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RiemannFit.h
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RiemannFit.h
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#ifndef RecoPixelVertexing_PixelTrackFitting_interface_RiemannFit_h
#define RecoPixelVertexing_PixelTrackFitting_interface_RiemannFit_h
#include "RecoPixelVertexing/PixelTrackFitting/interface/FitUtils.h"
namespace Rfit {
/*! Compute the Radiation length in the uniform hypothesis
*
* The Pixel detector, barrel and forward, is considered as an omogeneous
* cilinder of material, whose radiation lengths has been derived from the TDR
* plot that shows that 16cm correspond to 0.06 radiation lengths. Therefore
* one radiation length corresponds to 16cm/0.06 =~ 267 cm. All radiation
* lengths are computed using this unique number, in both regions, barrel and
* endcap.
*
* NB: no angle corrections nor projections are computed inside this routine.
* It is therefore the responsibility of the caller to supply the proper
* lengths in input. These lenghts are the path travelled by the particle along
* its trajectory, namely the so called S of the helix in 3D space.
*
* \param length_values vector of incremental distances that will be translated
* into radiation length equivalent. Each radiation length i is computed
* incrementally with respect to the previous length i-1. The first lenght has
* no reference point (i.e. it has the dca).
*
* \return incremental radiation lengths that correspond to each segment.
*/
template <typename VNd1, typename VNd2>
__host__ __device__ inline void computeRadLenUniformMaterial(const VNd1& length_values, VNd2& rad_lengths) {
// Radiation length of the pixel detector in the uniform assumption, with
// 0.06 rad_len at 16 cm
constexpr double XX_0_inv = 0.06 / 16.;
u_int n = length_values.rows();
rad_lengths(0) = length_values(0) * XX_0_inv;
for (u_int j = 1; j < n; ++j) {
rad_lengths(j) = std::abs(length_values(j) - length_values(j - 1)) * XX_0_inv;
}
}
/*!
\brief Compute the covariance matrix along cartesian S-Z of points due to
multiple Coulomb scattering to be used in the line_fit, for the barrel
and forward cases.
The input covariance matrix is in the variables s-z, original and
unrotated.
The multiple scattering component is computed in the usual linear
approximation, using the 3D path which is computed as the squared root of
the squared sum of the s and z components passed in.
Internally a rotation by theta is performed and the covariance matrix
returned is the one in the direction orthogonal to the rotated S3D axis,
i.e. along the rotated Z axis.
The choice of the rotation is not arbitrary, but derived from the fact that
putting the horizontal axis along the S3D direction allows the usage of the
ordinary least squared fitting techiques with the trivial parametrization y
= mx + q, avoiding the patological case with m = +/- inf, that would
correspond to the case at eta = 0.
*/
template <typename V4, typename VNd1, typename VNd2, int N>
__host__ __device__ inline auto Scatter_cov_line(Matrix2d const* cov_sz,
const V4& fast_fit,
VNd1 const& s_arcs,
VNd2 const& z_values,
const double theta,
const double B,
MatrixNd<N>& ret) {
#ifdef RFIT_DEBUG
Rfit::printIt(&s_arcs, "Scatter_cov_line - s_arcs: ");
#endif
constexpr u_int n = N;
double p_t = std::min(20., fast_fit(2) * B); // limit pt to avoid too small error!!!
double p_2 = p_t * p_t * (1. + 1. / (fast_fit(3) * fast_fit(3)));
VectorNd<N> rad_lengths_S;
// See documentation at http://eigen.tuxfamily.org/dox/group__TutorialArrayClass.html
// Basically, to perform cwise operations on Matrices and Vectors, you need
// to transform them into Array-like objects.
VectorNd<N> S_values = s_arcs.array() * s_arcs.array() + z_values.array() * z_values.array();
S_values = S_values.array().sqrt();
computeRadLenUniformMaterial(S_values, rad_lengths_S);
VectorNd<N> sig2_S;
sig2_S = .000225 / p_2 * (1. + 0.038 * rad_lengths_S.array().log()).abs2() * rad_lengths_S.array();
#ifdef RFIT_DEBUG
Rfit::printIt(cov_sz, "Scatter_cov_line - cov_sz: ");
#endif
Matrix2Nd<N> tmp = Matrix2Nd<N>::Zero();
for (u_int k = 0; k < n; ++k) {
tmp(k, k) = cov_sz[k](0, 0);
tmp(k + n, k + n) = cov_sz[k](1, 1);
tmp(k, k + n) = tmp(k + n, k) = cov_sz[k](0, 1);
}
for (u_int k = 0; k < n; ++k) {
for (u_int l = k; l < n; ++l) {
for (u_int i = 0; i < std::min(k, l); ++i) {
tmp(k + n, l + n) += std::abs(S_values(k) - S_values(i)) * std::abs(S_values(l) - S_values(i)) * sig2_S(i);
}
tmp(l + n, k + n) = tmp(k + n, l + n);
}
}
// We are interested only in the errors orthogonal to the rotated s-axis
// which, in our formalism, are in the lower square matrix.
#ifdef RFIT_DEBUG
Rfit::printIt(&tmp, "Scatter_cov_line - tmp: ");
#endif
ret = tmp.block(n, n, n, n);
}
/*!
\brief Compute the covariance matrix (in radial coordinates) of points in
the transverse plane due to multiple Coulomb scattering.
\param p2D 2D points in the transverse plane.
\param fast_fit fast_fit Vector4d result of the previous pre-fit
structured in this form:(X0, Y0, R, Tan(Theta))).
\param B magnetic field use to compute p
\return scatter_cov_rad errors due to multiple scattering.
\warning input points must be ordered radially from the detector center
(from inner layer to outer ones; points on the same layer must ordered too).
\details Only the tangential component is computed (the radial one is
negligible).
