/usr/include/Gyoto/GyotoMetric.h is in libgyoto2-dev 0.2.3-1.
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* \file GyotoMetric.h
* \brief Base class for metric description
*
* Classes which represent a metric (e.g. Gyoto::Kerr) should inherit
* from Gyoto::Metric::Generic and implement all of the virtual
* methods plus at least one of the gmunu methods and one of the
* christoffel methods.
*
*/
/*
Copyright 2011, 2013 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 __GyotoMetric_H_
#define __GyotoMetric_H_
#include <iostream>
#include <fstream>
#include <string>
#include <GyotoSmartPointer.h>
#include <GyotoAstrobj.h>
#include <GyotoRegister.h>
#include <GyotoHooks.h>
#include <GyotoDefs.h>
namespace Gyoto {
namespace Metric {
class Generic;
/// A function to build instances of a specific Metric::Generic sub-class
/**
* This is a more specific version of the
* SmartPointee::Subcontractor_t type. A Metric::Subcontrator_t is
* called by the Gyoto::Factory to build an instance of the kind
* of metric specified in an XML file (see Register()). The
* Factory and Subcontractor_t function communicate through a
* Gyoto::FactoryMessenger.
*/
typedef SmartPointer<Metric::Generic> Subcontractor_t(FactoryMessenger*);
/**
* \brief Subcontractor template
*
* Instead of reimplementing the wheel, your subcontractor can simply be
* Gyoto::Metric::Subcontractor<MyKind>
*
* \tparam T Sub-class of Metric::Generic
*/
template<typename T> SmartPointer<Metric::Generic> Subcontractor
(FactoryMessenger* fmp) {
SmartPointer<T> gg = new T();
#ifdef GYOTO_USE_XERCES
gg -> setParameters(fmp);
#endif
return gg;
}
/// Query the Metric register
/**
* Query the Metric register to get the Metric::Subcontractor_t
* correspondig to a given kind name. This function is normally
* called only from the Factory.
*
* \param name e.g. "KerrBL"
* \param errmode int=0. If errmode==0, failure to find a
* registered Metric by that name is an error. Else, simply
* return NULL pointer in that case.
* \return pointer to the corresponding subcontractor.
*/
Gyoto::Metric::Subcontractor_t* getSubcontractor(std::string name,
int errmode=0);
/// The Metric register
/**
* Use the Metric::initRegister() once in your program to
* initiliaze it, the Metric::Register() function to fill it, and
* the Metric::getSubcontractor() function to query it.
*/
extern Register::Entry * Register_;
/// Make a Metric kind known to the Factory
/**
* Register a new Metric::Generic sub-class so that the
* Gyoto::Factory knows it.
*
* \param kind The kind name which identifies this object type in
* an XML file, as in <Metric kind="name">
*
* \param scp A pointer to the subcontractor, which will
* communicate whith the Gyoto::Factory to build an instance of
* the class from its XML description
*/
void Register(std::string kind, Gyoto::Metric::Subcontractor_t* scp);
/// Empty the Metric register.
/**
* This must be called once. It is called by
* Gyoto::Register::init().
*/
void initRegister();
}
/* Documented elswhere */
class Worldline;
}
/**
* \namespace Gyoto::Metric
* \brief Access to metrics
*
* Objects which describe space-time geometry must inherit from the
* Gyoto::Metric::Generic class.
*
* To be usable, a Metric::Generic sub-class should register a
* Metric::Subcontractor_t function using the Metric::Register()
* function. See also \ref writing_plugins_page .
*/
/**
* \class Gyoto::Metric::Generic
* \brief Base class for metrics
*
* Example: class Gyoto::Metric::KerrBL
*
* See Gyoto::Metric for an introduction.
*
*/
class Gyoto::Metric::Generic
: protected Gyoto::SmartPointee,
public Gyoto::Hook::Teller
{
friend class Gyoto::SmartPointer<Gyoto::Metric::Generic>;
private:
std::string kind_; ///< Metric kind name (e.g. "KerrBL")
double mass_; ///< Mass yielding geometrical unit (in kg).
int coordkind_; ///< Kind of coordinates (cartesian-like, spherical-like, unspecified)
protected:
double delta_min_; ///< Minimum integration step for the adaptive integrator
double delta_max_; ///< Maximum integration step for the adaptive integrator
/**
* \brief Numerical tuning parameter
*
* Ensure that delta (the numerical integration step) is never
* larger than a fraction of the distance between the current
* location and the center of the coordinate system.
*
* For investigations close to the event horizon, 0.5 is usually
* fine. If high accuracy is needed long after deflection (weak
* lensing), then this must be smaller. A good test is to look at a
* MinDistance map for a FixedStar: it must be smooth.
*/
double delta_max_over_r_;
bool keplerian_; ///< 1 if circularVelocity should return the Newtonian Keplerian velocity, in r^-3/2
protected:
/**
* \brief Set kind_
*
* kind(const std::string) is protected because, for most Metrics,
* it should not be changed in runtime.
