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/**
Lenstool-HPC: HPC based massmodeling software and Lens-map generation
Copyright (C) 2017 Christoph Schaefer, EPFL (christophernstrerne.schaefer@epfl.ch), Gilles Fourestey (gilles.fourestey@epfl.ch)
This program is free software: you can redistribute it and/or modify
it under the terms of the GNU General Public License as published by
the Free Software Foundation, either version 3 of the License, or
(at your option) any later version.
This program is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
GNU General Public License for more details.
You should have received a copy of the GNU General Public License
along with this program. If not, see <http://www.gnu.org/licenses/>.
@brief: Function for second order computation on CPU to compare with GPUs
*/
#include <iostream>
#include <iomanip>
#include <string.h>
//#include <cuda_runtime.h>
#include <math.h>
#include <sys/time.h>
#include <fstream>
#include <immintrin.h>
#include <map>
/*
#ifdef __AVX__
#include "simd_math_avx.h"
#endif
#ifdef __AVX512F__
#include "simd_math_avx512f.h"
#endif
*/
#include "structure_hpc.hpp"
#include "gradient2.hpp"
//lenstool fct
/*
* derivates of I0.5 KK
* Parameters :
* - (x,y) is the computation position of the potential
* - eps is the ellepticity (a-b)/(a+b)
* - rc is the core radius
* - b0 asymptotic Einstein radius E0. (6pi*vdisp^2/c^2)
*
* Return a the 4 second derivatives of the PIEMD potential
*/
inline
void mdci05_hpc(type_t x, type_t y, type_t eps, type_t rc, type_t b0, struct matrix *res)
{
type_t ci, sqe, cx1, cxro, cyro, wrem;
type_t didyre, didyim, didxre; // didxim;
type_t cx1inv, den1, num2, den2;
//
sqe = sqrt(eps);
cx1 = (1. - eps)/(1. + eps);
cx1inv = 1./cx1;
//
cxro = (1. + eps)*(1. + eps); /* rem^2=x^2/(1+e^2) + y^2/(1-e^2) Eq 2.3.6*/
cyro = (1. - eps)*(1. - eps);
ci = 0.5*(1. - eps * eps) / sqe;
wrem = sqrt(rc*rc + x*x/cxro + y*y/cyro); /*wrem^2=w^2+rem^2 with w core radius*/
den1 = 2.*sqe*wrem - y*cx1inv;
den1 = cx1*cx1*x*x + den1*den1;
num2 = 2.*rc*sqe - y;
den2 = x*x + num2*num2;
//
didxre = ci*( cx1*(2.*sqe*x*x/cxro/wrem - 2.*sqe*wrem + y*cx1inv)/den1 + num2/den2 );
didyre = ci*( (2.*sqe*x*y*cx1/cyro/wrem - x)/den1 + x/den2 );
didyim = ci * ( (2.* sqe * wrem * cx1inv - y * cx1inv * cx1inv - 4.*eps*y/cyro +
2.* sqe * y * y / cyro / wrem * cx1inv)/den1 - num2/den2 );
//
res->a = b0 * didxre;
res->b = res->d = b0 * didyre; //(didyre+didxim)/2.;
res->c = b0 * didyim;
// return(res);
}
//
void printmat(matrix A){
std::cerr << A.a << " " << A.b << " " << A.c << " " << A.d << std::endl;
}
//
// SOA versions, vectorizable
//
//
struct matrix module_potentialDerivatives_totalGradient2_81_SOA_v2(const struct point *pImage, const struct Potential_SOA *lens, int shalos, int nhalos)
{
asm volatile("# module_potentialDerivatives_totalGradient2_81_SOA begins");
//std::cout << "# module_potentialDerivatives_totalGradient_81_SOA begins" << std::endl;