*/
template <typename M2xN, typename V4, int N>
__host__ __device__ inline MatrixNd<N> Scatter_cov_rad(const M2xN& p2D,
const V4& fast_fit,
VectorNd<N> const& rad,
double B) {
constexpr u_int n = N;
double p_t = std::min(20., fast_fit(2) * B); // limit pt to avoid too small error!!!
double p_2 = p_t * p_t * (1. + 1. / (fast_fit(3) * fast_fit(3)));
double theta = atan(fast_fit(3));
theta = theta < 0. ? theta + M_PI : theta;
VectorNd<N> s_values;
VectorNd<N> rad_lengths;
const Vector2d o(fast_fit(0), fast_fit(1));
// associated Jacobian, used in weights and errors computation
for (u_int i = 0; i < n; ++i) { // x
Vector2d p = p2D.block(0, i, 2, 1) - o;
const double cross = cross2D(-o, p);
const double dot = (-o).dot(p);
const double atan2_ = atan2(cross, dot);
s_values(i) = std::abs(atan2_ * fast_fit(2));
}
computeRadLenUniformMaterial(s_values * sqrt(1. + 1. / (fast_fit(3) * fast_fit(3))), rad_lengths);
MatrixNd<N> scatter_cov_rad = MatrixNd<N>::Zero();
VectorNd<N> sig2 = (1. + 0.038 * rad_lengths.array().log()).abs2() * rad_lengths.array();
sig2 *= 0.000225 / (p_2 * sqr(sin(theta)));
for (u_int k = 0; k < n; ++k) {
for (u_int l = k; l < n; ++l) {
for (u_int i = 0; i < std::min(k, l); ++i) {
scatter_cov_rad(k, l) += (rad(k) - rad(i)) * (rad(l) - rad(i)) * sig2(i);
}
scatter_cov_rad(l, k) = scatter_cov_rad(k, l);
}
}
#ifdef RFIT_DEBUG
Rfit::printIt(&scatter_cov_rad, "Scatter_cov_rad - scatter_cov_rad: ");
#endif
return scatter_cov_rad;
}
/*!
\brief Transform covariance matrix from radial (only tangential component)
to Cartesian coordinates (only transverse plane component).
\param p2D 2D points in the transverse plane.
\param cov_rad covariance matrix in radial coordinate.
\return cov_cart covariance matrix in Cartesian coordinates.
*/
template <typename M2xN, int N>
__host__ __device__ inline Matrix2Nd<N> cov_radtocart(const M2xN& p2D,
const MatrixNd<N>& cov_rad,
const VectorNd<N>& rad) {
#ifdef RFIT_DEBUG
printf("Address of p2D: %p\n", &p2D);
#endif
printIt(&p2D, "cov_radtocart - p2D:");
constexpr u_int n = N;
Matrix2Nd<N> cov_cart = Matrix2Nd<N>::Zero();
VectorNd<N> rad_inv = rad.cwiseInverse();
printIt(&rad_inv, "cov_radtocart - rad_inv:");
for (u_int i = 0; i < n; ++i) {
for (u_int j = i; j < n; ++j) {
cov_cart(i, j) = cov_rad(i, j) * p2D(1, i) * rad_inv(i) * p2D(1, j) * rad_inv(j);
cov_cart(i + n, j + n) = cov_rad(i, j) * p2D(0, i) * rad_inv(i) * p2D(0, j) * rad_inv(j);
cov_cart(i, j + n) = -cov_rad(i, j) * p2D(1, i) * rad_inv(i) * p2D(0, j) * rad_inv(j);
cov_cart(i + n, j) = -cov_rad(i, j) * p2D(0, i) * rad_inv(i) * p2D(1, j) * rad_inv(j);
cov_cart(j, i) = cov_cart(i, j);
cov_cart(j + n, i + n) = cov_cart(i + n, j + n);
cov_cart(j + n, i) = cov_cart(i, j + n);
cov_cart(j, i + n) = cov_cart(i + n, j);
}
}
return cov_cart;
}
/*!
\brief Transform covariance matrix from Cartesian coordinates (only
transverse plane component) to radial coordinates (both radial and
tangential component but only diagonal terms, correlation between different
point are not managed).
\param p2D 2D points in transverse plane.
\param cov_cart covariance matrix in Cartesian coordinates.
\return cov_rad covariance matrix in raidal coordinate.
\warning correlation between different point are not computed.
*/
template <typename M2xN, int N>
__host__ __device__ inline VectorNd<N> cov_carttorad(const M2xN& p2D,
const Matrix2Nd<N>& cov_cart,
const VectorNd<N>& rad) {
constexpr u_int n = N;
VectorNd<N> cov_rad;
const VectorNd<N> rad_inv2 = rad.cwiseInverse().array().square();
for (u_int i = 0; i < n; ++i) {
//!< in case you have (0,0) to avoid dividing by 0 radius
if (rad(i) < 1.e-4)
cov_rad(i) = cov_cart(i, i);
else {
cov_rad(i) = rad_inv2(i) * (cov_cart(i, i) * sqr(p2D(1, i)) + cov_cart(i + n, i + n) * sqr(p2D(0, i)) -
2. * cov_cart(i, i + n) * p2D(0, i) * p2D(1, i));
}
}
return cov_rad;
}
/*!
\brief Transform covariance matrix from Cartesian coordinates (only
transverse plane component) to coordinates system orthogonal to the
pre-fitted circle in each point.
Further information in attached documentation.
\param p2D 2D points in transverse plane.
\param cov_cart covariance matrix in Cartesian coordinates.
\param fast_fit fast_fit Vector4d result of the previous pre-fit
structured in this form:(X0, Y0, R, tan(theta))).
\return cov_rad covariance matrix in the pre-fitted circle's
orthogonal system.
