Page MenuHomec4science
Files F76652754

main.cpp
No OneTemporary
Actions

File Metadata

Created
Fri, Aug 9, 15:06

main.cpp
View Options

/**
* @file main.cpp
* @Author Christoph Schaaefer, EPFL (christophernstrerne.schaefer@epfl.ch)
* @date October 2016
* @brief Benchmark for gradhalo function
*/
#include <iostream>
#include <string.h>
#include <cuda_runtime.h>
#include "structure.h"
#include <math.h>
#include <sys/time.h>
#include <fstream>
/** for both gradient and second derivatives **/
static struct point rotateCoordinateSystem(struct point P, double theta);
/** gradient **/
struct point module_potentialDerivatives_totalGradient(const runmode_param *runmode, const struct point *pImage, const struct Potential *lens);
static struct point grad_halo(const struct point *pImage, const struct Potential *lens);
/** PIEMD **/
static complex piemd_1derivatives_ci05(double x, double y, double eps, double rc);
/** Potential **/
void module_readParameters_calculatePotentialparameter(Potential *lens);
int main()
{
//Constant
int small(10);
int medium(100);
int big(1000);
//Variable creation
struct timeval t1, t2, t3, t4;
runmode_param runmodesmall;
runmode_param runmodemedium;
runmode_param runmodebig;
point image;
Potential *ilens;
Potential lens[big];
//Initialisation
runmodesmall.nhalos = small;
runmodemedium.nhalos = medium;
runmodebig.nhalos = big;
image.x = image.y = 2;
for (int i = 0; i <big; ++i){
ilens = &lens[i];
ilens->position.x = ilens->position.y = 0.;
ilens->type = 8;
ilens->ellipticity = 0.11;
ilens->ellipticity_potential = 0.;
ilens->ellipticity_angle = 0.;
ilens->rcut = 5.;
ilens->rcore = 1;
ilens->weight = 0;
ilens->rscale = 0;
ilens->exponent = 0;
ilens->alpha = 0.;
ilens->einasto_kappacritic = 0;
ilens->z = 0.4;
module_readParameters_calculatePotentialparameter(ilens);
}
gettimeofday(&t1, 0);
module_potentialDerivatives_totalGradient(&runmodesmall,&image, lens);
gettimeofday(&t2, 0);
module_potentialDerivatives_totalGradient(&runmodemedium,&image, lens);
gettimeofday(&t3, 0);
module_potentialDerivatives_totalGradient(&runmodebig,&image, lens);
gettimeofday(&t4, 0);
double time1 = (1000000.0*(t2.tv_sec-t1.tv_sec) + t2.tv_usec-t1.tv_usec)/1000000.0;
double time2 = (1000000.0*(t3.tv_sec-t2.tv_sec) + t3.tv_usec-t2.tv_usec)/1000000.0;
double time3 = (1000000.0*(t4.tv_sec-t3.tv_sec) + t4.tv_usec-t3.tv_usec)/1000000.0;
std::cout << "Benchmark for Gradient Calculation "<< std::endl;
std::cout << "Sample size " << small << ": " << time1 << std::endl;
std::cout << "Sample size " << medium << ": " << time2 << std::endl;
std::cout << "Sample size " << big << ": " << time3 << std::endl;
std::ofstream myfile;
myfile.open ("BenchmarkGrad.txt");
myfile << "Benchmark for Gradient Calculation "<< std::endl;
myfile << "Sample size " << small << ": " << time1 << std::endl;
myfile << "Sample size " << medium << ": " << time2 << std::endl;
myfile << "Sample size " << big << ": " << time3 << std::endl;
myfile.close();
}
struct point module_potentialDerivatives_totalGradient(const runmode_param *runmode, const struct point *pImage, const struct Potential *lens)
{
struct point grad, clumpgrad;
grad.x=0;
grad.y=0;
for(int i=0; i<runmode->nhalos; i++){
clumpgrad=grad_halo(pImage,&lens[i]); //compute gradient for each clump separately
if(clumpgrad.x == clumpgrad.x or clumpgrad.y == clumpgrad.y){ //nan check
grad.x+=clumpgrad.x;
grad.y+=clumpgrad.y;
} // add the gradients
}
return(grad);
}
/**@brief Return the gradient of the projected lens potential for one clump
* !!! You have to multiply by dlsds to obtain the true gradient
* for the expressions, see the papers : JP Kneib & P Natarajan, Cluster Lenses, The Astronomy and Astrophysics Review (2011) for 1 and 2
* and JP Kneib PhD (1993) for 3
*
* @param pImage point where the result is computed in the lens plane
* @param lens mass distribution
*/
static struct point grad_halo(const struct point *pImage, const struct Potential *lens)
{
struct point true_coord, true_coord_rotation, result;
double R, angular_deviation;
complex zis;
result.x = result.y = 0.;
/*positionning at the potential center*/
true_coord.x = pImage->x - lens->position.x; // Change the origin of the coordinate system to the center of the clump
true_coord.y = pImage->y - lens->position.y;
switch (lens->type)
{
