star_bin_kinema_xcts.C

/*
 * Method Star_bin_xcts::kinematics
 * (see file star.h for documentation)
 */
 
/*
 *   Copyright (c) 2010 Michal Bejger
 *
 *   This file is part of LORENE.
 *
 *   LORENE is free software; you can redistribute it and/or modify
 *   it under the terms of the GNU General Public License version 2
 *   as published by the Free Software Foundation.
 *
 *   LORENE 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 LORENE; if not, write to the Free Software
 *   Foundation, Inc., 59 Temple Place, Suite 330, Boston, MA  02111-1307  USA
 *
 */
 
char star_bin_kinema_xcts_C[] = "$Header: /cvsroot/Lorene/C++/Source/Star/star_bin_kinema_xcts.C,v 1.6 2014/10/13 08:53:38 j_novak Exp $" ;
 
/*
 * $Id: star_bin_kinema_xcts.C,v 1.6 2014/10/13 08:53:38 j_novak Exp $
 * $Log: star_bin_kinema_xcts.C,v $
 * Revision 1.6  2014/10/13 08:53:38  j_novak
 * Lorene classes and functions now belong to the namespace Lorene.
 *
 * Revision 1.5  2014/10/06 15:13:17  j_novak
 * Modified #include directives to use c++ syntax.
 *
 * Revision 1.4  2010/12/09 10:43:53  m_bejger
 * Small changes, annule --> annule_domain
 *
 * Revision 1.3  2010/10/26 19:57:02  m_bejger
 * Various cleanups
 *
 * Revision 1.2  2010/06/04 19:57:52  m_bejger
 * Added condition for mp.get_rot_phi
 *
 * Revision 1.1  2010/05/04 07:51:05  m_bejger
 * Initial version
 *
 * $Header: /cvsroot/Lorene/C++/Source/Star/star_bin_kinema_xcts.C,v 1.6 2014/10/13 08:53:38 j_novak Exp $
 *
 */
 
#include <cmath>
 
// Headers Lorene
#include "star.h"
 
namespace Lorene {
void Star_bin_xcts::kinematics(double omega, double x_axe) {
 
    int nzm1 = mp.get_mg()->get_nzone() - 1 ;
 
    // --------------------
    // Computation of B^i/N
    // --------------------
 
    //  1/ Computation of omega m^i
 
    const Coord& xa = mp.xa ;
    const Coord& ya = mp.ya ;
 
    bsn.change_triad(mp.get_bvect_cart()) ;
 
      if (fabs(mp.get_rot_phi()) < 1e-10) {
 
        bsn.set(1) = - omega * ya ;
        bsn.set(2) = omega * (xa - x_axe) ;
        bsn.set(3) = 0 ;
 
        } else {
 
        bsn.set(1) = omega * ya ;
        bsn.set(2) = - omega * (xa - x_axe) ;
        bsn.set(3) = 0 ;
 
    }
 
    bsn.annule_domain(nzm1) ;   // set to zero in the ZEC
 
    // Addition of beta and division by lapse
    // Eq. 47 from Gourgoulhon et al. (2001)
    // New convention : l = Nn + B ==> B = \beta + \Omega d\phi
    //---------------------------------------------------------
 
    bsn = ( bsn + beta ) / nn ;
 
    bsn.annule_domain(nzm1) ;   // set to zero in the ZEC
    bsn.std_spectral_base() ;
 
    //----------------------
    // Centrifugal potential
    //----------------------
 
    // Lorentz factor between the co-orbiting observer
    // and the Eulerian one
    // Eq. 23 from Gourgoulhon et al. (2001)
 
    Sym_tensor gamma_cov (gamma.cov()) ;
    gamma_cov.change_triad(mp.get_bvect_cart()) ;
 
    Scalar gam0 = 1 / sqrt(1 - contract(gamma_cov, 0, 1, bsn * bsn, 0, 1)) ;
    pot_centri = - log( gam0 ) ;
 
    pot_centri.annule_domain(nzm1) ;    // set to zero in the external domain
    pot_centri.std_spectral_base() ;    // set the bases for spectral expansions
 
      // The derived quantities are obsolete
      // -----------------------------------
 
      del_deriv() ;
 
}
}