*/
template <typename M2xN, typename V4, int N>
__host__ __device__ inline VectorNd<N> cov_carttorad_prefit(const M2xN& p2D,
const Matrix2Nd<N>& cov_cart,
V4& fast_fit,
const VectorNd<N>& rad) {
constexpr u_int n = N;
VectorNd<N> cov_rad;
for (u_int i = 0; i < n; ++i) {
//!< in case you have (0,0) to avoid dividing by 0 radius
if (rad(i) < 1.e-4)
cov_rad(i) = cov_cart(i, i); // TO FIX
else {
Vector2d a = p2D.col(i);
Vector2d b = p2D.col(i) - fast_fit.head(2);
const double x2 = a.dot(b);
const double y2 = cross2D(a, b);
const double tan_c = -y2 / x2;
const double tan_c2 = sqr(tan_c);
cov_rad(i) =
1. / (1. + tan_c2) * (cov_cart(i, i) + cov_cart(i + n, i + n) * tan_c2 + 2 * cov_cart(i, i + n) * tan_c);
}
}
return cov_rad;
}
/*!
\brief Compute the points' weights' vector for the circle fit when multiple
scattering is managed.
Further information in attached documentation.
\param cov_rad_inv covariance matrix inverse in radial coordinated
(or, beter, pre-fitted circle's orthogonal system).
\return weight VectorNd points' weights' vector.
\bug I'm not sure this is the right way to compute the weights for non
diagonal cov matrix. Further investigation needed.
*/
template <int N>
__host__ __device__ inline VectorNd<N> Weight_circle(const MatrixNd<N>& cov_rad_inv) {
return cov_rad_inv.colwise().sum().transpose();
}
/*!
\brief Find particle q considering the sign of cross product between
particles velocity (estimated by the first 2 hits) and the vector radius
between the first hit and the center of the fitted circle.
\param p2D 2D points in transverse plane.
\param par_uvr result of the circle fit in this form: (X0,Y0,R).
\return q int 1 or -1.
*/
template <typename M2xN>
__host__ __device__ inline int32_t Charge(const M2xN& p2D, const Vector3d& par_uvr) {
return ((p2D(0, 1) - p2D(0, 0)) * (par_uvr.y() - p2D(1, 0)) - (p2D(1, 1) - p2D(1, 0)) * (par_uvr.x() - p2D(0, 0)) >
0)
? -1
: 1;
}
/*!
\brief Compute the eigenvector associated to the minimum eigenvalue.
\param A the Matrix you want to know eigenvector and eigenvalue.
\param chi2 the double were the chi2-related quantity will be stored.
\return the eigenvector associated to the minimum eigenvalue.
\warning double precision is needed for a correct assessment of chi2.
\details The minimus eigenvalue is related to chi2.
We exploit the fact that the matrix is symmetrical and small (2x2 for line
fit and 3x3 for circle fit), so the SelfAdjointEigenSolver from Eigen
library is used, with the computedDirect method (available only for 2x2
and 3x3 Matrix) wich computes eigendecomposition of given matrix using a
fast closed-form algorithm.
For this optimization the matrix type must be known at compiling time.
*/
__host__ __device__ inline Vector3d min_eigen3D(const Matrix3d& A, double& chi2) {
#ifdef RFIT_DEBUG
printf("min_eigen3D - enter\n");
#endif
Eigen::SelfAdjointEigenSolver<Matrix3d> solver(3);
solver.computeDirect(A);
int min_index;
chi2 = solver.eigenvalues().minCoeff(&min_index);
#ifdef RFIT_DEBUG
printf("min_eigen3D - exit\n");
#endif
return solver.eigenvectors().col(min_index);
}
/*!
\brief A faster version of min_eigen3D() where double precision is not
needed.
\param A the Matrix you want to know eigenvector and eigenvalue.
\param chi2 the double were the chi2-related quantity will be stored
\return the eigenvector associated to the minimum eigenvalue.
\detail The computedDirect() method of SelfAdjointEigenSolver for 3x3 Matrix
indeed, use trigonometry function (it solves a third degree equation) which
speed up in single precision.
*/
__host__ __device__ inline Vector3d min_eigen3D_fast(const Matrix3d& A) {
Eigen::SelfAdjointEigenSolver<Matrix3f> solver(3);
solver.computeDirect(A.cast<float>());
int min_index;
solver.eigenvalues().minCoeff(&min_index);
return solver.eigenvectors().col(min_index).cast<double>();
}
/*!
\brief 2D version of min_eigen3D().
\param A the Matrix you want to know eigenvector and eigenvalue.
\param chi2 the double were the chi2-related quantity will be stored
\return the eigenvector associated to the minimum eigenvalue.
\detail The computedDirect() method of SelfAdjointEigenSolver for 2x2 Matrix
do not use special math function (just sqrt) therefore it doesn't speed up
significantly in single precision.
*/
__host__ __device__ inline Vector2d min_eigen2D(const Matrix2d& A, double& chi2) {
Eigen::SelfAdjointEigenSolver<Matrix2d> solver(2);
solver.computeDirect(A);
int min_index;
chi2 = solver.eigenvalues().minCoeff(&min_index);
return solver.eigenvectors().col(min_index);
}
/*!
\brief A very fast helix fit: it fits a circle by three points (first, middle
and last point) and a line by two points (first and last).
\param hits points to be fitted
\return result in this form: (X0,Y0,R,tan(theta)).
\warning points must be passed ordered (from internal layer to external) in
order to maximize accuracy and do not mistake tan(theta) sign.
\details This fast fit is used as pre-fit which is needed for:
- weights estimation and chi2 computation in line fit (fundamental);
- weights estimation and chi2 computation in circle fit (useful);
- computation of error due to multiple scattering.
*/
template <typename M3xN, typename V4>
__host__ __device__ inline void Fast_fit(const M3xN& hits, V4& result) {
constexpr uint32_t N = M3xN::ColsAtCompileTime;
constexpr auto n = N; // get the number of hits
printIt(&hits, "Fast_fit - hits: ");
// CIRCLE FIT
// Make segments between middle-to-first(b) and last-to-first(c) hits
const Vector2d b = hits.block(0, n / 2, 2, 1) - hits.block(0, 0, 2, 1);
const Vector2d c = hits.block(0, n - 1, 2, 1) - hits.block(0, 0, 2, 1);
printIt(&b, "Fast_fit - b: ");
printIt(&c, "Fast_fit - c: ");
// Compute their lengths
auto b2 = b.squaredNorm();
auto c2 = c.squaredNorm();
// The algebra has been verified (MR). The usual approach has been followed:
// * use an orthogonal reference frame passing from the first point.