// 6 DP loads, i.e. 48 Bytes: position_x, position_y, ellipticity_angle, ellipticity_potential, rcore, b0
//
type_t t05;
type_t RR;
//
struct matrix grad2, clump, clumpcore, clumpcut;
struct point true_coord, true_coord_rotation;
//
grad2.a = clump.a = 0;
grad2.b = clump.b = 0;
grad2.c = clump.c = 0;
grad2.d = clump.d = 0;
//
for(int i = shalos; i < shalos + nhalos; i++)
{
//if (lens->ellipticity_potential[i] < 0.0001) printf("halo = %d, ellipticity_potential = %f\n", i, lens->ellipticity_potential[i]);
//if(lens->ellipticity_potential[i] > 0.0001)
if (true)
{
//True coord
true_coord.x = pImage->x - lens->position_x[i];
true_coord.y = pImage->y - lens->position_y[i];
//
//std::cerr << "start" << std::endl;
//Rotation
type_t cose = lens->anglecos[i];
type_t sine = lens->anglesin[i];
//
type_t x = true_coord.x*cose + true_coord.y*sine;
type_t y = true_coord.y*cose - true_coord.x*sine;
// 81 comput
t05 = lens->rcut[i] / (lens->rcut[i] - lens->rcore[i]);
mdci05_hpc(x, y, lens->ellipticity_potential[i], lens->rcore[i], lens->b0[i], &clumpcore);
mdci05_hpc(x, y, lens->ellipticity_potential[i], lens->rcut[i], lens->b0[i], &clumpcut);
//printf("X %f Y %f Ga: %f %f\n",true_coord.x ,true_coord.y , clumpcore.a, clumpcut.a);
//printf("X %f Y %f Gb: %f %f\n",true_coord.x ,true_coord.y, clumpcore.b, clumpcut.b);
//printf("X %f Y %f Gc: %f %f\n", true_coord.x ,true_coord.y,clumpcore.c, clumpcut.c);
//printf("X %f Y %f Gd: %f %f\n",true_coord.x ,true_coord.y, clumpcore.d, clumpcut.d);
//
clumpcore.a = t05 * (clumpcore.a - clumpcut.a);
clumpcore.b = t05 * (clumpcore.b - clumpcut.b);
clumpcore.c = t05 * (clumpcore.c - clumpcut.c);
clumpcore.d = t05 * (clumpcore.d - clumpcut.d);
//printmat(clumpcore);
//printf("X %f Y %f Ga: %f %f\n",pImage->x ,pImage->y , clumpcore.a, t05);
//printf("X %f Y %f Gb: %f %f\n",pImage->x ,pImage->y, clumpcore.b, clumpcut.b);
//printf("X %f Y %f Gc: %f %f\n",pImage->x ,pImage->y, clumpcore.c, clumpcut.c);
//printf("X %f Y %f Gd: %f %f\n",pImage->x ,pImage->y, clumpcore.d, clumpcut.d);
//rotation matrix 1
clumpcut.a = clumpcore.a * cose + clumpcore.b * -sine;
clumpcut.b = clumpcore.a * sine + clumpcore.b * cose;
clumpcut.c = clumpcore.d * sine + clumpcore.c * cose;
clumpcut.d = clumpcore.d * cose + clumpcore.c * -sine;
//printf("X %f Y %f theta: %f %f %f\n",pImage->x ,pImage->y,lens->ellipticity_angle[i], cose, sine);
//printmat(clumpcut);
//rotation matrix 2
clump.a = cose*clumpcut.a - sine*clumpcut.d;
clump.b = cose*clumpcut.b - sine*clumpcut.c;
clump.c = sine*clumpcut.b + cose*clumpcut.c;
clump.d = sine*clumpcut.a + cose*clumpcut.d;
//
//printf("X %f Y %f Ga: %f \n",pImage->x ,pImage->y , clump.a );
//printf("X %f Y %f Gb: %f \n",pImage->x ,pImage->y, clump.b );
//printf("X %f Y %f Gc: %f \n",pImage->x ,pImage->y, clump.c);
//printf("X %f Y %f Gd: %f \n",pImage->x ,pImage->y, clump.d );
//printmat(clump);
//
grad2.a += clump.a;
grad2.b += clump.b;
grad2.c += clump.c;
grad2.d += clump.d;
}
else if((RR = true_coord.x * true_coord.x + true_coord.y * true_coord.y) > 0.)
