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Ray.ipp
Go to the documentation of this file. Or view the newest version in sPHENIX GitHub for file Ray.ipp
1 // This file is part of the Acts project.
2 //
3 // Copyright (C) 2018-2019 CERN for the benefit of the Acts project
4 //
5 // This Source Code Form is subject to the terms of the Mozilla Public
6 // License, v. 2.0. If a copy of the MPL was not distributed with this
7 // file, You can obtain one at http://mozilla.org/MPL/2.0/.
8 
10 
11 template <typename value_t, size_t DIM>
13  : m_origin(origin), m_dir(dir.normalized()), m_idir(1 / m_dir.array()) {}
14 template <typename value_t, size_t DIM>
15 std::ostream& Acts::Ray<value_t, DIM>::toStream(std::ostream& os) const {
16  os << "Ray(";
17  for (size_t i = 0; i < DIM; i++) {
18  if (i > 0) {
19  os << ", ";
20  }
21  os << m_origin[i];
22  }
23  os << " -> ";
24  for (size_t i = 0; i < DIM; i++) {
25  if (i > 0) {
26  os << ", ";
27  }
28  os << m_dir[i];
29  }
30  os << ")";
31 
32  return os;
33 }
34 
35 template <typename value_t, size_t DIM>
37  const transform_type& trf) const {
38  return Ray<value_t, DIM>(trf * m_origin, trf.rotation() * m_dir);
39 }
40 
41 template <typename value_t, size_t DIM>
42 template <size_t D, std::enable_if_t<D == 3, int>>
44  value_type far_distance) const {
45  static_assert(DIM == 3, "OBJ is only supported in 3D");
46 
47  helper.line(m_origin, (m_origin + m_dir * far_distance).eval());
48 }
49 
50 template <typename U, size_t V>
51 std::ostream& operator<<(std::ostream& os, const Acts::Ray<U, V>& ray) {
52  ray.dump(os);
53  return os;
54 }