188 lines
5.5 KiB
C++
188 lines
5.5 KiB
C++
/*+
|
|
This is CosmoTool (./sample/testkd3.cpp) -- Copyright (C) Guilhem Lavaux (2007-2014)
|
|
|
|
guilhem.lavaux@gmail.com
|
|
|
|
This software is a computer program whose purpose is to provide a toolbox for cosmological
|
|
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
|
|
|
|
This software is governed by the CeCILL license under French law and
|
|
abiding by the rules of distribution of free software. You can use,
|
|
modify and/ or redistribute the software under the terms of the CeCILL
|
|
license as circulated by CEA, CNRS and INRIA at the following URL
|
|
"http://www.cecill.info".
|
|
|
|
As a counterpart to the access to the source code and rights to copy,
|
|
modify and redistribute granted by the license, users are provided only
|
|
with a limited warranty and the software's author, the holder of the
|
|
economic rights, and the successive licensors have only limited
|
|
liability.
|
|
|
|
In this respect, the user's attention is drawn to the risks associated
|
|
with loading, using, modifying and/or developing or reproducing the
|
|
software by the user in light of its specific status of free software,
|
|
that may mean that it is complicated to manipulate, and that also
|
|
therefore means that it is reserved for developers and experienced
|
|
professionals having in-depth computer knowledge. Users are therefore
|
|
encouraged to load and test the software's suitability as regards their
|
|
requirements in conditions enabling the security of their systems and/or
|
|
data to be ensured and, more generally, to use and operate it in the
|
|
same conditions as regards security.
|
|
|
|
The fact that you are presently reading this means that you have had
|
|
knowledge of the CeCILL license and that you accept its terms.
|
|
+*/
|
|
|
|
#include <ctime>
|
|
#include <cassert>
|
|
#include <cstdlib>
|
|
#include <iostream>
|
|
#include <fstream>
|
|
#define __KD_TREE_NUMNODES
|
|
#include "mykdtree.hpp"
|
|
#include "kdtree_splitters.hpp"
|
|
#include <limits>
|
|
|
|
#define NTRY 30
|
|
#define NGB 24
|
|
#define ND 3
|
|
|
|
using namespace std;
|
|
using namespace CosmoTool;
|
|
|
|
typedef KDTree<ND,char,ComputePrecision,KD_homogeneous_cell_splitter<ND, char> > MyTree;
|
|
//typedef KDTree<ND,char,ComputePrecision > MyTree;
|
|
typedef KDCell<ND,char> MyCell;
|
|
|
|
static double periodic(double a)
|
|
{
|
|
while (a < -0.5)
|
|
a+=1;
|
|
while (a > 0.5)
|
|
a -= 1;
|
|
return a;
|
|
}
|
|
|
|
MyCell *findNearest(MyTree::coords& xc, MyCell *cells, uint32_t Ncells)
|
|
{
|
|
MyCell *near2 = 0;
|
|
double R2 = INFINITY;
|
|
for (int i = 0; i < Ncells; i++)
|
|
{
|
|
double d2 = 0;
|
|
for (int j = 0; j < ND; j++)
|
|
{
|
|
double delta = periodic(xc[j]-cells[i].coord[j]);
|
|
d2 += delta*delta;
|
|
}
|
|
if (d2 < R2)
|
|
{
|
|
near2 = &cells[i];
|
|
R2 = d2;
|
|
}
|
|
}
|
|
return near2;
|
|
}
|
|
|
|
int main()