// * build the segments (chords)
// * build orthogonal lines through mid points
// * make a system and solve for X0 and Y0.
// * add the initial point
bool flip = abs(b.x()) < abs(b.y());
auto bx = flip ? b.y() : b.x();
auto by = flip ? b.x() : b.y();
auto cx = flip ? c.y() : c.x();
auto cy = flip ? c.x() : c.y();
//!< in case b.x is 0 (2 hits with same x)
auto div = 2. * (cx * by - bx * cy);
// if aligned TO FIX
auto Y0 = (cx * b2 - bx * c2) / div;
auto X0 = (0.5 * b2 - Y0 * by) / bx;
result(0) = hits(0, 0) + (flip ? Y0 : X0);
result(1) = hits(1, 0) + (flip ? X0 : Y0);
result(2) = sqrt(sqr(X0) + sqr(Y0));
printIt(&result, "Fast_fit - result: ");
// LINE FIT
const Vector2d d = hits.block(0, 0, 2, 1) - result.head(2);
const Vector2d e = hits.block(0, n - 1, 2, 1) - result.head(2);
printIt(&e, "Fast_fit - e: ");
printIt(&d, "Fast_fit - d: ");
// Compute the arc-length between first and last point: L = R * theta = R * atan (tan (Theta) )
auto dr = result(2) * atan2(cross2D(d, e), d.dot(e));
// Simple difference in Z between last and first hit
auto dz = hits(2, n - 1) - hits(2, 0);
result(3) = (dr / dz);
#ifdef RFIT_DEBUG
printf("Fast_fit: [%f, %f, %f, %f]\n", result(0), result(1), result(2), result(3));
#endif
}
/*!
\brief Fit a generic number of 2D points with a circle using Riemann-Chernov
algorithm. Covariance matrix of fitted parameter is optionally computed.
Multiple scattering (currently only in barrel layer) is optionally handled.
\param hits2D 2D points to be fitted.
\param hits_cov2D covariance matrix of 2D points.
\param fast_fit pre-fit result in this form: (X0,Y0,R,tan(theta)).
(tan(theta) is not used).
\param B magnetic field
\param error flag for error computation.
\param scattering flag for multiple scattering
\return circle circle_fit:
-par parameter of the fitted circle in this form (X0,Y0,R); \n
-cov covariance matrix of the fitted parameter (not initialized if
error = false); \n
-q charge of the particle; \n
-chi2.
\warning hits must be passed ordered from inner to outer layer (double hits
on the same layer must be ordered too) so that multiple scattering is
treated properly.
\warning Multiple scattering for barrel is still not tested.
\warning Multiple scattering for endcap hits is not handled (yet). Do not
fit endcap hits with scattering = true !
\bug for small pt (<0.3 Gev/c) chi2 could be slightly underestimated.
\bug further investigation needed for error propagation with multiple
scattering.
*/
template <typename M2xN, typename V4, int N>
__host__ __device__ inline circle_fit Circle_fit(const M2xN& hits2D,
const Matrix2Nd<N>& hits_cov2D,
const V4& fast_fit,
const VectorNd<N>& rad,
const double B,
const bool error) {
#ifdef RFIT_DEBUG
printf("circle_fit - enter\n");
#endif
// INITIALIZATION
Matrix2Nd<N> V = hits_cov2D;
constexpr u_int n = N;
printIt(&hits2D, "circle_fit - hits2D:");
printIt(&hits_cov2D, "circle_fit - hits_cov2D:");
#ifdef RFIT_DEBUG
printf("circle_fit - WEIGHT COMPUTATION\n");
#endif
// WEIGHT COMPUTATION
VectorNd<N> weight;
MatrixNd<N> G;
double renorm;
{
MatrixNd<N> cov_rad = cov_carttorad_prefit(hits2D, V, fast_fit, rad).asDiagonal();
MatrixNd<N> scatter_cov_rad = Scatter_cov_rad(hits2D, fast_fit, rad, B);
printIt(&scatter_cov_rad, "circle_fit - scatter_cov_rad:");
printIt(&hits2D, "circle_fit - hits2D bis:");
#ifdef RFIT_DEBUG
printf("Address of hits2D: a) %p\n", &hits2D);
#endif
V += cov_radtocart(hits2D, scatter_cov_rad, rad);
printIt(&V, "circle_fit - V:");
cov_rad += scatter_cov_rad;
printIt(&cov_rad, "circle_fit - cov_rad:");
math::cholesky::invert(cov_rad, G);
// G = cov_rad.inverse();
renorm = G.sum();
G *= 1. / renorm;
weight = Weight_circle(G);
}
printIt(&weight, "circle_fit - weight:");
// SPACE TRANSFORMATION
#ifdef RFIT_DEBUG
printf("circle_fit - SPACE TRANSFORMATION\n");
#endif
// center
#ifdef RFIT_DEBUG
printf("Address of hits2D: b) %p\n", &hits2D);
#endif
const Vector2d h_ = hits2D.rowwise().mean(); // centroid
printIt(&h_, "circle_fit - h_:");
Matrix3xNd<N> p3D;
p3D.block(0, 0, 2, n) = hits2D.colwise() - h_;
printIt(&p3D, "circle_fit - p3D: a)");
Vector2Nd<N> mc; // centered hits, used in error computation
mc << p3D.row(0).transpose(), p3D.row(1).transpose();
printIt(&mc, "circle_fit - mc(centered hits):");
// scale
const double q = mc.squaredNorm();
const double s = sqrt(n * 1. / q); // scaling factor
p3D *= s;
// project on paraboloid
p3D.row(2) = p3D.block(0, 0, 2, n).colwise().squaredNorm();
printIt(&p3D, "circle_fit - p3D: b)");
#ifdef RFIT_DEBUG
printf("circle_fit - COST FUNCTION\n");
#endif
// COST FUNCTION
// compute
Vector3d r0;
r0.noalias() = p3D * weight; // center of gravity
const Matrix3xNd<N> X = p3D.colwise() - r0;
Matrix3d A = X * G * X.transpose();
printIt(&A, "circle_fit - A:");
#ifdef RFIT_DEBUG
printf("circle_fit - MINIMIZE\n");
#endif
// minimize
double chi2;
Vector3d v = min_eigen3D(A, chi2);
#ifdef RFIT_DEBUG
printf("circle_fit - AFTER MIN_EIGEN\n");
#endif
printIt(&v, "v BEFORE INVERSION");
v *= (v(2) > 0) ? 1 : -1; // TO FIX dovrebbe essere N(3)>0
printIt(&v, "v AFTER INVERSION");
// This hack to be able to run on GPU where the automatic assignment to a
// double from the vector multiplication is not working.
