energy spectrum above is obtained by eye-ball fitting of AMS data (Alcaraz et al. More...
const G4double	a_reentrant = 2.5
G4double	LOW_CUTOFF = 0.16

---

Function Documentation

G4double beta ( G4double E ) [inline]

Definition at line 45 of file CrProtonReentrant.cxx.

G4double energy ( G4double rigidity ) [inline]

Definition at line 55 of file CrProtonReentrant.cxx.

G4double reentrantCRenergy ( HepRandomEngine * engine, G4double cor, G4double solarPotential )

Definition at line 105 of file CrProtonReentrant.cxx. Referenced by CrProtonReentrant::energySrc(), and CrElectronReentrant::energySrc().

G4double reentrantCRenvelope ( G4double E, G4double cor, G4double phi ) [inline]

Definition at line 86 of file CrProtonReentrant.cxx. Referenced by reentrantCRenergy().

G4double reentrantCRenvelope_integral ( G4double E, G4double cor, G4double phi ) [inline]

Definition at line 93 of file CrProtonReentrant.cxx. Referenced by reentrantCRenergy().

G4double reentrantCRenvelope_integral_inv ( G4double value, G4double cor, G4double phi ) [inline]

Definition at line 99 of file CrProtonReentrant.cxx. Referenced by reentrantCRenergy().

G4double reentrantCRspec ( G4double E, G4double cor, G4double phi ) [inline]

Definition at line 81 of file CrProtonReentrant.cxx. Referenced by reentrantCRenergy().

G4double rigidity ( G4double E ) [inline]

Definition at line 50 of file CrProtonReentrant.cxx.

---

Variable Documentation

const G4double A_reentrant = 3.0e-3

Generate a random distribution of secondary cosmic ray protons: j(E) = A * E**-a * exp(-pow(energy/LOW_CUTOFF,-1)) A = 3.0e-03 a = 2.5 LOW_CUTOFF = 0.16 References: Energy spectrum above is obtained by eye-ball fitting of AMS data (Alcaraz et al. 2000, Phys. Letter B 472, 215) Definition at line 73 of file CrProtonReentrant.cxx.

const G4double INTEGRAL_reentrant = 26.449

Definition at line 41 of file CrProtonReentrant.cxx.

G4double LOW_CUTOFF = 0.16

Definition at line 77 of file CrProtonSplash.cxx.

const G4double a_reentrant = 2.5

Definition at line 75 of file CrProtonReentrant.cxx.

const G4double highE_reentrant = 10.0

Definition at line 34 of file CrProtonReentrant.cxx.

const G4double lowE_reentrant = 0.1

Definition at line 33 of file CrProtonReentrant.cxx.

---