I have a mathematical model of differential equations that begins as linear and then uses correctional coefficients after reaching a certain value (1).
Currently, I solve the linear function independently, find out where the array goes from less than 1 to greater than 1, and then use that value from the array as the new initial condition. I also correct the time scale.
def vttmodel_linear(m,t,tm,tv,M_max):
n = 1/(7*tm)
dMdt = n
return dMdt
M_0 = 0
M_max = 1 + 7*((RH_crit-RH)/(RH_crit-100)) - 2*np.square((RH_crit-RH)/(RH_crit-100))
print(M_max)
# tm = days
# M = weeks so 7*tm
t = np.arange(0,104+1)
tm = np.exp(-0.68*np.log(T) - 13.9*np.log(RH) + 0.14*W - 0.33*SQ + 66.02)
tv = np.exp(-0.74*np.log(T) - 12.72*np.log(RH) + 0.06*W + 61.50)
m = odient(vttmodel_linear, M_0, t, args=(tm,tv,M_max))
M_0 = m[(np.where(m>1)[0][0])-1]
t = np.where(m>1)[0]
Then I use the new initial condition, M_0 and the updated time scale to solve the non-linear portion of the model.
def vttmodel(M,t,tm,tv,M_max):
n = 1/(7*tm)
k1 = 2/((tv/tm)-1)
k2 = np.max([1-np.exp(2.3*(M-M_max)), 0])
dMdt = n*k1*k2
return dMdt
M = odient(vttmodel, M_0, t, args=(tm,tv,M_max))
I then splice the arrays m and M at the location I found earlier and graph the result.
I would like to find a simplified way to do this. I have tried using If statements within the odient function and also a While loop when calling the two functions, but have not had any luck interrupting the odient function. Suggestions would be helpful. Thank you.
Related
I am trying to calculate the second-order autocorrelation function
g(lag) = < P2 (m(t) . m(t+lag)) >
for a given numpy array m where P2 is the second-order Legendre polynomial P2(x) = 0.5 * (3*x**2-1). The average is calculated over all initial points t for all possible lag times lag.
I have written a simple function to calculate this function g(lag)
def calc_tau_fast_build(vector):
maxLag = numpy.int(np.floor(len(vector)/2))
g = numpy.zeros((maxLag));
for tau in range(0, maxLag):
w = 0;
tmp = 0;
for t in range(0, len(vector) - tau):
theta = vector[t] * vector[tau + t]
tmp = tmp + 0.5*(3*theta**2-1)
w = w + 1
g[tau] = tmp/w
return g
This works just fine, however for large inputs the performance is rather poor.
I would like to replace the entire function with numpy.correlate if possible. In fact, without the P2 = 0.5*(3*theta**2-1) part, I can get the same results, upto a normalization constant, with
res = numpy.correlate(vector,vector,mode='full')
res[numpy.int(res.size/2):]
I basically couldn't think of a way to incorporate the P2 function into the numpy.correlate without playing around with the numpy source code. Could anyone please suggest a way to use numpy.correlate in this context?
I am developing a code that uses a method called Platen to solve stochastic differential equations. Then I must solve that stochastic differential equation many times (on the order of 10,000 times) to average all the results. My code is:
import numpy as np
import random
import numba
#numba.jit(nopython=True)
def integrador2(y,t,h): #this is the integrator of the function that solves the SDE
m = 6.6551079E-26 #parameters
gamma=0.05
T = 5E-3
k_b = 1.3806488E-23
b=np.sqrt(2*m*gamma*T*k_b)
c=np.sqrt(h)
for i in range(len(t)):
dW=c*random.gauss(0,1)
A=np.array([y[i,-1]/m,-gamma*y[i,-1]]) #this is the platen method that is applied at
B_dW=np.array([0,b*dW]) #each time step
z=y[i]+A*h+B_dW
Az=np.array([z[-1]/m,-gamma*z[-1]])
y[i+1]=y[i]+1/2*(Az+A)*h+B_dW
return y
def media(args): #args is a tuple with the parameters
y = args[0]
t = args[1]
k = args[2]
x=0
p=0
for n in range(k): #k=number of trajectories
y=integrador2(y,t,h)
x=(1./(n+1))*(n*x+y[:,0]) #I do the average like this so as not to have to save all the
p=(1./(n+1))*(n*p+y[:,1]) #solutions in memory
return x,p
The variables y, t and h are:
y0 = np.array([initial position, initial moment]) #initial conditions
t = np.linspace(initial time, final time, number of time intervals) #time array
y = np.zeros((len(t)+1,len(y0))) #array of positions and moments
y[0,:]=np.array(y0) #I keep the initial condition
h = (final time-initial time)/(number of time intervals) #time increment
I need to be able to run the program for a number of time intervals of 10 ** 7 and solve it 10 ** 4 times (k = 10 ** 4).
