What is the functional integral theorem for polynomial times Gaussian integrals?

Click For Summary
The discussion centers on the functional integral theorem for polynomial times Gaussian integrals, specifically the integral of a polynomial multiplied by a Gaussian function. The key result presented is that this integral can be expressed as P(-∂/∂b)(det A)^{-1/2}, with the derivation involving differentiation under the integral sign. The conversation clarifies that the expression for the integral can be derived by completing the square and shifting the integration variable, leading to a relationship with the Taylor expansion of the polynomial. It is noted that if the polynomial has an infinite Taylor expansion, the exchange of summation and integration may not be valid. The participants conclude that understanding the role of the linear term in the integral is crucial for grasping the theorem.
Chopin
Messages
367
Reaction score
13
I've been watching Sidney Coleman's QFT lectures (http://www.physics.harvard.edu/about/Phys253.html). I've gotten up to his discussion of functional integration, and I have some questions.

He starts out by discussing a finite-dimensional integral of a Gaussian function: \int{\frac{d^n x}{(2\pi)^{n/2}}e^{-\frac{1}{2}xAx}} = (det A)^{-1/2}, where x is an n-dimensional vector, and A an n-dimensional symmetric matrix. So far, that makes sense--if you diagonalize A, it just turns into the product of n Gaussian integrals. He then goes on to discuss the integral of a polynomial times a Gaussian, \int{\frac{d^n x}{(2\pi)^{n/2}}P(x)e^{-\frac{1}{2}xAx}}, where P(x) is a polynomial. Seemingly out of nowhere, he gives the result of this integral as P(-\frac{\partial}{\partial b})(det A)^{-1/2}. I have absolutely no idea where this comes from.

Google is turning up bits and pieces of information on this, but nothing I can make a complete picture out of. The best I've been able to work out is that it's in some way related to differentiating under the integration sign, but I can't quite put the pieces together. This is clearly going to become important in the subsequent sections, where we're going to go on to develop the path integral formulation of QFT, so I'd really like to figure this out. Can anybody shed any light on how this works?
 
Physics news on Phys.org
Near as I can tell, there are some missing pieces to the formula you wrote. Perhaps these were not copied correctly in the notes?

The general expressions is <br /> f(A,b) = \int \frac{d^n x}{(2\pi)^{n/2}} \exp{\left(-\frac{x A x}{2} + b x\right)} = \left(\det{A}\right)^{-1/2} \exp{\left(\frac{b A^{-1} b}{2}\right)}.<br />
The final equality follows by completing the square under the integral and then shifting the integration variable. Now assuming that you can exchange integration and differentiation you can write

<br /> \int \frac{d^n x}{(2\pi)^{n/2}} x^k \exp{\left(-\frac{x A x}{2}\right)} = \int \frac{d^n x}{(2\pi)^{n/2}} \left[\frac{\partial^k}{\partial b^k} \exp{\left(-\frac{x A x}{2}+bx\right)}\right]_{b=0} = \left[\frac{\partial^k}{\partial b^k} f(A,b) \right]_{b=0}.<br />
The expression for general P then follows from the Taylor expansion of P. There is some indexology that I have left schematic, but let me know if you have trouble working it out. Also, note that if P has an infinite Taylor expansion then the exchange of summation and integration may not be valid i.e. one could use P(d/db) inside the integral but not outside it.
 
Last edited:
Ahh, that's where the b comes from. Yeah, he added a linear term earlier on in the lecture when discussing the integral of a generalized Gaussian, but by the time we got to this point, he'd absorbed everything into a general quadratic form e^{-Q(x)}, so I didn't realize that was the b we were talking about. I didn't include it in my initial description because I didn't realize it was relevant, but now I see what's going on.

Physics Monkey said:
Also, note that if P has an infinite Taylor expansion then the exchange of summation and integration may not be valid i.e. one could use P(d/db) inside the integral but not outside it.
P(x) is given as being a finite-order polynomial, so I can say with reasonable certainty that its Taylor expansion terminates. :smile:

Thank you very much--this makes perfect sense now.
 
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

Similar threads

  • · Replies 7 ·
Replies
7
Views
1K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 24 ·
Replies
24
Views
2K
  • · Replies 13 ·
Replies
13
Views
2K
  • · Replies 15 ·
Replies
15
Views
3K
  • · Replies 11 ·
Replies
11
Views
2K
  • · Replies 19 ·
Replies
19
Views
3K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 59 ·
2
Replies
59
Views
5K
  • · Replies 4 ·
Replies
4
Views
1K