#ifdef RFIT_DEBUG
printf("circle_fit - AFTER MIN_EIGEN 1\n");
#endif
Eigen::Matrix<double, 1, 1> cm;
#ifdef RFIT_DEBUG
printf("circle_fit - AFTER MIN_EIGEN 2\n");
#endif
cm = -v.transpose() * r0;
#ifdef RFIT_DEBUG
printf("circle_fit - AFTER MIN_EIGEN 3\n");
#endif
const double c = cm(0, 0);
// const double c = -v.transpose() * r0;
#ifdef RFIT_DEBUG
printf("circle_fit - COMPUTE CIRCLE PARAMETER\n");
#endif
// COMPUTE CIRCLE PARAMETER
// auxiliary quantities
const double h = sqrt(1. - sqr(v(2)) - 4. * c * v(2));
const double v2x2_inv = 1. / (2. * v(2));
const double s_inv = 1. / s;
Vector3d par_uvr_; // used in error propagation
par_uvr_ << -v(0) * v2x2_inv, -v(1) * v2x2_inv, h * v2x2_inv;
circle_fit circle;
circle.par << par_uvr_(0) * s_inv + h_(0), par_uvr_(1) * s_inv + h_(1), par_uvr_(2) * s_inv;
circle.q = Charge(hits2D, circle.par);
circle.chi2 = abs(chi2) * renorm * 1. / sqr(2 * v(2) * par_uvr_(2) * s);
printIt(&circle.par, "circle_fit - CIRCLE PARAMETERS:");
printIt(&circle.cov, "circle_fit - CIRCLE COVARIANCE:");
#ifdef RFIT_DEBUG
printf("circle_fit - CIRCLE CHARGE: %d\n", circle.q);
#endif
#ifdef RFIT_DEBUG
printf("circle_fit - ERROR PROPAGATION\n");
#endif
// ERROR PROPAGATION
if (error) {
#ifdef RFIT_DEBUG
printf("circle_fit - ERROR PRPAGATION ACTIVATED\n");
#endif
ArrayNd<N> Vcs_[2][2]; // cov matrix of center & scaled points
MatrixNd<N> C[3][3]; // cov matrix of 3D transformed points
#ifdef RFIT_DEBUG
printf("circle_fit - ERROR PRPAGATION ACTIVATED 2\n");
#endif
{
Eigen::Matrix<double, 1, 1> cm;
Eigen::Matrix<double, 1, 1> cm2;
cm = mc.transpose() * V * mc;
const double c = cm(0, 0);
Matrix2Nd<N> Vcs;
Vcs.template triangularView<Eigen::Upper>() =
(sqr(s) * V + sqr(sqr(s)) * 1. / (4. * q * n) *
(2. * V.squaredNorm() + 4. * c) * // mc.transpose() * V * mc) *
(mc * mc.transpose()));
printIt(&Vcs, "circle_fit - Vcs:");
C[0][0] = Vcs.block(0, 0, n, n).template selfadjointView<Eigen::Upper>();
Vcs_[0][1] = Vcs.block(0, n, n, n);
C[1][1] = Vcs.block(n, n, n, n).template selfadjointView<Eigen::Upper>();
Vcs_[1][0] = Vcs_[0][1].transpose();
printIt(&Vcs, "circle_fit - Vcs:");
}
{
const ArrayNd<N> t0 = (VectorXd::Constant(n, 1.) * p3D.row(0));
const ArrayNd<N> t1 = (VectorXd::Constant(n, 1.) * p3D.row(1));
const ArrayNd<N> t00 = p3D.row(0).transpose() * p3D.row(0);
const ArrayNd<N> t01 = p3D.row(0).transpose() * p3D.row(1);
const ArrayNd<N> t11 = p3D.row(1).transpose() * p3D.row(1);
const ArrayNd<N> t10 = t01.transpose();
Vcs_[0][0] = C[0][0];
;
C[0][1] = Vcs_[0][1];
C[0][2] = 2. * (Vcs_[0][0] * t0 + Vcs_[0][1] * t1);
Vcs_[1][1] = C[1][1];
C[1][2] = 2. * (Vcs_[1][0] * t0 + Vcs_[1][1] * t1);
MatrixNd<N> tmp;
tmp.template triangularView<Eigen::Upper>() =
(2. * (Vcs_[0][0] * Vcs_[0][0] + Vcs_[0][0] * Vcs_[0][1] + Vcs_[1][1] * Vcs_[1][0] +
Vcs_[1][1] * Vcs_[1][1]) +
4. * (Vcs_[0][0] * t00 + Vcs_[0][1] * t01 + Vcs_[1][0] * t10 + Vcs_[1][1] * t11))
.matrix();
C[2][2] = tmp.template selfadjointView<Eigen::Upper>();
}
printIt(&C[0][0], "circle_fit - C[0][0]:");
Matrix3d C0; // cov matrix of center of gravity (r0.x,r0.y,r0.z)
for (u_int i = 0; i < 3; ++i) {
for (u_int j = i; j < 3; ++j) {
Eigen::Matrix<double, 1, 1> tmp;
tmp = weight.transpose() * C[i][j] * weight;
const double c = tmp(0, 0);
C0(i, j) = c; //weight.transpose() * C[i][j] * weight;
C0(j, i) = C0(i, j);
}
}
printIt(&C0, "circle_fit - C0:");
const MatrixNd<N> W = weight * weight.transpose();
const MatrixNd<N> H = MatrixNd<N>::Identity().rowwise() - weight.transpose();
