How can I normalize a function solved numerically?

I'm trying to make the pdf of a quantum harmonic oscillator, once the equation is solved numerically, the pdf area should be 1 but instead it is 2.2604e-28. Thanks for advanced
function test(n,y0,dy0)
syms y(x)
m=9.1093821545*1e-31; k=m*(4.57*1e14)^2; w=sqrt(k/m); hb=(6.6260695729*1e-34)/(2*pi); En=hb*w*(n+.5); c1=-2*m/(hb^2); c_i0=sqrt(hb/(m*w));
[V] = odeToVectorField(diff(y,x,2) == c1*(En-.5*k*x.^2).*y);
x1=0;
x2=2e-9;
M = matlabFunction(V,'vars',{'x','Y'});
[p,q]= ode45(M,[x1 x2],[y0 dy0]);
dens=(q(:,1).*q(:,1));
% A plotear
plot([-p p],En+dens,'-k') %psi quadrat
%plot(-p,En+q(:,1),'-k') psi
hold on
%plot(p,En+q(:,1),'-k') psi
potencial=0.5*k*p.^2;
plot([-p p],potencial,'-r') %potencial
plot([-p p], ones(1,length(p))*En,'-b') %En
% natural frequency of the oscillator w = 4.57e14 Hz
hold off
grid on
u=zeros(1,length(dens));
2*trapz(p,dens) %area of the pdf
end

6 Comments

What are typical values for ‘n’, ‘y0’, and ‘dy0’ ?
they're initial conditions, i.e: 0,5.0331e-10,0
Instead of doing the trapz for dens over time, you could add another variable to the ode which is V(1).^2 . The output at the corresponding position would automatically be the integral of that value.
thanks! but do you know if there's some method to normalize the function numerically? or it can only be done analytically?
Walter means that you should add the equation
dy(3)/dt = y(1)^2
to your system of ordinary differential equations, integrate numerically and afterwards normalize y(1) according to
dense=dense/q(end,3).
Best wishes
Torsten.

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 Accepted Answer

Hi david,
A normalization integral that small shows that the scaling could be improved upon, but as a workaround is this what you are looking for?
densnorm = dens/(2*trapz(p,dens));
2*trapz(p,densnorm) %area of the pdf
ans = 1

3 Comments

thanks David! the plot would be this one right?
plot([-p p],densnorm)
yes, that's the new one to use. Maybe I should have just said dens = dens / (2*trapz(p,dens)) but I wanted to emphasize normalization.
Incidentally, if you go to rescaled units for x as you almost did, then things are easier:
xs = sqrt(hb/(m*w)) length scale, same as your c_i0
Es = hb*w energy scale
Fn = En/Es = n+1/2 normalized energy
u = x/xs normalized x
In that case all the constants disappear from the differential equation, leaving just the factors of 1/2 and you can solve
[V] = odeToVectorField( (-1/2)*diff(y,u,2) == (Fn-(1/2)*u.^2).*y );
The integration limits on u are something like 0 to 10.
To normalize the resulting density with the new p array (which represents u) you do exactly like before, dens = dens / (2*trapz(p,dens)). It's easier to do plots since now the potential energy is (1/2)*p.^2 and fits on the plot without rescaling.
Then if you want to get the real distances back again, since p means u right now, you would use x = p*xs as the new variable. If you wanted a normalized density in terms of x you would invoke (guess what) dens = dens / (2*trapz(x,dens)).
thank you! I'm definitely trying your method

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