Fernando Garcia

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From denominators to an integral: A proof of Feynman's parametrization

July 17th, 2024.

Introduction

In the last few weeks, I have used the so-called "Feynman Formula" for integrals, for which I much rather prefer the name "Feynman parametrization". This should not be confused with Feynman's trick "differentiation under the integral sign."

This technique is extremely useful when dealing with loop integrals in Quantum Field Theory. It is usually the case that the technique is presented but not proven, even though there seems to be a lot of magic going on under the hood. After all, it certainly breaks down an integral into a product of denominators!

This is what we are trying to show today:

1A1α1Anαn=Γ(iαi)iΓ(αi)1(n1)!dFnixiαi1(ixiAi)iαi

Where

dFn=(n1)!01dx1dxnδ(x1++xn1)

The above formula is a generalization of a simpler form of it (where we assume that all the alphas α are 1):

1A1An=dFn(x1A1++xnAn)1

Where we could argue that both serve the same purpose: Instead of having denominators to some power, you can take many denominators to the first power. This will, of course, add more xi variables to deal with later on.

The Gamma function

The Gamma function is defined by the following integral

Γ(z)=0tz1etdt

Which is related to the familiar notion of factorial for positive integers:

Γ(n)=(n1)!

More useful to us will be:

(i)Γ(α)Aα=0dttα1eAt

Which follows from a change of variables:

(Use u=At)0dttα1eAt=0duA(uA)α1eu=0duuα11Aα11Aeu=1Aα0duuα1eu=1AαΓ(α)

Another way of writing 1

Before employing Eq. (i), there is another thing we will make us of and needs some introduction/justification. Consider

(ii)1=0dsδ(siti)

An equation that follows directly from the definition of the Dirac delta δ(x):

δ(xa)dx=1

Proof of Feynman's formula

We have the tools needed to prove Feynman's parametrization.

Consider taking an indexed finite product of Eq. (i). That is, index the α and A values by some index i. For a product of two of them:

Γ(α1)Γ(α2)A1α1A2α2=0dt1dt2t1α11t2α21exp(A1t1A2t2)

And in general:

iΓ(αi)iAiαi=0dt1dtnitiαi1exp(iAiti)

We now multiply by 1 on both sides. That is, let's make us of Eq. (ii), placing the right hand side on the right hand side:

iΓ(αi)iAiαi=0dt1dtndsitiαi1exp(iAiti)δ(siti)

Let's change each ti variable by sxi, so that dti=sdxi:

iΓ(αi)iAiαi=0dx1dxndssni(sxi)αi1exp(iAisxi)δ(sisxi)

It is important to note that we picked up a factor of sn (one for each of the n u-subs). Let's now rewrite the right hand side by first making some important remarks:

The Delta Dirac satisfies δ(ax)=1|a|δ(x), so

δ(sisxi)=δ(s[1ixi])=1sδ(1ixi)

Where I ignored the absolute values at the end since s will always be non-negative.

Similarly, it is important to remark that

iaibi=(iai)(ibi)

So

i(sxi)αi1=(ixiαi1)(isαi1)=(ixiαi1)(isαi)(s1)n=(ixiαi1)(isαi)1sn=(ixiαi1)siαi1sn

The right-most factor of 1/sn will cancel with the factor of sn we picked up from the n u-substitutions. We see then that

iΓ(αi)iAiαi=0dx1dxnds(ixiαi1)siαi1exp(siAixi)δ(1ixi)

The s integral is an integral of the form of Eq. (i), with α=iαi and A=iAixi. The above then simplifies to (carry out the s integral):

iΓ(αi)iAiαi=0dx1dxn(ixiαi1)δ(1ixi)Γ(iαi)(iAixi)iαi

Cleaning this up a bit, and taking Γ(iαi) outside of the integral gives:

iΓ(αi)iAiαi=Γ(iαi)0dx1dxnδ(1x1x2xn)ixiαi1(iAixi)iαi

Since the (n) xis can't be greater than 1 (because of the δ function), it is safe to rewrite the above as integrals from 0 to 1 rather than to :

iΓ(αi)iAiαi=Γ(iαi)01dx1dxnδ(1x1x2xn)ixiαi1(iAixi)iαi

The combination of dxis integrals from 0 to 1 and the Dirac delta gives precisely (times a factor of (n1)!) the definition of dFn, so:

iΓ(αi)iAiαi=Γ(iαi)(n1)!dFnixiαi1(iAixi)iαi

So

1A1α1Anαn=Γ(iαi)iΓ(αi)1(n1)!dFnixiαi1(ixiAi)iαi

Conclusion

Of course, Equation (i) is true. This formula should not be thought of as a formula to solve integrals, but as a tool to make an expression take a more useful form. That is, it is not that we always want to go from the right hand side (an integral) to the left hand side (a denominator), but rather turn denominators into integrals.

A simple problem where this is used is in computing 1-loop corrections to the propagator of a ϕ3 theory. For more on this, see Srednicki chapter 14.


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