I feel that I have already reached a dead end because I already accelerate the function that calculates the result with Numba and then (although I do not put it here) I parallelize the "media" function to work with the four cores that my computer has. Even doing all this, my program takes an hour and a half to execute for 10 ** 6 time intervals and k = 10 ** 4, I have not had the courage to execute it for 10 ** 7 time intervals because my intuition tells me that it would take more than 10 hours.
I would really appreciate if someone could advise me to make some parts of the code faster.
Finally, I apologize if I have not expressed myself completely correctly in any part of the question, I am a physicist, not a computer scientist and my English is far from perfect.
I can save about 75% of compute time by simplifying the math in the loop:
def integrador2(y,t,h): #this is the integrator of the function that solves the SDE
m = 6.6551079E-26 #parameters
gamma=0.05
T = 5E-3
k_b = 1.3806488E-23
b=np.sqrt(2*m*gamma*T*k_b)
c=np.sqrt(h)
h = h * 1.
coeff0 = h/m - gamma*h**2/(2.*m)
coeff1 = (1. - gamma*h + gamma**2*h**2/2.)
coeffd = c*b*(1. - gamma*h/2.)
for i in range(len(t)):
dW=np.random.normal()
# Method 2
y[i+1] = np.array([y[i][0] + y[i][1]*coeff0, y[i][1]*coeff1 + dW*coeffd])
return y
Here's a method using filters with scipy, which I don't think is compatible with Numba, but is slightly faster than the solution above:
from scipy import signal
# #numba.jit(nopython=True)
def integrador2(y,t,h): #this is the integrator of the function that solves the SDE
m = 6.6551079E-26 #parameters
gamma=0.05
T = 5E-3
k_b = 1.3806488E-23
b=np.sqrt(2*m*gamma*T*k_b)
c=np.sqrt(h)
h = h * 1.
coeff0a = 1.
coeff0b = h/m - gamma*h**2/(2.*m)
coeff1 = (1. - gamma*h + gamma**2*h**2/2.)
coeffd = c*b*(1. - gamma*h/2.)
noise = np.zeros(y.shape[0])
noise[1:] = np.random.normal(0.,coeffd*1.,y.shape[0]-1)
noise[0] = y[0,1]
a = [1, -coeff1]
b = [1]
y[1:,1] = signal.lfilter(b,a,noise)[1:]
a = [1, -coeff0a]
b = [coeff0b]
y[1:,0] = signal.lfilter(b,a,y[:,1])[1:]
return y
I am currently trying to write some python code to solve an arbitrary system of first order ODEs, using a general explicit Runge-Kutta method defined by the values alpha, gamma (both vectors of dimension m) and beta (lower triangular matrix of dimension m x m) of the Butcher table which are passed in by the user. My code appears to work for single ODEs, having tested it on a few different examples, but I'm struggling to generalise my code to vector valued ODEs (i.e. systems).
