Ordinarty differential equations

In summary, the conversation discusses techniques to investigate ordinary differential equations using a discrete description of the system called the master equation. The basic idea is to describe the system using a state function and define operators such as annihilation and creation operators and a number operator. The conversation also mentions the use of Feynman diagrams for the master equation. The speaker proposes two approaches to solving the master equation, one using a perturbative method and the other using the Lie product formula.
  • #1
Strum
105
4
With
$$
H = \alpha \left(x^{2}\partial_{x} - x \partial_{x} \right) + \beta\left(x \partial_{x}^{2} - x^{2}\partial_{x}^{2}\right)
$$

Sorry for the messed up tex. I don't know how to fix it. It works in my editor.

Hallo PF! This might become a somewhat long post so for the tldr-people just jump to the bold "introduction over".

John Baez and Jacob Biamonte recently published some lecture notes called A Course on Quantum Techniques for Stochastic Mechanics(http://arxiv.org/abs/1209.3632). In these notes they develope some techniques to investigate some ordinarty differential equations in continuus variables using a discrete description of the system instead( The master equation). It is sort of like going from the concentration of a thing to describing the actual things one by one. The basic idear is to describe the system using a state function
$$
\Psi(t) = \sum_{n} \psi_{n}(t)x^{n}
$$
## \psi_{n} ## is the probability of having a state with n things. That is we have
$$
\sum_{n} \psi_{n}(t) = 1
$$
A pure state of n things is thus given by ## \Psi(t) = x^{n} ##. The time evolution for this system is described by a hamiltonian and is given by
$$
d_{t} \Psi(t) = H\Psi(t)
$$
Hence the thread title :). Within this framework the anahilation and creation operators is simply
$$
a^{\dagger} = x \quad \text{and} \quad a = \partial_{x}
$$
As in quantum mechanics we define an expectation value as
$$
< O > = \left(O \Psi\right)\big|_{z=1} = \sum O \Psi
$$
Where the last equality is just notation such we match the one used in the notes. The last thing we need is the number operator given by
$$
N = a^{\dagger} a
$$
As far as I have understood in principle when taking the expectation value for the number operator we should in some sense get back to the solution of the original ordinary differential equations in the continuum variable( the concentration). These things and more can be found in chapter 2-5 of the lecture notes. Chapter 6 deals with feynman diagrams for the master equation. Essentially the develope a diagramatic expansion for the master equation by expanding the solution of the master equation as
$$
\exp(tH)\Psi(0) = (1 +tH + \frac{1}{2}t^{2}H^{2}+ \cdots)\Psi(0)
$$
Unfortunetly they do not show an example where this series converge or is easy to sum. This is more or less where you, physics forum comes in :) !
Introduction over
The simple ordinary differential equation
$$
\frac{dP}{dt} = \alpha P - \beta P^{2}
$$
Has the solution
$$
P(t) = \frac{Q}{1 + A \exp(-\alpha t)} \qquad \text{with} \qquad A = \frac{Q - P(0)}{P(0)}, \qquad Q = \frac{\alpha}{\beta}
$$
This is the example they study in chapter 6. Using the rules developed in chapter 5 we find that this system can be described in the discrete version by the hamiltonian
$$
H = \alpha \left(x^{2}\partial_{x} - x \partial_{x} \right) + \beta\left(x \partial_{x}^{2} - x^{2}\partial_{x}^{2}\right)
$$
(See chapter 6.3). Now I would like to see if it is possible to solve the master equation perturbatively and calculating ## < N > ## to get a better and better approximation to the solution given above.

Solution attempt 1.