|
|
{
|
|
uint32_t Ncells = 3000000;
|
|
MyCell *cells = new MyCell[Ncells];
|
|
|
|
for (int i = 0; i < Ncells; i++)
|
|
{
|
|
cells[i].active = true;
|
|
for (int l = 0; l < ND; l++)
|
|
cells[i].coord[l] = drand48();
|
|
}
|
|
|
|
// Check timing
|
|
clock_t startTimer = clock();
|
|
MyTree tree(cells, Ncells);
|
|
clock_t endTimer = clock();
|
|
|
|
tree.setPeriodic(true, 1.0);
|
|
|
|
clock_t delta = endTimer-startTimer;
|
|
double myTime = delta*1.0/CLOCKS_PER_SEC * 1.0;
|
|
|
|
cout << "KDTree build = " << myTime << " s" << endl;
|
|
|
|
MyTree::coords *xc = new MyTree::coords[NTRY];
|
|
|
|
cout << "Generating seeds..." << endl;
|
|
for (int k = 0; k < NTRY; k++)
|
|
{
|
|
for (int l = 0; l < ND; l++)
|
|
xc[k][l] = drand48();
|
|
}
|
|
|
|
// Check consistency
|
|
cout << "Check consistency..." << endl;
|
|
MyCell **ngb = new MyCell *[NGB];
|
|
double *distances = new double[NGB];
|
|
|
|
ofstream fngb("nearest.txt");
|
|
for (int k = 0; k < NTRY; k++) {
|
|
cout << "Seed = " << xc[k][0] << " " << xc[k][1] << " " << xc[k][2] << endl;
|
|
tree.getNearestNeighbours(xc[k], NGB, ngb, distances);
|
|
int last = -1;
|
|
|
|
for (uint32_t i = 0; i < NGB; i++)
|
|
{
|
|
if (ngb[i] == 0)
|
|
continue;
|
|
|
|
last = i;
|
|
|
|
double d2 = 0;
|
|
for (int l = 0; l < 3; l++)
|
|
d2 += ({double delta = periodic(xc[k][l] - ngb[i]->coord[l]); delta*delta;});
|
|
fngb << ngb[i]->coord[0] << " " << ngb[i]->coord[1] << " " << ngb[i]->coord[2] << " " << sqrt(d2) << " " << sqrt(distances[i]) << endl;
|
|
}
|
|
fngb << endl << endl;
|
|
double farther_dist = distances[last];
|
|
for (uint32_t i = 0; i < Ncells; i++)
|
|
{
|
|
bool found = false;
|
|
// If the points is not in the list, it means it is farther than the farthest point
|
|
for (int j =0; j < NGB; j++)
|
|
{
|
|
if (&cells[i] == ngb[j]) {
|
|
found = true;
|
|
break;
|
|
}
|
|
}
|
|
double dist_to_seed = 0;
|
|
for (int l = 0; l < 3; l++)
|
|
{
|
|
double delta = periodic(xc[k][l]-cells[i].coord[l]);
|
|
dist_to_seed += delta*delta;
|
|
}
|
|
double delta_epsilon = fabs(farther_dist/dist_to_seed-1);
|
|
if (!found)
|
|
{
|
|
if (dist_to_seed <= farther_dist &&
|
|
delta_epsilon > 1000*sqrt(numeric_limits<double>::epsilon()))
|
|
{
|
|
cout << "SHOULD BE IN (d=" << dist_to_seed << "): Failed iteration " << k << " particle " << i << " (farthest=" << sqrt(farther_dist) << ")" << endl;
|
|
cout << "delta_epsilon = " << delta_epsilon << endl;
|
|
abort();
|
|
}
|
|
}
|
|
else
|
|
{
|
|
if (dist_to_seed > farther_dist &&
|
|
delta_epsilon > 1000*sqrt(numeric_limits<double>::epsilon()))
|
|
{
|
|
cout << "SHOULD BE OUT (d=" << sqrt(dist_to_seed) << "): Failed iteration " << k << " particle " << i << " (farthest=" << sqrt(farther_dist) << ")" << endl;
|
|
cout << "delta_epsilon = " << delta_epsilon << " epsilon = " << 100*sqrt(numeric_limits<double>::epsilon()) << endl;
|
|
abort();
|
|
}
|
|
}
|
|
}
|
|
}
|
|
|
|
return 0;
|
|
}
|