*/
void kind(const std::string); ///< Set kind_
/**
* \brief Set coordkind_
*
* coordkind(int coordkind) is protected because, for most Metrics,
* it should not be changed in runtime.
*/
void coordKind(int coordkind); ///< Set coordinate kind
public:
const std::string kind() const; ///< Get kind_
int getRefCount();
// Constructors - Destructor
// -------------------------
Generic(const int coordkind, const std::string &name); ///< Constructor setting Generic::coordkind_ and kind_
virtual ~Generic() ; ///< Destructor
// Mutators / assignment
// ---------------------
virtual Generic * clone() const ; ///< Virtual copy constructor
void mass(const double); ///< Set mass used in unitLength()
void mass(const double, const std::string &unit); ///< Set mass used in unitLength()
// Accessors
int coordKind() const; ///< Get coordinate kind
double mass() const; ///< Get mass used in unitLength()
double mass(const std::string &unit) const; ///< Get mass used in unitLength()
/**
* Metrics implementations are free to express lengths and distances
* in whatever unit they see fit (presumably most often geometrical
* units). This function returns this unit in SI (meters).
*/
double unitLength() const ; ///< M * G / c^2, M is in kg, unitLength in meters
double unitLength(const std::string &unit) const ; ///< unitLength expressed in specified unit
/**
* Get delta_min_
*/
double deltaMin() const;
/**
* Set delta_min_
*/
void deltaMin(double h1);
/**
* Get delta_max_
*/
double deltaMax() const;
/**
* Get delta max at a given position
*
* \param pos 4-position
* \param[optional] delta_max_external external constraint on delta_max
* \return the smallest value between delta_max_,
* delta_max_external, and R*delta_max_over_r_ where R is pos[1] in
* spherical coordinates and max(x1, x2, x3) in Cartesian
* coordinates.
*/
virtual double deltaMax(double const pos[8], double delta_max_external) const;
/**
* Set delta_max_
*/
void deltaMax(double h1);
double deltaMaxOverR() const; ///< Get delta_max_over_r_
void deltaMaxOverR(double t); ///< Set delta_max_over_r_
bool keplerian() const; ///< Get keplerian_
void keplerian(bool); ///< Set keplerian_
virtual void cartesianVelocity(double const coord[8], double vel[3]);
///< Compute xprime, yprime and zprime from 8-coordinates
/**
* \param coord 4-position (geometrical units);
* \param v 3-velocity dx1/dx0, dx2/dx0, dx3/dx0;
* \return tdot = dx0/dtau.
*/
virtual double SysPrimeToTdot(const double coord[4], const double v[3]) const;
///<Compute tdot as a function of dr/dt, dtheta/dt and dphi/dt. Everything is in geometrical units.
/**
* \brief Yield circular velocity at a given position
*
* Give the velocity of a massive particle in circular orbit at the
* given position projected onto the equatorial plane. Such a
* velocity may not exist everywhere (or anywhere) for a given
* metric. This method is intended to be used by Astrobj classes
* such as Torus or ThinDisk.
*
* If keplerian_ is set to true, this method should return the
* Keplerian velcity instead (derived classes should ensure this,
* see KerrBL::circularVelocity() for instance).
*
* The default implementation throws an error if keplerian_ is set
* to false.
*
* \param pos input: position,
* \param vel output: velocity,
* \param dir 1 for corotating, -1 for counterrotating.
*/
virtual void circularVelocity(double const pos[4], double vel[4],
double dir=1.) const ;
/**
* Set coord[4] so that the 4-velocity coord[4:7] is lightlike,
* i.e. of norm 0. There may be up to two solutions. coord[4] is set
* to the hightest. The lowest can be retrieved using
* nullifyCoord(double coord[8], double& tdot2) const. Everything is
* expressed in geometrical units.
*
* \param[in,out] coord 8-position, coord[4] will be set according
* to the other elements;
*/
virtual void nullifyCoord(double coord[8]) const;
///< Set tdot (coord[4]) such that coord is light-like. Everything is in geometrical units.
/**
* Set coord[4] so that the 4-velocity coord[4:7] is lightlike,
* i.e. of norm 0. There may be up to two solutions. coord[4] is set
* to the hightest. The lowest can be retrieved in tdot2. Everything
* is expressed in geometrical units.
*
* \param[in,out] coord 8-position, coord[4] will be set according
* to the other elements;
* \param[out] tdot2 will be set to the smallest solution
*/
virtual void nullifyCoord(double coord[8], double& tdot2) const;
///< Set tdot (coord[4]) such that coord is light-like and return other possible tdot
/**
* Compute the scalarproduct of the two quadrivectors u1 and u2 in
* this Metric, at point pos expressed in coordinate system sys.