Lets just calculate the first few terms in the expansion.
[tex]
\begin{align}
H^{2} =& (\beta^{2}a^{\dagger 4}-2\beta^{2}a^{\dagger3}+\beta^{2}a^{\dagger2})a^{4} \notag \\
&+(-2\alpha\beta a^{\dagger 4}+(4\alpha\beta+4\beta^{2})a^{\dagger3}+(-2\alpha\beta-6\beta^{2})a^{\dagger2}+2\beta^{2}a^{\dagger})a^{3} \notag \\
&+(\alpha^{2}a^{\dagger 4}+(-2\alpha^{2}-6\alpha\beta)a^{\dagger 3}+(\alpha^{2}+9\alpha\beta+2\beta^{2})a^{\dagger2}+(-3\alpha\beta-2\beta^{2})a^{\dagger})a^{2} \notag \\
&+(2\alpha^{2}a^{\dagger 3}+(-3\alpha^{2}-2\alpha\beta)a^{\dagger2}+(\alpha^{2}+2\alpha\beta)a^{\dagger})a
\end{align}
[/tex]
The next
[tex]
\begin{align}
H^{3} = & (-\beta^{3}a^{\dagger6}+3\beta^{3}a^{\dagger5}-3\beta^{3}a^{\dagger4}+\beta^{3}a^{\dagger3})a^{6} \notag \\
& +((-9\alpha\beta^{2}-12\beta^{3})a^{\dagger5}+6\beta^{3}a^{\dagger2}+(-3\alpha\beta^{2}-24\beta^{3})a^{\dagger3}+3\alpha\beta^{2}a^{\dagger6}+(9\alpha\beta^{2}+30\beta^{3})a^{\dagger4})a^{5} \notag \\ & +\big[(-9\alpha^{2}\beta-75\alpha\beta^{2}-38\beta^{3})a^{\dagger4}+(9\alpha^{2}\beta+30\alpha\beta^{2})a^{\dagger5}+6\beta^{3}a^{\dagger}-3\alpha^{2}\beta a^{\dagger6}+(-15\alpha\beta^{2}-44\beta^{3})a^{\dagger2} \notag \\ & +(3\alpha^{2}\beta+60\alpha\beta^{2}+76\beta^{3})a^{\dagger3}\big]a^{4} \notag \\
& +\big[(3\alpha^{3}+60\alpha^{2}\beta+76\alpha\beta^{2})a^{\dagger4}+(-3\alpha^{3}-24\alpha^{2}\beta)a^{\dagger5}+(-12\alpha\beta^{2}-16\beta^{3})a^{\dagger} \notag \\
&+\alpha^{3}a^{\dagger6}+(12\alpha^{2}\beta+88\alpha\beta^{2}+48\beta^{3})a^{\dagger2}+(-\alpha^{3}-48\alpha^{2}\beta-152\alpha\beta^{2}-32\beta^{3})a^{\dagger3}\big]a^{3} \notag \\
& +\big[(12\alpha^{3}+88\alpha^{2}\beta+48\alpha\beta^{2})a^{\dagger3}+(7\alpha^{2}\beta+24\alpha\beta^{2}+4\beta^{3})a^{\dagger}+(-15\alpha^{3}-44\alpha^{2}\beta)a^{\dagger4}+6\alpha^{3}a^{\dagger5} \notag \\
&+(-3\alpha^{3}-51\alpha^{2}\beta-72\alpha\beta^{2}-4\beta^{3})a^{\dagger2}\big]a^{2} \notag \\
& +((-\alpha^{3}-8\alpha^{2}\beta-4\alpha\beta^{2})a^{\dagger}+6\alpha^{3}a^{\dagger4}+(-12\alpha^{3}-16\alpha^{2}\beta)a^{\dagger3}+(7\alpha^{3}+24\alpha^{2}\beta+4\alpha \beta^{2})a^{\dagger2})a
\end{align}
[/tex]
And I have the next one as well but that probably won't help much. Looking for some thing more manageble let's look at the specific example of
$$
\alpha = \beta = 1 \quad \Psi(0) = x^{2}
$$
That is the pure state with 2 things which we will expect decays to x. Inserting I find
[tex]
\begin{align}
\Psi(0) & = z^{2} \\
tH\Psi(0) & = t\left(2 x^{3}-4 x^{2}+2 x \right)\\
\frac{t^{2}}{2!} H^{2}\Psi(0) & = \frac{t^{2}}{2!}\left(6 x^{4}-26 x^{3}+30 x^{2}-10 x \right)\\
\frac{t^{3}}{3!}H^{3}\Psi(0) & =\frac{t^{3}}{3!}\left( 24 x^{5}-174 x^{4}+366 x^{3}-286 x^{2}+70 x \right) \\
\frac{t^{4}}{4!}H^{4}\Psi(0) &=\frac{t^{4}}{4!} \left( 120 x^{6}-1296 x^{5}+4362 x^{4}-5954 x^{3}+3410 x^{2}-642 x \right)
\end{align}
[/tex]
(Why doesn't the tex work?)
The fourth order expansion of the exponential becomes
[tex]
\begin{align}
\Psi(t)_{(4)} =& 5t^{4}x^{6}+(-54t^{4}+4t^{3})x^{5}+(-29t^{3}+3t^{2}+(727/4)t^{4})x^{4}+(2t+61t^{3}-(2977/12)t^{4}-13t^{2})x^{3} \notag \\
&+(-4t+1+15t^{2}+(1705/12)t^{4}-(143/3)t^{3})x^{2}+((35/3)t^{3}-(107/4)t^{4}+2t-5t^{2})x
\end{align}
[/tex]
(the first 4 is to show that it is from the fourth order expansion). A quick calculation show that ## \sum_{n=1}^{4}\psi_{(4),n}(t) = 1 ## however ## \sum_{n=1}^{4}|\psi_{(4),n}(t)| \neq 1##.
Looking at the solution of $\Psi$ to different orders I find
[tex]
\begin{align}
\psi_{(1),2} & < 0 \quad \text{for} \quad t>\frac{1}{4} \\
\psi_{(2),3} & < 0 \quad \text{for} \quad t>\frac{2}{13} \\
\psi_{(3),4} & < 0 \quad \text{for} \quad t>\frac{3}{29} \\
\psi_{(4),5} & < 0 \quad \text{for} \quad t>\frac{2}{27}
\end{align}
[/tex]
That is the probability becomes negative at shorter and shorter time the higher I expand! This seems horrible.
Is there any reasonably comments on this? I do not know what to do with this :(.