const MatrixNx3d<N> s_v = H * p3D.transpose();
printIt(&W, "circle_fit - W:");
printIt(&H, "circle_fit - H:");
printIt(&s_v, "circle_fit - s_v:");
MatrixNd<N> D_[3][3]; // cov(s_v)
{
D_[0][0] = (H * C[0][0] * H.transpose()).cwiseProduct(W);
D_[0][1] = (H * C[0][1] * H.transpose()).cwiseProduct(W);
D_[0][2] = (H * C[0][2] * H.transpose()).cwiseProduct(W);
D_[1][1] = (H * C[1][1] * H.transpose()).cwiseProduct(W);
D_[1][2] = (H * C[1][2] * H.transpose()).cwiseProduct(W);
D_[2][2] = (H * C[2][2] * H.transpose()).cwiseProduct(W);
D_[1][0] = D_[0][1].transpose();
D_[2][0] = D_[0][2].transpose();
D_[2][1] = D_[1][2].transpose();
}
printIt(&D_[0][0], "circle_fit - D_[0][0]:");
constexpr u_int nu[6][2] = {{0, 0}, {0, 1}, {0, 2}, {1, 1}, {1, 2}, {2, 2}};
Matrix6d E; // cov matrix of the 6 independent elements of A
for (u_int a = 0; a < 6; ++a) {
const u_int i = nu[a][0], j = nu[a][1];
for (u_int b = a; b < 6; ++b) {
const u_int k = nu[b][0], l = nu[b][1];
VectorNd<N> t0(n);
VectorNd<N> t1(n);
if (l == k) {
t0 = 2. * D_[j][l] * s_v.col(l);
if (i == j)
t1 = t0;
else
t1 = 2. * D_[i][l] * s_v.col(l);
} else {
t0 = D_[j][l] * s_v.col(k) + D_[j][k] * s_v.col(l);
if (i == j)
t1 = t0;
else
t1 = D_[i][l] * s_v.col(k) + D_[i][k] * s_v.col(l);
}
if (i == j) {
Eigen::Matrix<double, 1, 1> cm;
cm = s_v.col(i).transpose() * (t0 + t1);
const double c = cm(0, 0);
E(a, b) = 0. + c;
} else {
Eigen::Matrix<double, 1, 1> cm;
cm = (s_v.col(i).transpose() * t0) + (s_v.col(j).transpose() * t1);
const double c = cm(0, 0);
E(a, b) = 0. + c; //(s_v.col(i).transpose() * t0) + (s_v.col(j).transpose() * t1);
}
if (b != a)
E(b, a) = E(a, b);
}
}
printIt(&E, "circle_fit - E:");
Eigen::Matrix<double, 3, 6> J2; // Jacobian of min_eigen() (numerically computed)
for (u_int a = 0; a < 6; ++a) {
const u_int i = nu[a][0], j = nu[a][1];
Matrix3d Delta = Matrix3d::Zero();
Delta(i, j) = Delta(j, i) = abs(A(i, j) * d);
J2.col(a) = min_eigen3D_fast(A + Delta);
const int sign = (J2.col(a)(2) > 0) ? 1 : -1;
J2.col(a) = (J2.col(a) * sign - v) / Delta(i, j);
}
printIt(&J2, "circle_fit - J2:");
Matrix4d Cvc; // joint cov matrix of (v0,v1,v2,c)
{
Matrix3d t0 = J2 * E * J2.transpose();
Vector3d t1 = -t0 * r0;
Cvc.block(0, 0, 3, 3) = t0;
Cvc.block(0, 3, 3, 1) = t1;
Cvc.block(3, 0, 1, 3) = t1.transpose();
Eigen::Matrix<double, 1, 1> cm1;
Eigen::Matrix<double, 1, 1> cm3;
cm1 = (v.transpose() * C0 * v);
// cm2 = (C0.cwiseProduct(t0)).sum();
cm3 = (r0.transpose() * t0 * r0);
const double c = cm1(0, 0) + (C0.cwiseProduct(t0)).sum() + cm3(0, 0);
Cvc(3, 3) = c;
// (v.transpose() * C0 * v) + (C0.cwiseProduct(t0)).sum() + (r0.transpose() * t0 * r0);
}
printIt(&Cvc, "circle_fit - Cvc:");
Eigen::Matrix<double, 3, 4> J3; // Jacobian (v0,v1,v2,c)->(X0,Y0,R)
{
const double t = 1. / h;
J3 << -v2x2_inv, 0, v(0) * sqr(v2x2_inv) * 2., 0, 0, -v2x2_inv, v(1) * sqr(v2x2_inv) * 2., 0,
v(0) * v2x2_inv * t, v(1) * v2x2_inv * t, -h * sqr(v2x2_inv) * 2. - (2. * c + v(2)) * v2x2_inv * t, -t;
}
printIt(&J3, "circle_fit - J3:");
const RowVector2Nd<N> Jq = mc.transpose() * s * 1. / n; // var(q)
printIt(&Jq, "circle_fit - Jq:");
Matrix3d cov_uvr = J3 * Cvc * J3.transpose() * sqr(s_inv) // cov(X0,Y0,R)
+ (par_uvr_ * par_uvr_.transpose()) * (Jq * V * Jq.transpose());
circle.cov = cov_uvr;
}
printIt(&circle.cov, "Circle cov:");
#ifdef RFIT_DEBUG
printf("circle_fit - exit\n");
#endif
return circle;
}
/*! \brief Perform an ordinary least square fit in the s-z plane to compute
* the parameters cotTheta and Zip.