* \param pos 4-position;
* \param u1 1st quadrivector;
* \param u2 2nd quadrivector;
* \return u1*u2
*/
virtual double ScalarProd(const double pos[4],
const double u1[4], const double u2[4]) const; ///< Scalar product
virtual double Norm3D(double* pos) const; ///< not clear
/**
* \brief Set parameter by name
*
* Assume MyKind is a subclass of Metric::Generic which has two
* members (a string StringMember and a double DoubleMember):
\code
int MyKind::setParameter(std::string name, std::string content, std::string unit) {
if (name=="StringMember") setStringMember(content);
else if (name=="DoubleMember") setDoubleMemeber(atof(content.c_str()), unit);
else return Generic::setParameter(name, content, unit);
return 0;
}
\endcode
* If MyKind is not a direct subclass of Generic, it should call the
* corresponding setParameter() implementation instead of
* Generic::setParameter().
*
* \param name XML name of the parameter
* \param content string representation of the value
* \param unit string representation of the unit
* \return 0 if this parameter is known, 1 if it is not.
*/
virtual void setParameter(std::string name,
std::string content,
std::string unit);
// Outputs
#ifdef GYOTO_USE_XERCES
/**
* \brief Main loop in Subcontractor_t function
*
* The Subcontractor_t function for each Metric kind should look
* somewhat like this (templated as
* Gyoto::Metric::Subcontractor<MyKind>):
\code
SmartPointer<Metric::Generic>
Gyoto::Metric::MyKind::Subcontractor(FactoryMessenger* fmp) {
SmartPointer<MyKind> gg = new MyKind();
gg -> setParameters(fmp);
return gg;
}
\endcode
*
* Each metric kind should implement setParameter(string name,
* string content, string unit) to interpret the individual XML
* elements. setParameters() can be overloaded in case the specific
* Metric class needs low level access to the FactoryMessenger. See
* Gyoto::Astrobj::UniformSphere::setParameters().
*/
virtual void setParameters(Gyoto::FactoryMessenger *fmp) ;
/**
* Metrics implementations should impement fillElement to save their
* parameters to XML and call the Metric::fillElement(fmp) for the
* shared properties
*/
virtual void fillElement(FactoryMessenger *fmp) ; ///< called from Factory
/**
* \brief Process generic XML parameters
*/
void processGenericParameters(Gyoto::FactoryMessenger *fmp) ;
#endif
/**
* \brief Metric coefficients
*
* The default implementation calls Metric:: gmunu(double g[4][4], const double * pos) const
*
* \param x 4-position at which to compute the coefficient;
* \param mu 1st index of coefficient, 0≤μ≤3;
* \param nu 2nd index of coefficient, 0≤ν≤3;
* \return Metric coefficient g<SUB>μ,ν</SUB> at point x
*/
virtual double gmunu(const double * x, int mu, int nu) const;
/**
* \brief Metric coefficients
*
* The default implementation calls double gmunu(const double * x, int mu, int nu) const.
*
* \param[out] g 4x4 array to store the coeefficients
* \param[in] x 4-position at which to compute the coefficients;
* \return Metric coefficient g<SUB>μ,ν</SUB> at point x
*/
virtual void gmunu(double g[4][4], const double * pos) const;
/**
* \brief Chistoffel symbol
*
* Value of Christoffel symbol
* Γ<SUP>α</SUP><SUB>μν</SUB> at point
* (x<SUB>1</SUB>, x<SUB>2</SUB>, x<SUB>3</SUB>).
*/
virtual double christoffel(const double coord[8],
const int alpha, const int mu, const int nu) const;
/**
* \brief Chistoffel symbol
*
* Value of Christoffel symbol
* Γ<SUP>α</SUP><SUB>μν</SUB> at point
* (x<SUB>1</SUB>, x<SUB>2</SUB>, x<SUB>3</SUB>).
*/
virtual int christoffel(double dst[4][4][4], const double coord[8]) const ;
/**
* \brief RK4 integrator
*/
virtual int myrk4(Worldline * line, const double coord[8], double h, double res[8]) const;
/**
* \brief RK4 integrator with adaptive step
*/
virtual int myrk4_adaptive(Gyoto::Worldline* line, const double coord[8],
double lastnorm, double normref,
double coordnew[8], double h0, double& h1,
double deltamax=GYOTO_DEFAULT_DELTA_MAX) const;
/**
* \brief Check whether integration should stop
*
* The integrating loop will ask this the Metric through this method
* whether or not it is happy to conitnue the integration.
* Typically, the Metric should answer 0 when everything is fine, 1
* when too close to the event horizon, inside the BH...
*
* \param coord 8-coordinate vector to check.
*/
virtual int isStopCondition(double const * const coord) const;
/**
* \brief F function such as dy/dtau=F(y,cst)
*/
virtual int diff(const double y[8], double res[8]) const ;
/**
* \brief Set Metric-specific constants of motion. Used e.g. in KerrBL.
*/
virtual void setParticleProperties(Gyoto::Worldline* line,
const double * coord) const;
};
#endif
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