Solution attempt 2

Rescaling the coefficients in the starting ordinary differential equation I find
$$
\frac{dP}{dt} = -\alpha P - 2\beta P^{2}
$$
Which gives the hamiltonian
$$
H = \alpha \left(a -a^{\dagger}a\right) + \beta \left(a^{2} - a^{\dagger2}a^{2}\right)
$$
Perhaps it is possible to use something like the Lie product formula
$$
e^{tH}\Psi = \lim_{N \rightarrow \infty} \left(e^{t \alpha a/N}e^{-t \alpha a^{\dagger}a/N} e^{t\beta a^{2}/N} e^{-t\beta a^{\dagger2}a^{2}/N} \Psi^{1/N}\right)^{N}
$$
Defining ## \Psi = x^{n} ## using some known identities for the generators of scaling and translation and some calculations I find
[tex]
\begin{align}
e^{-t \alpha a^{\dagger}a/N } \Psi^{1/N} &= \Psi^{1/N} \exp\left( - t\alpha \frac{n}{N^{2}} \right) = \Psi^{1/N}A_{\alpha} \\
e^{-t\beta a^{\dagger2}a^{2}/N} \Psi^{1/N} &= \Psi^{1/N}\exp\left( - t\beta \frac{n/N (n/N-1)}{N} \right) = \Psi^{1/N}A_{\beta} \\
e^{t \alpha a/N}\Psi^{1/N} &= \left(x + t\alpha/N\right)^{n/N} \\
e^{t\beta a^{2}/N} \left(x + t\alpha/N\right)^{n/N} & =\left(x + t\alpha/N\right)^{n/N} \sum_{k=0}^{\infty}\frac{(n/N)^{\underbar{2k}}}{\left(Nx+t\alpha\right)^{2k}k!}\left(tN\beta \right)^{k}
\end{align}
[/tex]
(is there a limit on how many tex I can use?)
This is how far I've gotten with this approach. I don't even know if it is okay to use this Lie product formula.
Any sort of help would be very much appriciated :). Even vague ideas are welcome.
 