*
* The fit is performed in the rotated S3D-Z' plane, following the formalism of
* Frodesen, Chapter 10, p. 259.
*
* The system has been rotated to both try to use the combined errors in s-z
* along Z', as errors in the Y direction and to avoid the patological case of
* degenerate lines with angular coefficient m = +/- inf.
*
* The rotation is using the information on the theta angle computed in the
* fast fit. The rotation is such that the S3D axis will be the X-direction,
* while the rotated Z-axis will be the Y-direction. This pretty much follows
* what is done in the same fit in the Broken Line approach.
*/
template <typename M3xN, typename M6xN, typename V4>
__host__ __device__ inline line_fit Line_fit(const M3xN& hits,
const M6xN& hits_ge,
const circle_fit& circle,
const V4& fast_fit,
const double B,
const bool error) {
constexpr uint32_t N = M3xN::ColsAtCompileTime;
constexpr auto n = N;
double theta = -circle.q * atan(fast_fit(3));
theta = theta < 0. ? theta + M_PI : theta;
// Prepare the Rotation Matrix to rotate the points
Eigen::Matrix<double, 2, 2> rot;
rot << sin(theta), cos(theta), -cos(theta), sin(theta);
// PROJECTION ON THE CILINDER
//
// p2D will be:
// [s1, s2, s3, ..., sn]
// [z1, z2, z3, ..., zn]
// s values will be ordinary x-values
// z values will be ordinary y-values
Matrix2xNd<N> p2D = Matrix2xNd<N>::Zero();
Eigen::Matrix<double, 2, 6> Jx;
#ifdef RFIT_DEBUG
printf("Line_fit - B: %g\n", B);
printIt(&hits, "Line_fit points: ");
printIt(&hits_ge, "Line_fit covs: ");
printIt(&rot, "Line_fit rot: ");
#endif
// x & associated Jacobian
// cfr https://indico.cern.ch/event/663159/contributions/2707659/attachments/1517175/2368189/Riemann_fit.pdf
// Slide 11
// a ==> -o i.e. the origin of the circle in XY plane, negative
// b ==> p i.e. distances of the points wrt the origin of the circle.
const Vector2d o(circle.par(0), circle.par(1));
// associated Jacobian, used in weights and errors computation
Matrix6d Cov = Matrix6d::Zero();
Matrix2d cov_sz[N];
for (u_int i = 0; i < n; ++i) {
Vector2d p = hits.block(0, i, 2, 1) - o;
const double cross = cross2D(-o, p);
const double dot = (-o).dot(p);
// atan2(cross, dot) give back the angle in the transverse plane so tha the
// final equation reads: x_i = -q*R*theta (theta = angle returned by atan2)
const double atan2_ = -circle.q * atan2(cross, dot);
// p2D.coeffRef(1, i) = atan2_ * circle.par(2);
p2D(0, i) = atan2_ * circle.par(2);
// associated Jacobian, used in weights and errors- computation
const double temp0 = -circle.q * circle.par(2) * 1. / (sqr(dot) + sqr(cross));
double d_X0 = 0., d_Y0 = 0., d_R = 0.; // good approximation for big pt and eta
if (error) {
d_X0 = -temp0 * ((p(1) + o(1)) * dot - (p(0) - o(0)) * cross);
d_Y0 = temp0 * ((p(0) + o(0)) * dot - (o(1) - p(1)) * cross);
d_R = atan2_;
}
const double d_x = temp0 * (o(1) * dot + o(0) * cross);
const double d_y = temp0 * (-o(0) * dot + o(1) * cross);
Jx << d_X0, d_Y0, d_R, d_x, d_y, 0., 0., 0., 0., 0., 0., 1.;
Cov.block(0, 0, 3, 3) = circle.cov;
Cov(3, 3) = hits_ge.col(i)[0]; // x errors
Cov(4, 4) = hits_ge.col(i)[2]; // y errors
Cov(5, 5) = hits_ge.col(i)[5]; // z errors
Cov(3, 4) = Cov(4, 3) = hits_ge.col(i)[1]; // cov_xy
Cov(3, 5) = Cov(5, 3) = hits_ge.col(i)[3]; // cov_xz
Cov(4, 5) = Cov(5, 4) = hits_ge.col(i)[4]; // cov_yz
Matrix2d tmp = Jx * Cov * Jx.transpose();
cov_sz[i].noalias() = rot * tmp * rot.transpose();
}
// Math of d_{X0,Y0,R,x,y} all verified by hand
p2D.row(1) = hits.row(2);
// The following matrix will contain errors orthogonal to the rotated S
// component only, with the Multiple Scattering properly treated!!
MatrixNd<N> cov_with_ms;
Scatter_cov_line(cov_sz, fast_fit, p2D.row(0), p2D.row(1), theta, B, cov_with_ms);
#ifdef RFIT_DEBUG
printIt(cov_sz, "line_fit - cov_sz:");
printIt(&cov_with_ms, "line_fit - cov_with_ms: ");
#endif
// Rotate Points with the shape [2, n]
Matrix2xNd<N> p2D_rot = rot * p2D;
#ifdef RFIT_DEBUG
printf("Fast fit Tan(theta): %g\n", fast_fit(3));
printf("Rotation angle: %g\n", theta);
printIt(&rot, "Rotation Matrix:");
printIt(&p2D, "Original Hits(s,z):");
printIt(&p2D_rot, "Rotated hits(S3D, Z'):");
printIt(&rot, "Rotation Matrix:");
#endif
// Build the A Matrix
Matrix2xNd<N> A;
A << MatrixXd::Ones(1, n), p2D_rot.row(0); // rotated s values
#ifdef RFIT_DEBUG
printIt(&A, "A Matrix:");
#endif
// Build A^T V-1 A, where V-1 is the covariance of only the Y components.