case(5): /*Elliptical Isothermal Sphere*/
/*rotation of the coordiante axes to match the potential axes*/
true_coord_rotation = rotateCoordinateSystem(true_coord, lens->ellipticity_angle);
R=sqrt(true_coord_rotation.x*true_coord_rotation.x*(1-lens->ellipticity/3.)+true_coord_rotation.y*true_coord_rotation.y*(1+lens->ellipticity/3.)); //ellippot = ellipmass/3
result.x=(1-lens->ellipticity/3.)*lens->b0*true_coord_rotation.x/(R);
result.y=(1+lens->ellipticity/3.)*lens->b0*true_coord_rotation.y/(R);
break;
case(8): /* PIEMD */
/*rotation of the coordiante axes to match the potential axes*/
true_coord_rotation = rotateCoordinateSystem(true_coord, lens->ellipticity_angle);
/*Doing something....*/
zis = piemd_1derivatives_ci05(true_coord_rotation.x, true_coord_rotation.y, lens->ellipticity_potential, lens->rcore);
result.x=lens->b0 * zis.re;
result.y=lens->b0 * zis.im;
break;
default:
std::cout << "ERROR: Grad 1 profil type of clump "<< lens->name << " unknown : "<< lens->type << std::endl;
break;
};
return result;
}
/**** usefull functions for PIEMD profile : see old lenstool ****/
/** I*w,v=0.5 Kassiola & Kovner, 1993 PIEMD, paragraph 4.1
*
* Global variables used :
* - none
*/
static complex piemd_1derivatives_ci05(double x, double y, double eps, double rc)
{
double sqe, cx1, cxro, cyro, rem2;
complex zci, znum, zden, zis, zres;
double norm;
sqe = sqrt(eps);
cx1 = (1. - eps) / (1. + eps);
cxro = (1. + eps) * (1. + eps);
cyro = (1. - eps) * (1. - eps);
rem2 = x * x / cxro + y * y / cyro;
/*zci=cpx(0.,-0.5*(1.-eps*eps)/sqe);
znum=cpx(cx1*x,(2.*sqe*sqrt(rc*rc+rem2)-y/cx1));
zden=cpx(x,(2.*rc*sqe-y));
zis=pcpx(zci,lncpx(dcpx(znum,zden)));
zres=pcpxflt(zis,b0);*/
// --> optimized code
zci.re = 0;
zci.im = -0.5 * (1. - eps * eps) / sqe;
znum.re = cx1 * x;
znum.im = 2.*sqe * sqrt(rc * rc + rem2) - y / cx1;
zden.re = x;
zden.im = 2.*rc * sqe - y;
norm = zden.re * zden.re + zden.im * zden.im; // zis = znum/zden
zis.re = (znum.re * zden.re + znum.im * zden.im) / norm;
zis.im = (znum.im * zden.re - znum.re * zden.im) / norm;
norm = zis.re;
zis.re = log(sqrt(norm * norm + zis.im * zis.im)); // ln(zis) = ln(|zis|)+i.Arg(zis)
zis.im = atan2(zis.im, norm);
// norm = zis.re;
zres.re = zci.re * zis.re - zci.im * zis.im; // Re( zci*ln(zis) )
zres.im = zci.im * zis.re + zis.im * zci.re; // Im( zci*ln(zis) )
//zres.re = zis.re*b0;
//zres.im = zis.im*b0;
return(zres);
}
/// Useful functions
// changes the coordinates of point P into a new basis (rotation of angle theta)
// y' y x'
// * | /
// * | / theta
// * | /
// *|--------->x
static struct point rotateCoordinateSystem(struct point P, double theta)
{
struct point Q;
Q.x = P.x*cos(theta) + P.y*sin(theta);
Q.y = P.y*cos(theta) - P.x*sin(theta);
return(Q);
}
/** @brief This module function calculates profile depended information like the impactparameter b0 and the potential ellipticity epot
*
* @param lens: mass distribution for which to calculate parameters
*/
void module_readParameters_calculatePotentialparameter(Potential *lens){
switch (lens->type)
{
case(5): /*Elliptical Isothermal Sphere*/
//impact parameter b0
lens->b0 = 4* pi_c2 * lens->vdisp * lens->vdisp ;
//ellipticity_potential
lens->ellipticity_potential = lens->ellipticity/3 ;
break;
case(8): /* PIEMD */
//impact parameter b0
lens->b0 = 6.*pi_c2 * lens->vdisp * lens->vdisp;
//ellipticity_parameter
if ( lens->ellipticity == 0. && lens->ellipticity_potential != 0. ){
// emass is (a2-b2)/(a2+b2)
lens->ellipticity = 2.*lens->ellipticity_potential / (1. + lens->ellipticity_potential * lens->ellipticity_potential);
//printf("1 : %f %f \n",lens->ellipticity,lens->ellipticity_potential);
}
else if ( lens->ellipticity == 0. && lens->ellipticity_potential == 0. ){
lens->ellipticity_potential = 0.00001;
//printf("2 : %f %f \n",lens->ellipticity,lens->ellipticity_potential);
}
else{
// epot is (a-b)/(a+b)
lens->ellipticity_potential = (1. - sqrt(1 - lens->ellipticity * lens->ellipticity)) / lens->ellipticity;
//printf("3 : %f %f \n",lens->ellipticity,lens->ellipticity_potential);
}
break;
default:
std::cout << "ERROR: LENSPARA profil type of clump "<< lens->name << " unknown : "<< lens->type << std::endl;
//printf( "ERROR: LENSPARA profil type of clump %s unknown : %d\n",lens->name, lens->type);
break;
};
}

Event Timeline

c4science · Help