In particular, I try to solve a Van der Pol oscillator ODE (reduced to a first order system) using Heun's method defined by the Butcher Tableau values given in my code, but I receive the errors
"RuntimeWarning: overflow encountered in double_scalars f = lambda t,u: np.array(... etc)" and
"RuntimeWarning: invalid value encountered in add kvec[i] = f(t+alpha[i]*h,y+h*sum)"
followed by my solution vector that is clearly blowing up. Note that the commented out code below is one of the examples of single ODEs that I tried and is solved correctly. Could anyone please help? Here is my code:
import numpy as np
def rk(t,y,h,f,alpha,beta,gamma):
'''Runga Kutta iteration'''
return y + h*phi(t,y,h,f,alpha,beta,gamma)
def phi(t,y,h,f,alpha,beta,gamma):
'''Phi function for the Runga Kutta iteration'''
m = len(alpha)
count = np.zeros(len(f(t,y)))
kvec = k(t,y,h,f,alpha,beta,gamma)
for i in range(1,m+1):
count = count + gamma[i-1]*kvec[i-1]
return count
def k(t,y,h,f,alpha,beta,gamma):
'''returning a vector containing each step k_{i} in the m step Runga Kutta method'''
m = len(alpha)
kvec = np.zeros((m,len(f(t,y))))
kvec[0] = f(t,y)
for i in range(1,m):
sum = np.zeros(len(f(t,y)))
for l in range(1,i+1):
sum = sum + beta[i][l-1]*kvec[l-1]
kvec[i] = f(t+alpha[i]*h,y+h*sum)
return kvec
def timeLoop(y0,N,f,alpha,beta,gamma,h,rk):
'''function that loops through time using the RK method'''
t = np.zeros([N+1])
y = np.zeros([N+1,len(y0)])
y[0] = y0
t[0] = 0
for i in range(1,N+1):
y[i] = rk(t[i-1],y[i-1], h, f,alpha,beta,gamma)
t[i] = t[i-1]+h
return t,y
#################################################################
'''f = lambda t,y: (c-y)**2
Y = lambda t: np.array([(1+t*c*(c-1))/(1+t*(c-1))])
h0 = 1
c = 1.5
T = 10
alpha = np.array([0,1])
gamma = np.array([0.5,0.5])
beta = np.array([[0,0],[1,0]])
eff_rk = compute(h0,Y(0),T,f,alpha,beta,gamma,rk, Y,11)'''
#constants
mu = 100
T = 1000
h = 0.01
N = int(T/h)
#initial conditions
y0 = 0.02
d0 = 0
init = np.array([y0,d0])
#Butcher Tableau for Heun's method
alpha = np.array([0,1])
gamma = np.array([0.5,0.5])
beta = np.array([[0,0],[1,0]])
#rhs of the ode system
f = lambda t,u: np.array([u[1],mu*(1-u[0]**2)*u[1]-u[0]])
#solving the system
time, sol = timeLoop(init,N,f,alpha,beta,gamma,h,rk)
print(sol)
Your step size is not small enough. The Van der Pol oscillator with mu=100 is a fast-slow system with very sharp turns at the switching of the modes, so rather stiff. With explicit methods this requires small step sizes, the smallest sensible step size is 1e-5 to 1e-6. You get a solution on the limit cycle already for h=0.001, with resulting velocities up to 150.
You can reduce some of that stiffness by using a different velocity/impulse variable. In the equation
x'' - mu*(1-x^2)*x' + x = 0
you can combine the first two terms into a derivative,
mu*v = x' - mu*(1-x^2/3)*x
so that
x' = mu*(v+(1-x^2/3)*x)
v' = -x/mu
The second equation is now uniformly slow close to the limit cycle, while the first has long relatively straight jumps when v leaves the cubic v=x^3/3-x.
This integrates nicely with the original h=0.01, keeping the solution inside the box [-3,3]x[-2,2], even if it shows some strange oscillations that are not present for smaller step sizes and the exact solution.
I have an stochastic differential equation (SDE) that I am trying to solve using Milsteins method but am getting results that disagree with experiment.
