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ex20.cpp
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ex20.cpp
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// MFEM Example 20
//
// Compile with: make ex20
//
// Sample runs: ex20
// ex20 -p 1 -o 1 -n 120 -dt 0.1
// ex20 -p 1 -o 2 -n 60 -dt 0.2
// ex20 -p 1 -o 3 -n 40 -dt 0.3
// ex20 -p 1 -o 4 -n 30 -dt 0.4
//
// Description: This example demonstrates the use of the variable order,
// symplectic ODE integration algorithm. Symplectic integration
// algorithms are designed to conserve energy when integrating, in
// time, systems of ODEs which are derived from Hamiltonian
// systems.
//
// Hamiltonian systems define the energy of a system as a function
// of time (t), a set of generalized coordinates (q), and their
// corresponding generalized momenta (p).
//
// H(q,p,t) = T(p) + V(q,t)
//
// Hamilton's equations then specify how q and p evolve in time:
//
// dq/dt = dH/dp
// dp/dt = -dH/dq
//
// To use the symplectic integration classes we need to define an
// mfem::Operator P which evaluates the action of dH/dp, and an
// mfem::TimeDependentOperator F which computes -dH/dq.
//
// This example offers five simple 1D Hamiltonians:
// 0) Simple Harmonic Oscillator (mass on a spring)
// H = ( p^2 / m + q^2 / k ) / 2
// 1) Pendulum
// H = ( p^2 / m - k ( 1 - cos(q) ) ) / 2
// 2) Gaussian Potential Well
// H = ( p^2 / m ) / 2 - k exp(-q^2 / 2)
// 3) Quartic Potential
// H = ( p^2 / m + k ( 1 + q^2 ) q^2 ) / 2
// 4) Negative Quartic Potential
// H = ( p^2 / m + k ( 1 - q^2 /8 ) q^2 ) / 2
//
// In all cases these Hamiltonians are shifted by constant values
// so that the energy will remain positive. The mean and standard
// deviation of the computed energies at each time step are
// displayed upon completion.
//
// We then use GLVis to visualize the results in a non-standard way
// by defining the axes to be q, p, and t rather than x, y, and z.
// In this space we build a ribbon-like mesh with nodes at (0,0,t)
// and (q,p,t). Finally we plot the energy as a function of time
// as a scalar field on this ribbon-like mesh.
//
// For a more traditional plot of the results, including q, p, and
// H, can be obtained by selecting the "-gp" option. This creates
// a data file and input deck for the GnuPlot application (not
// included with MFEM). To visualize these results on most Linux
// systems type the command "gnuplot gnuplot_ex20.inp". The data
// file, named "ex20.dat", should be simple enough to display with
// other plotting programs as well.
#include "mfem.hpp"
#include <fstream>
#include <iostream>
using namespace std;
using namespace mfem;
// Constants used in the Hamiltonian
static int prob_ = 0;
static double m_ = 1.0;
static double k_ = 1.0;
// Hamiltonian functional, see below for implementation
double hamiltonian(double q, double p, double t);
class GradT : public Operator
{
public:
GradT() : Operator(1) {}
void Mult(const Vector &x, Vector &y) const { y.Set(1.0/m_, x); }
};
class NegGradV : public TimeDependentOperator
{
public:
NegGradV() : TimeDependentOperator(1) {}
void Mult(const Vector &x, Vector &y) const;
};
int main(int argc, char *argv[])
{
// 1. Parse command-line options.
