Variational Equations (C)
This example shows how to use first and second order variational equations. See also https://github.com/hannorein/rebound/blob/master/ipython_examples/VariationalEquations.ipynb and Rein and Tamayo (2016).
#include "rebound.h"
#include <stdio.h>
#include <stdlib.h>
// This function creates a simulation with one star, one planet and one test particle.
struct reb_simulation* create_sim(){
struct reb_simulation* r = reb_create_simulation();
r->integrator = REB_INTEGRATOR_IAS15; // First and second order variational equations supported in IAS15.
// r->integrator = REB_INTEGRATOR_BS; // First and second order variational equations supported in BS.
// r->integrator = REB_INTEGRATOR_WHFAST; Only first order variational equations supported in WHFast.
struct reb_particle star = {0.};
star.m = 1;
reb_add(r, star);
struct reb_particle planet = reb_tools_orbit_to_particle(1.,star,1e-3,1.,0.,0.,0.,0.,0.);
reb_add(r, planet);
struct reb_particle testparticle = reb_tools_orbit_to_particle(1.,star,0.,1.7,0.1,0.2,0.3,0.4,0.5);
reb_add(r, testparticle);
return r;
}
int main(int argc, char* argv[]) {
struct reb_simulation* r;
int var_i, var_ii;
// We first integrate the vanilla simulation forward in time and look at the position of the testparticle at the end of the simulation.
r = create_sim();
reb_integrate(r,100.);
printf("Position of testparticle at t=100: %.8f %.8f\n",r->particles[2].x,r->particles[2].y);
reb_free_simulation(r);
// Next, we shift the planet's initial x coordinate by a small amount and integrate the system again up til t=100.
double DeltaX = 0.001;
printf("\nShifting planet's x coordinate by %f.\n", DeltaX);
r = create_sim();
r->particles[1].x += DeltaX;
reb_integrate(r,100.);
printf("Position of testparticle at t=100 in shifted simulation: %.8f %.8f\n",r->particles[2].x,r->particles[2].y);
reb_free_simulation(r);
// Instead of shifting the initial x coordinate, we can also use variational equations.
r = create_sim();
var_i = reb_add_var_1st_order(r, -1); // The -1 means we vary a particle which is not a testparticle and therefore can influence other particles
// By default all components of variational particles are initialized to zero.
// We are interested in shifting the planet's x coordinates and thus initialize the x coordinate of the variational particle to 1.
r->particles[var_i+1].x = 1.;
reb_integrate(r,100.);
// After the integration ran, we can estimate where the test particle would have been had we shifted the inner planet's initial x coordinate.
printf("Position of testparticle at t=100 using 1st order var. eqs.: %.8f %.8f\n",r->particles[2].x+DeltaX*r->particles[var_i+2].x,r->particles[2].y+DeltaX*r->particles[var_i+2].y);
reb_free_simulation(r);
// Better yet, we can use second order variational particles.
r = create_sim();
var_i = reb_add_var_1st_order(r, -1);
var_ii = reb_add_var_2nd_order(r, -1, var_i, var_i);
r->particles[var_i+1].x = 1.;
reb_integrate(r,100.);
printf("Position of testparticle at t=100 using 2nd order var. eqs.: %.8f %.8f\n",r->particles[2].x+DeltaX*r->particles[var_i+2].x+DeltaX*DeltaX/2.*r->particles[var_ii+2].x,r->particles[2].y+DeltaX*r->particles[var_i+2].y+DeltaX*DeltaX/2.*r->particles[var_ii+2].y);
reb_free_simulation(r);
// We now do the same as above, but vary the testparticle's position
printf("\nShifting testparticle's x coordinate by %f.\n", DeltaX);
r = create_sim();
r->particles[2].x += DeltaX;
reb_integrate(r,100.);
printf("Position of testparticle at t=100 in shifted simulation: %.8f %.8f\n",r->particles[2].x,r->particles[2].y);
reb_free_simulation(r);
r = create_sim();
var_i = reb_add_var_1st_order(r, 2); // The 2 corresponds to the index of the testparticle that we vary.
r->particles[var_i].x = 1.;
reb_integrate(r,100.);
printf("Position of testparticle at t=100 using 1st order var. eqs.: %.8f %.8f\n",r->particles[2].x+DeltaX*r->particles[var_i].x,r->particles[2].y+DeltaX*r->particles[var_i].y);
reb_free_simulation(r);
r = create_sim();
var_i = reb_add_var_1st_order(r, 2);
var_ii = reb_add_var_2nd_order(r, 2, var_i, var_i);
r->particles[var_i].x = 1.;
reb_integrate(r,100.);
printf("Position of testparticle at t=100 using 2nd order var. eqs.: %.8f %.8f\n",r->particles[2].x+DeltaX*r->particles[var_i].x+DeltaX*DeltaX/2.*r->particles[var_ii].x,r->particles[2].y+DeltaX*r->particles[var_i].y+DeltaX*DeltaX/2.*r->particles[var_ii].y);
reb_free_simulation(r);
// Instead of varying cartesian coordinates, we can also vary orbital elements.
printf("\nShifting planet's semi-major axis by %f.\n", DeltaX);
r = create_sim();
r->particles[2] = reb_tools_orbit_to_particle(1.,r->particles[0],0.,1.7+DeltaX,0.1,0.2,0.3,0.4,0.5);
reb_integrate(r,100.);
printf("Position of testparticle at t=100 in shifted simulation: %.8f %.8f\n",r->particles[2].x,r->particles[2].y);
reb_free_simulation(r);
r = create_sim();
var_i = reb_add_var_1st_order(r, 2);
// The function that sets up the variational particle gets the same orbital parameters as the original particle.
r->particles[var_i] = reb_derivatives_a(1.,r->particles[0],r->particles[2]);
reb_integrate(r,100.);
printf("Position of testparticle at t=100 using 1st order var. eqs.: %.8f %.8f\n",r->particles[2].x+DeltaX*r->particles[var_i].x,r->particles[2].y+DeltaX*r->particles[var_i].y);
reb_free_simulation(r);
r = create_sim();
var_i = reb_add_var_1st_order(r, 2);
var_ii = reb_add_var_2nd_order(r, 2, var_i, var_i);
// first derivative with respect to a
r->particles[var_i] = reb_derivatives_a(1.,r->particles[0],r->particles[2]);
// second derivative with respect to a
r->particles[var_ii] = reb_derivatives_a_a(1.,r->particles[0],r->particles[2]);
reb_integrate(r,100.);
printf("Position of testparticle at t=100 using 2nd order var. eqs.: %.8f %.8f\n",r->particles[2].x+DeltaX*r->particles[var_i].x+DeltaX*DeltaX/2.*r->particles[var_ii].x,r->particles[2].y+DeltaX*r->particles[var_i].y+DeltaX*DeltaX/2.*r->particles[var_ii].y);
reb_free_simulation(r);
}
This example is located in the directory examples/variational_equations