Last edited by a moderator:
Physics news on Phys.org
  • #2



Hi there,

Thank you for sharing your thoughts and ideas on this topic. I am not familiar with the lecture notes you mentioned, but I find the concept of using a discrete description to investigate ordinary differential equations in continuous variables very interesting. It seems like a useful tool for understanding and solving these types of equations.

Regarding your solution attempts, I am not sure if I fully understand the notations and calculations, but I do have a few thoughts and suggestions. In your first attempt, it seems like you are expanding the exponential solution of the master equation in terms of the Hamiltonian. However, I am not sure if this approach is valid, as the master equation is a first-order differential equation while the Hamiltonian is a second-order differential operator. Perhaps this is why you are getting negative probabilities? I am not sure, but it might be worth exploring this further.

In your second attempt, using the Lie product formula seems like a promising approach. However, I am not sure if your expressions for the generators of scaling and translation are correct. It might be worth double-checking these or looking for other references on these operators. Additionally, I am not sure if your expression for the exponential of the Hamiltonian is correct, as the Hamiltonian is a second-order differential operator while your expression seems to involve only first-order terms. Maybe you could try expanding the exponential using the Baker-Campbell-Hausdorff formula and see if that leads to anything useful.

Overall, I think your ideas and approaches are very interesting and have potential. It might be worth discussing them with colleagues or seeking out other resources or references on these topics to further develop your ideas. I hope this helps and I wish you the best of luck in your research!
 

What are ordinary differential equations?

Ordinary differential equations (ODEs) are mathematical equations that describe the relationship between a function and its derivatives. They involve only one independent variable, such as time, and the derivatives represent the rate of change of the dependent variable with respect to the independent variable.

What is the difference between ordinary and partial differential equations?

The main difference between ordinary and partial differential equations is the number of independent variables. ODEs involve only one independent variable, while partial differential equations (PDEs) involve two or more independent variables. This means that PDEs are more complex and require different techniques to solve them.

What are some real-world applications of ordinary differential equations?

ODEs are used in many fields of science and engineering to model and predict the behavior of systems over time. They are commonly used in physics, chemistry, biology, economics, and engineering to describe processes such as population growth, chemical reactions, motion, and heat transfer.

How are ordinary differential equations solved?

ODEs can be solved analytically or numerically. Analytical solutions involve finding an exact expression for the dependent variable as a function of the independent variable. Numerical solutions involve using numerical methods, such as Euler's method or Runge-Kutta methods, to approximate the solution. The choice of method depends on the complexity of the equation and the required level of accuracy.

What are some common techniques for solving ordinary differential equations?

Some common techniques for solving ODEs include separation of variables, integrating factors, and substitution. These techniques are used to reduce the equation to a simpler form that can be solved analytically. Other techniques, such as Laplace transforms and power series, can also be used for more complex equations.

Similar threads

  • Differential Equations
Replies
2
Views
2K
  • Differential Equations
Replies
3
Views
1K
  • Quantum Physics
Replies
5
Views
444
  • Differential Equations
Replies
14
Views
2K
  • Differential Equations
Replies
3
Views
1K
  • Differential Equations
Replies
1
Views
666
Replies
1
Views
1K
Replies
3
Views
622
  • Differential Equations
Replies
2
Views
1K
  • Differential Equations
Replies
7
Views
390
Back
Top