{
// Circular dPIE Elliasdottir 2007 Eq A23 slighly modified for t05
type_t X,Y,z,p,t05;
X = lens->rcore[i];
Y = lens->rcut[i];
t05 = lens->b0[i] * Y / (Y - X); // 1/u because t05/sqrt(u) and normalised Q/sqrt(u)
z = sqrt(RR + X * X) - X - sqrt(RR + Y * Y) + Y; // R*dphi/dR
X = RR / X;
Y = RR / Y;
p = (1. - 1. / sqrt(1. + X / lens->rcore[i])) / X - (1. - 1. / sqrt(1. + Y / lens->rcut[i])) / Y; // d2phi/dR2
X = true_coord.x * true_coord.x / RR;
Y = true_coord.y * true_coord.y / RR;
clump.a = t05 * (p * X + z * Y / RR);
clump.c = t05 * (p * Y + z * X / RR);
X = true_coord.x * true_coord.y / RR;
clump.b = clump.d = t05 * (p * X - z * X / RR);
grad2.a += clump.a;
grad2.b += clump.b;
grad2.c += clump.c;
grad2.d += clump.d;
}
else
{
clump.a = clump.c = lens->b0[i] / lens->rcore[i]/ 2.;
clump.b = clump.d = 0.;
grad2.a += clump.a;
grad2.b += clump.b;
grad2.c += clump.c;
grad2.d += clump.d;
}
}
//
return(grad2);
}
//
//This natrix handles the calling of the gradient functions for the different type without losing time to switch or if condition
//
typedef struct matrix (*halo_g2_func_t) (const struct point *pImage, const struct Potential_SOA *lens, int shalos, int nhalos);
halo_g2_func_t halo_g2_func[100] =
{
0, 0, 0, 0, 0, 0, 0, 0, 0, 0,
0, 0, 0, 0, 0, 0, 0, 0, 0, 0,
0, 0, 0, 0, 0, 0, 0, 0, 0, 0,
0, 0, 0, 0, 0, 0, 0, 0, 0, 0,
0, 0, 0, 0, 0, 0, 0, 0, 0, 0,
0, 0, 0, 0, 0, 0, 0, 0, 0, 0,
0, 0, 0, 0, 0, 0, 0, 0, 0, 0,
0, 0, 0, 0, 0, 0, 0, 0, 0, 0,
0, module_potentialDerivatives_totalGradient2_81_SOA_v2, 0, 0, 0, 0, 0, 0, 0, 0,
0, 0, 0, 0, 0, 0, 0, 0, 0, 0
};
//
//
//
struct matrix module_potentialDerivatives_totalGradient2_SOA(const struct point *pImage, const struct Potential_SOA *lens, int nhalos)
{
struct matrix grad2, clumpgrad;
//
grad2.a = clumpgrad.a = 0;
grad2.b = clumpgrad.b = 0;
grad2.c = clumpgrad.c = 0;
grad2.d = clumpgrad.d = 0;
//
int shalos = 0;
while (shalos < nhalos)
{
int lens_type = lens->type[shalos];
int count = 1;
while (lens->type[shalos + count] == lens_type and shalos + count < nhalos) count++;
//std::cerr << "type = " << lens_type << " " << count << " " << shalos << " " << nhalos << " " << " func = " << halo_g2_func[lens_type] << std::endl;
//
clumpgrad = (*halo_g2_func[lens_type])(pImage, lens, shalos, count);
//
grad2.a += clumpgrad.a;
grad2.b += clumpgrad.b;
grad2.c += clumpgrad.c;
grad2.d += clumpgrad.d;
shalos += count;
}
return(grad2);
}
//
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