The SDE is
which I have broken up into 2 first order equations:
eq1:
eq2:
Then I have used the Ito form:
So that for eq1:
and for eq2:
My python code used to attempt to solve this is like so:
# set constants from real data
Gamma0 = 4000 # defines enviromental damping
Omega0 = 75e3*2*np.pi # defines the angular frequency of the motion
eta = 0 # set eta 0 => no effect from non-linear p*q**2 term
T_0 = 300 # temperature of enviroment
k_b = scipy.constants.Boltzmann
m = 3.1e-19 # mass of oscillator
# set a and b functions for these 2 equations
def a_p(t, p, q):
return -(Gamma0 - Omega0*eta*q**2)*p
def b_p(t, p, q):
return np.sqrt(2*Gamma0*k_b*T_0/m)
def a_q(t, p, q):
return p
# generate time data
dt = 10e-11
tArray = np.arange(0, 200e-6, dt)
# initialise q and p arrays and set initial conditions to 0, 0
q0 = 0
p0 = 0
q = np.zeros_like(tArray)
p = np.zeros_like(tArray)
q[0] = q0
p[0] = p0
# generate normally distributed random numbers
dwArray = np.random.normal(0, np.sqrt(dt), len(tArray)) # independent and identically distributed normal random variables with expected value 0 and variance dt
# iterate through implementing Milstein's method (technically Euler-Maruyama since b' = 0
for n, t in enumerate(tArray[:-1]):
dw = dwArray[n]
p[n+1] = p[n] + a_p(t, p[n], q[n])*dt + b_p(t, p[n], q[n])*dw + 0
q[n+1] = q[n] + a_q(t, p[n], q[n])*dt + 0
Where in this case p is velocity and q is position.
I then get the following plots of q and p:
I expected the resulting plot of position to look something like the following, which I get from experimental data (from which the constants used in the model are determined):
Have I implemented Milstein's method correctly?
If I have, what else might be wrong my process of solving the SDE that'd causing this disagreement with the experiment?
You missed a term in the drift coefficient, note that to the right of dp there are two dt terms. Thus
def a_p(t, p, q):
return -(Gamma0 - Omega0*eta*q**2)*p - Omega0**2*q
which is actually the part that makes the oscillator into an oscillator. With that corrected the solution looks like
And no, you did not implement the Milstein method as there are no derivatives of b_p which are what distinguishes Milstein from Euler-Maruyama, the missing term is +0.5*b'(X)*b(X)*(dW**2-dt).
There is also a derivative-free version of Milsteins method as a two-stage kind-of Runge-Kutta method, documented in wikipedia or the original in arxiv.org (PDF).
The step there is (vector based, duplicate into X=[p,q], K1=[k1_p,k1_q] etc. to be close to your conventions)
S = random_choice_of ([-1,1])
K1 = a(X )*dt + b(X )*(dW - S*sqrt(dt))
Xh = X + K1
K2 = a(Xh)*dt + b(Xh)*(dW + S*sqrt(dt))
X = X + 0.5 * (K1+K2)
I have a second order differential equation that I want to solve it in python. The problem is that for one of the variables I don't have the initial condition in 0 but only the value at infinity. Can one tell me what parameters I should provide for scipy.integrate.odeint ? Can it be solved?
Equation:
Theta needs to be found in terms of time. Its first derivative is equal to zero at t=0. theta is not known at t=0 but it goes to zero at sufficiently large time. all the rest is known. As an approximate I can be set to zero, thus removing the second order derivative which should make the problem easier.
This is far from being a full answer, but is posted here on the OP's request.
The method I described in the comment is what is known as a shooting method, that allows converting a boundary value problem into an initial value problem. For convenience, I am going to rename your function theta as y. To solve your equation numerically, you would first turn it into a first order system, using two auxiliary function, z1 = y and z2 = y', and so your current equation
I y'' + g y' + k y = f(y, t)
would be rewitten as the system
z1' = z2
z2' = f(z1, t) - g z2 - k z1
and your boundary conditions are
z1(inf) = 0
z2(0) = 0
So first we set up the function to compute the derivative of your new vectorial function:
def deriv(z, t) :
return np.array([z[1],
f(z[0], t) - g * z[1] - k * z[0]])
If we had a condition z1[0] = a we could solve this numerically between t = 0 and t = 1000, and get the value of y at the last time as something like
def y_at_inf(a) :
return scipy.integrate.odeint(deriv, np.array([a, 0]),
np.linspace(0, 1000, 10000))[0][-1, 0]
So now all we need to know is what value of a makes y = 0 at t = 1000, our poor man's infinity, with
a = scipy.optimize.root(y_at_inf, [1])