MatrixNd<N> Vy_inv;
math::cholesky::invert(cov_with_ms, Vy_inv);
// MatrixNd<N> Vy_inv = cov_with_ms.inverse();
Eigen::Matrix<double, 2, 2> Cov_params = A * Vy_inv * A.transpose();
// Compute the Covariance Matrix of the fit parameters
math::cholesky::invert(Cov_params, Cov_params);
// Now Compute the Parameters in the form [2,1]
// The first component is q.
// The second component is m.
Eigen::Matrix<double, 2, 1> sol = Cov_params * A * Vy_inv * p2D_rot.row(1).transpose();
#ifdef RFIT_DEBUG
printIt(&sol, "Rotated solutions:");
#endif
// We need now to transfer back the results in the original s-z plane
auto common_factor = 1. / (sin(theta) - sol(1, 0) * cos(theta));
Eigen::Matrix<double, 2, 2> J;
J << 0., common_factor * common_factor, common_factor, sol(0, 0) * cos(theta) * common_factor * common_factor;
double m = common_factor * (sol(1, 0) * sin(theta) + cos(theta));
double q = common_factor * sol(0, 0);
auto cov_mq = J * Cov_params * J.transpose();
VectorNd<N> res = p2D_rot.row(1).transpose() - A.transpose() * sol;
double chi2 = res.transpose() * Vy_inv * res;
line_fit line;
line.par << m, q;
line.cov << cov_mq;
line.chi2 = chi2;
#ifdef RFIT_DEBUG
printf("Common_factor: %g\n", common_factor);
printIt(&J, "Jacobian:");
printIt(&sol, "Rotated solutions:");
printIt(&Cov_params, "Cov_params:");
printIt(&cov_mq, "Rotated Covariance Matrix:");
printIt(&(line.par), "Real Parameters:");
printIt(&(line.cov), "Real Covariance Matrix:");
printf("Chi2: %g\n", chi2);
#endif
return line;
}
/*!
\brief Helix fit by three step:
-fast pre-fit (see Fast_fit() for further info); \n
-circle fit of hits projected in the transverse plane by Riemann-Chernov
algorithm (see Circle_fit() for further info); \n
-line fit of hits projected on cylinder surface by orthogonal distance
regression (see Line_fit for further info). \n
Points must be passed ordered (from inner to outer layer).
\param hits Matrix3xNd hits coordinates in this form: \n
|x0|x1|x2|...|xn| \n
|y0|y1|y2|...|yn| \n
|z0|z1|z2|...|zn|
\param hits_cov Matrix3Nd covariance matrix in this form (()->cov()): \n
|(x0,x0)|(x1,x0)|(x2,x0)|.|(y0,x0)|(y1,x0)|(y2,x0)|.|(z0,x0)|(z1,x0)|(z2,x0)| \n
|(x0,x1)|(x1,x1)|(x2,x1)|.|(y0,x1)|(y1,x1)|(y2,x1)|.|(z0,x1)|(z1,x1)|(z2,x1)| \n
|(x0,x2)|(x1,x2)|(x2,x2)|.|(y0,x2)|(y1,x2)|(y2,x2)|.|(z0,x2)|(z1,x2)|(z2,x2)| \n
. . . . . . . . . . . \n
|(x0,y0)|(x1,y0)|(x2,y0)|.|(y0,y0)|(y1,y0)|(y2,x0)|.|(z0,y0)|(z1,y0)|(z2,y0)| \n
|(x0,y1)|(x1,y1)|(x2,y1)|.|(y0,y1)|(y1,y1)|(y2,x1)|.|(z0,y1)|(z1,y1)|(z2,y1)| \n
|(x0,y2)|(x1,y2)|(x2,y2)|.|(y0,y2)|(y1,y2)|(y2,x2)|.|(z0,y2)|(z1,y2)|(z2,y2)| \n
. . . . . . . . . . . \n
|(x0,z0)|(x1,z0)|(x2,z0)|.|(y0,z0)|(y1,z0)|(y2,z0)|.|(z0,z0)|(z1,z0)|(z2,z0)| \n
|(x0,z1)|(x1,z1)|(x2,z1)|.|(y0,z1)|(y1,z1)|(y2,z1)|.|(z0,z1)|(z1,z1)|(z2,z1)| \n
|(x0,z2)|(x1,z2)|(x2,z2)|.|(y0,z2)|(y1,z2)|(y2,z2)|.|(z0,z2)|(z1,z2)|(z2,z2)|
\param B magnetic field in the center of the detector in Gev/cm/c
unit, in order to perform pt calculation.
\param error flag for error computation.
\param scattering flag for multiple scattering treatment.
(see Circle_fit() documentation for further info).
\warning see Circle_fit(), Line_fit() and Fast_fit() warnings.
\bug see Circle_fit(), Line_fit() and Fast_fit() bugs.
*/
template <int N>
inline helix_fit Helix_fit(const Matrix3xNd<N>& hits,
const Eigen::Matrix<float, 6, N>& hits_ge,
const double B,
const bool error) {
constexpr u_int n = N;
VectorNd<4> rad = (hits.block(0, 0, 2, n).colwise().norm());
// Fast_fit gives back (X0, Y0, R, theta) w/o errors, using only 3 points.
Vector4d fast_fit;
Fast_fit(hits, fast_fit);
Rfit::Matrix2Nd<N> hits_cov = MatrixXd::Zero(2 * n, 2 * n);
Rfit::loadCovariance2D(hits_ge, hits_cov);
circle_fit circle = Circle_fit(hits.block(0, 0, 2, n), hits_cov, fast_fit, rad, B, error);
line_fit line = Line_fit(hits, hits_ge, circle, fast_fit, B, error);
par_uvrtopak(circle, B, error);
helix_fit helix;
helix.par << circle.par, line.par;
if (error) {
helix.cov = MatrixXd::Zero(5, 5);
helix.cov.block(0, 0, 3, 3) = circle.cov;
helix.cov.block(3, 3, 2, 2) = line.cov;
}
helix.q = circle.q;
helix.chi2_circle = circle.chi2;
helix.chi2_line = line.chi2;
return helix;