/usr/include/x86_64-linux-gnu/Gyoto/GyotoKerrBL.h is in libgyoto6-dev 1.2.0-4.
This file is owned by root:root, with mode 0o644.
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1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 | /**
* \file GyotoKerrBL.h
* \brief KerrBL metric
*
*/
/*
Copyright 2011 Frederic Vincent, Thibaut Paumard
This file is part of Gyoto.
Gyoto 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.
Gyoto 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 Gyoto. If not, see <http://www.gnu.org/licenses/>.
*/
#ifndef __GyotoKerrBL_H_
#define __GyotoKerrBL_H_
namespace Gyoto {
namespace Metric { class KerrBL; }
}
#include <GyotoMetric.h>
#include <GyotoWorldline.h>
#ifdef GYOTO_USE_XERCES
#include <GyotoRegister.h>
#endif
/// Default value for difftol_
#define GYOTO_KERRBL_DEFAULT_DIFFTOL 1e-2
/**
* \class Gyoto::Metric::KerrBL
* \brief Metric around a Kerr black-hole in Boyer-Lindquist coordinates
*/
class Gyoto::Metric::KerrBL : public Metric::Generic {
friend class Gyoto::SmartPointer<Gyoto::Metric::KerrBL>;
// Data :
// -----
protected:
double spin_ ; ///< Angular momentum parameter
double a2_ ; ///< spin_*spin_
double a3_ ; ///< a2_*spin_
double a4_ ; ///< a2_*a2_
/// Numerical tuning parameter
/**
* Small values yield more accurate integration at the expanse of
* computing time.
*/
double difftol_;
double rsink_; ///< numerical horizon
double drhor_; ///< horizon security
bool generic_integrator_; ///< which integrator to use
// Constructors - Destructor
// -------------------------
public:
GYOTO_OBJECT;
KerrBL(); ///< Default constructor
virtual KerrBL * clone () const ;
// Accessors
// ---------
public:
void spin(const double spin); ///< Set spin
double spin() const ; ///< Returns spin
double difftol() const; ///< Get difftol_
void difftol(double t); ///< Set difftol_
void horizonSecurity(double drhor);
double horizonSecurity() const;
void genericIntegrator(bool);
bool genericIntegrator() const ;
virtual double getRms() const;
virtual double getRmb() const;
virtual double getSpecificAngularMomentum(double rr) const;
virtual double getPotential(double const pos[4], double l_cst) const;
void gmunu(double g[4][4], const double * pos) const ;
double gmunu(const double * const x, int mu, int nu) const ;
/**
* \brief g<SUP>μ,ν</SUP>
*/
void gmunu_up(double gup[4][4], const double * pos) const ;
double gmunu_up(const double * const x, int mu, int nu) const ;
using Generic::christoffel;
int christoffel(double dst[4][4][4], const double pos[4]) const ;
double ScalarProd(const double pos[4],
const double u1[4], const double u2[4]) const ;
void nullifyCoord(double coord[8], double & tdot2) const;
void nullifyCoord(double coord[8]) const;
// friend std::ostream& operator<<(std::ostream& , const KerrBL& ) ;
// std::ostream& print(std::ostream&) const ;
virtual void circularVelocity(double const pos[4], double vel [4],
double dir=1.) const ;
public:
virtual void MakeCoord(const double coordin[8], const double cst[5], double coordout[8]) const ;
///< Inverse function of MakeMomentumAndCst
///< Computes pr, ptheta, E and L from rdot, thetadot, phidot, tdot
void MakeMomentum(const double coordin[8], const double cst[5], double coordout[8]) const;
///< Transforms from Boyer-Lindquist coordinates [t,r,th,phi,tdot,rdot,thdot,phidot] to [t,r,th,phi,pt,pr,pth,pphi] where pt,pr... are generalized momenta.
protected:
// outside the API
/* RK4 : y=[r,theta,phi,t,pr,ptheta],
cst=[a,E,L,Q,1/Q],dy/dtau=F(y,cst), h=proper time step.
For KerrBL geodesic computation.
*/
int myrk4(Worldline * line, const double coordin[8], double h, double res[8]) const; //external-use RK4
public:
int myrk4(const double coor[8], const double cst[5], double h, double res[8]) const;///< Internal-use RK4 proxy
int myrk4_adaptive(Gyoto::Worldline* line, const double coor[8], double lastnorm, double normref, double coor1[8], double h0, double& h1, double h1max=GYOTO_DEFAULT_DELTA_MAX) const; ///< Internal-use adaptive RK4 proxy
/**
* \brief Ensure conservation of the constants of motion
*
* Tweak thetadot if necessary.
*/
private:
int CheckCons(const double coor_init[8], const double cst[5], double coor_fin[8]) const;
/**
* \brief Normalize 4-velocity
*
* To 0 or -1. Changes rdot to allow norm conservation.
*/
void Normalize4v(double coord[8], const double part_mass) const;
public:
/** F function such as dy/dtau=F(y,cst)
*/
using Metric::Generic::diff;
private:
/**
* \brief Used in RK4 proxies.
*/
virtual int diff(const double y[8], const double cst[5],
double res[8]) const ;
/** Integrator. Computes the evolution of y (initcond=y(0)).
*/
virtual void computeCst(const double coord[8], double cst[5]) const;
public:
void setParticleProperties(Worldline* line, const double* coord) const;
virtual int isStopCondition(double const * const coord) const;
void observerTetrad(std::string const obskind,
double const pos[4], double fourvel[4],
double screen1[4], double screen2[4],
double screen3[4]) const;
};
#endif
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