libgyoto6-dev 1.2.0-4 / usr / include / x86_64-linux-gnu / Gyoto / GyotoStar.h

/**
 * \file GyotoStar.h
 * \brief Mass-less, spherical object following a timelike geodesic
 *
 *  A Gyoto::Star evolves in a Gyoto::Metric following time-like
 *  geodesics and is a Gyoto::Astrobj::Generic suitable for
 *  ray-tracing.
 */

/*
    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 __GyotoStar_H_ 
#define __GyotoStar_H_ 

namespace Gyoto{
  namespace Astrobj { class Star; }
}

#include <GyotoMetric.h>
#include <GyotoUniformSphere.h>
#include <GyotoSpectrum.h>
#include <GyotoWorldline.h>

#ifdef GYOTO_USE_XERCES
#include <GyotoRegister.h>
#endif

#include <string>

/**
 * \class Gyoto::Astrobj::Star
 * \brief Mass-less, spherical object following a timelike geodesic
 *
 * Gyoto can compute the Star's orbit in a Gyoto::Metric and perform
 * ray-tracing on this target. The XML description of a Star looks
 * like:
 * \code
 * <Astrobj kind = "Star">
 *   <Metric kind = "KerrBL">
 *     <Spin> 0. </Spin>
 *   </Metric>
 *   <Radius> 2. </Radius>
 *   <Velocity> 0. 0. 0.037037 </Velocity>
 *   <Position> 600. 9. 1.5707999999999999741 0 </Position>
 *   <Spectrum kind="BlackBody">
 *     <Temperature> 6000 </Temperature>
 *   </Spectrum>
 *   <Opacity kind="PowerLaw">
 *     <Exponent> 0 </Exponent>
 *     <Constant> 0.1 </Constant>
 *   </Opacity>
 *   <OpticallyThin/>
 * </Astrobj>
 * \endcode
 *
 * Star supports exactly the union of the parameters supported by
 * Gyoto::Astrobj::UniformSphere and Gyoto::Worldline.
 * 
 * The Metric element can be of any kind. This Metric sets the
 * coordinate system.
 *
 * The Star is a coordinate sphere of radius Radius in solid motion.
 *
 * Position sets the initial 4-coordinate of the centre of the
 * sphere. Velocity contains its initial 3-velocity (the time
 * derivatives of the 3 space coordinates).
 *
 * Like many Astrobj::Generic impementations, a Star can be
 * OpticallyThin or OpticallyThick.
 *
 * Spectrum and Opacity (if OpticallyThin) are the descriptions of two
 * Gyoto::Spectrum::Generic sub-classes.
 *
 */
class Gyoto::Astrobj::Star :
  public Gyoto::Astrobj::UniformSphere,
  public Gyoto::Worldline {
  friend class Gyoto::SmartPointer<Gyoto::Astrobj::Star>;
  
  // Data : 
  // -----

  // Constructors - Destructor
  // -------------------------
 public:
  GYOTO_OBJECT;

 /**
  * \brief Create Star object and set initial condition.
  * \param gg Gyoto::SmartPointer to the Gyoto::Metric in this part of the Universe
  * \param radius star radius
  * \param pos initial 4-position
  * \param v   initial 3-velocity
  */
  Star(SmartPointer<Metric::Generic> gg, double radius,
       double const pos[4], double const v[3]) ;

 /**
  * Create Star object with undefined initial conditions. One needs to
  * set the coordinate system, the metric, and the initial position
  * and velocity before integrating the orbit. setInititialCondition()
  * can be used for that.
  */
  Star(); ///< Default constructor
  
  Star(const Star& orig); ///< Copy constructor
  virtual Star * clone() const ;

  virtual ~Star() ;                        ///< Destructor
  
  // Accessors
  // ---------
 public:
  virtual std::string className() const ; ///< "Star"
  virtual std::string className_l() const ; ///< "star"

  virtual void metric(SmartPointer<Metric::Generic>);
  virtual SmartPointer<Metric::Generic> metric() const;

  /**
   * The mass of a Star is always 1. Stars do not perturb the
   * metric. The only relevant point is that Stars are massive
   * particules, their exact mass is of no importance.
   */
  virtual double getMass() const ; ///< Return 1.

 public:
  using UniformSphere::rMax;
  virtual double rMax() ;
  //  void setCoordSys(int); ///< Get coordinate system for integration
  //  int  getCoordSys(); ///< Set coordinate system for integration
  virtual void setInitialCondition(double const coord[8]); ///< Same as Worldline::setInitialCondition(gg, coord, sys,1)

 public:
  // Object / Property overloading for special needs:
  // Overload to interpret InitialCoordinate alias, and to interpret
  // Position/Velocity
  virtual int setParameter(std::string name,
			   std::string content,
			   std::string unit) ;
#ifdef GYOTO_USE_XERCES
  // Overload to 1- get metric first and 2- interpret Position/Velocity
  virtual void setParameters(FactoryMessenger *fmp) ;
  // Overload to dispatch InitCoord into Position and Velocity
  // for massive particle
  virtual void fillProperty(Gyoto::FactoryMessenger *fmp, Property const &p) const ;
#endif
  // Declare the wrappers around the Worldline accessors
  GYOTO_WORLDLINE;
  // Both base classes have deltaMax methods: we need to explicitly
  // use both
  using Gyoto::Worldline::deltaMax;
  using Gyoto::Astrobj::UniformSphere::deltaMax;

 public:
  
  /// Get the 6 Cartesian coordinates for specific dates.
  /**
   * This method is present in both the API of UniformSphere and
   * Worldline. It is pure virtual in UniformSphere. The Star
   * reimplementation is a trivial wrapper around
   * Worldline::getCartesian().
   */
  virtual void getCartesian(double const * const dates, size_t const n_dates,
		double * const x, double * const y,
		double * const z, double * const xprime=NULL,
		double * const yprime=NULL,  double * const zprime=NULL) ;
  virtual void getVelocity(double const pos[4], double vel[4]) ;

};


#endif