int order = 1;
int nsteps = 100;
double dt = 0.1;
bool visualization = true;
bool gnuplot = false;
OptionsParser args(argc, argv);
args.AddOption(&order, "-o", "--order",
"Time integration order.");
args.AddOption(&prob_, "-p", "--problem-type",
"Problem Type:\n"
"\t 0 - Simple Harmonic Oscillator\n"
"\t 1 - Pendulum\n"
"\t 2 - Gaussian Potential Well\n"
"\t 3 - Quartic Potential\n"
"\t 4 - Negative Quartic Potential");
args.AddOption(&nsteps, "-n", "--number-of-steps",
"Number of time steps.");
args.AddOption(&dt, "-dt", "--time-step",
"Time step size.");
args.AddOption(&m_, "-m", "--mass",
"Mass.");
args.AddOption(&k_, "-k", "--spring-const",
"Spring constant.");
args.AddOption(&visualization, "-vis", "--visualization", "-no-vis",
"--no-visualization",
"Enable or disable GLVis visualization.");
args.AddOption(&gnuplot, "-gp", "--gnuplot", "-no-gp", "--no-gnuplot",
"Enable or disable GnuPlot visualization.");
args.Parse();
if (!args.Good())
{
args.PrintUsage(cout);
return 1;
}
args.PrintOptions(cout);
// 2. Create and Initialize the Symplectic Integration Solver
SIAVSolver siaSolver(order);
GradT P;
NegGradV F;
siaSolver.Init(P,F);
// 3. Set the initial conditions
double t = 0.0;
Vector q(1), p(1);
Vector e(nsteps+1);
q(0) = 0.0;
p(0) = 1.0;
// 4. Prepare GnuPlot output file if needed
ofstream ofs;
if (gnuplot)
{
ofs.open("ex20.dat");
ofs << t << "\t" << q(0) << "\t" << p(0) << endl;
}
// 5. Create a Mesh for visualization in phase space
int nverts = (visualization) ? 2*(nsteps+1) : 0;
int nelems = (visualization) ? nsteps : 0;
Mesh mesh(2, nverts, nelems, 0, 3);
int v[4];
Vector x0(3); x0 = 0.0;
Vector x1(3); x1 = 0.0;
// 6. Perform time-stepping
double e_mean = 0.0;
for (int i = 0; i < nsteps; i++)
{
// 6a. Record initial state
if (i == 0)
{
e[0] = hamiltonian(q(0),p(0),t);
e_mean += e[0];
if (visualization)
{
x1[0] = q(0);
x1[1] = p(0);
x1[2] = 0.0;
mesh.AddVertex(x0);
mesh.AddVertex(x1);
}
}
// 6b. Advance the state of the system
siaSolver.Step(q,p,t,dt);
e[i+1] = hamiltonian(q(0),p(0),t);
e_mean += e[i+1];
// 6c. Record the state of the system
if (gnuplot)
{
ofs << t << "\t" << q(0) << "\t" << p(0) << "\t" << e[i+1] << endl;
}
// 6d. Add results to GLVis visualization
if (visualization)
{
x0[2] = t;
x1[0] = q(0);
x1[1] = p(0);
x1[2] = t;
mesh.AddVertex(x0);
mesh.AddVertex(x1);
v[0] = 2*i;
v[1] = 2*(i+1);
v[2] = 2*(i+1)+1;
v[3] = 2*i+1;
mesh.AddQuad(v);
}
}
// 7. Compute and display mean and standard deviation of the energy
e_mean /= (nsteps + 1);
double e_var = 0.0;
for (int i=0; i<=nsteps; i++)
{
e_var += pow(e[i] - e_mean, 2);
}
e_var /= (nsteps + 1);
double e_sd = sqrt(e_var);
cout << endl << "Mean and standard deviation of the energy" << endl;
cout << e_mean << "\t" << e_sd << endl;
// 8. Finalize the GnuPlot output
if (gnuplot)
{
ofs.close();
ofs.open("gnuplot_ex20.inp");
ofs << "plot 'ex20.dat' using 1:2 w l t 'q', "
<< "'ex20.dat' using 1:3 w l t 'p', "
<< "'ex20.dat' using 1:4 w l t 'H'" << endl;
ofs.close();
}
// 9. Finalize the GLVis output
if (visualization)
{
mesh.FinalizeQuadMesh(1);
H1_FECollection fec(order = 1, 2);
FiniteElementSpace fespace(&mesh, &fec);
GridFunction energy(&fespace);
energy = 0.0;
for (int i = 0; i <= nsteps; i++)
{
energy[2*i+0] = e[i];
energy[2*i+1] = e[i];
}
char vishost[] = "localhost";
int visport = 19916;
socketstream sock(vishost, visport);
sock.precision(8);
sock << "solution\n" << mesh << energy
<< "window_title 'Energy in Phase Space'\n"
<< "keys\n maac\n" << "axis_labels 'q' 'p' 't'\n"<< flush;
}
}
double hamiltonian(double q, double p, double t)
{
double h = 1.0 - 0.5 / m_ + 0.5 * p * p / m_;
switch (prob_)
{
case 1:
h += k_ * (1.0 - cos(q));
break;
case 2:
h += k_ * (1.0 - exp(-0.5 * q * q));
break;
case 3:
h += 0.5 * k_ * (1.0 + q * q) * q * q;
break;
case 4:
h += 0.5 * k_ * (1.0 - 0.125 * q * q) * q * q;
break;
default:
h += 0.5 * k_ * q * q;
break;
}
return h;
}
void NegGradV::Mult(const Vector &x, Vector &y) const
{
switch (prob_)
{
case 1:
y(0) = - k_* sin(x(0));
break;
case 2:
y(0) = - k_ * x(0) * exp(-0.5 * x(0) * x(0));
break;
case 3:
y(0) = - k_ * (1.0 + 2.0 * x(0) * x(0)) * x(0);
break;
case 4:
y(0) = - k_ * (1.0 - 0.25 * x(0) * x(0)) * x(0);
break;
default:
y(0) = - k_ * x(0);
break;
};
}