Feynman parametrization explained
Feynman parametrization is a technique for evaluating loop integrals which arise from Feynman diagrams with one or more loops. However, it is sometimes useful in integration in areas of pure mathematics as well.
Formulas
Richard Feynman observed that:[1]
| du |
\left[uA+(1-u)B\right]2 |
which is valid for any complex numbers A and B as long as 0 is not contained in the line segment connecting A and B. The formula helps to evaluate integrals like:
\begin{align}
\int
&=\intdp
| du |
\left[uA(p)+(1-u)B(p)\right]2 |
\\
&=
du\int
| dp |
\left[uA(p)+(1-u)B(p)\right]2 |
.
\end{align}
If A(p) and B(p) are linear functions of p, then the last integral can be evaluated using substitution.
:
[2]
&=(n-1)!
du1 …
dun
| |
| n | | \left(\sum | | ukAk\right)n | | k=1 | |
|
\\
&=(n-1)!
du1
du2 …
dun-1
| 1 |
\left[A | | n-1+A2(un-2-un-1)+...+An(1- | | 1u | |
|
.
\end{align}
This formula is valid for any complex numbers A1,...,An as long as 0 is not contained in their convex hull.
Even more generally, provided that
for all
:
=
| \Gamma(\alpha1+...+\alphan) |
\Gamma(\alpha1) … \Gamma(\alphan) |
du1
dun
where the
Gamma function
was used.
[3] Derivation
By using the substitution
,
we have
, and
,
from which we get the desired result
=
| du |
\left[uA+(1-u)B\right]2 |
.
In more general cases, derivations can be done very efficiently using the Schwinger parametrization. For example, in order to derive the Feynman parametrized form of
, we first reexpress all the factors in the denominator in their Schwinger parametrized form:
and rewrite,
ds1 …
dsn\exp\left(-\left(s1A1+ … +snAn\right)\right).
Then we perform the following change of integration variables,
\alphai=
; i=1,\ldots,n-1,
to obtain,
=
d\alpha1 … d\alphan-1
d\alpha \alphan-1\exp\left(-\alpha\left\{\alpha1A1+ … +\alphan-1An-1+\left(1-\alpha1- … -\alphan-1\right)An\right\}\right).
where
denotes integration over the region
with
.
The next step is to perform the
integration.
d\alpha \alphan-1\exp(-\alphax)=
| \partialn-1 |
\partial(-x)n-1 |
d\alpha\exp(-\alphax)\right)=
.
where we have defined
x=\alpha1A1+ … +\alphan-1An-1+\left(1-\alpha1- … -\alphan-1\right)An.
Substituting this result, we get to the penultimate form,
d\alpha1 … d\alphan-1
| 1 |
[\alpha1A1+ … +\alphan-1An-1+\left(1-\alpha1- … -\alphan-1\right)An]n |
,
and, after introducing an extra integral, we arrive at the final form of the Feynman parametrization, namely,
d\alpha1 … \int
d\alphan
| \delta\left(1-\alpha1- … -\alphan\right) |
[\alpha1A1+ … +\alphanAn]n |
.
Similarly, in order to derive the Feynman parametrization form of the most general case, one could begin with the suitable different Schwinger parametrization form of factors in the denominator, namely,
and then proceed exactly along the lines of previous case.
Alternative form
An alternative form of the parametrization that is sometimes useful is
This form can be derived using the change of variables
.We can use the
product rule to show that
, then
&=
| du |
\left[uA+(1-u)B\right]2 |
\\
&=
\\
&=
\\
\end{align}
More generally we have
=
| \Gamma(m+n) |
\Gamma(m)\Gamma(n) |
| λm-1dλ |
\left[λA+B\right]n+m |
,
where
is the
gamma function.
This form can be useful when combining a linear denominator
with a quadratic denominator
, such as in
heavy quark effective theory (HQET).
Symmetric form
A symmetric form of the parametrization is occasionally used, where the integral is instead performed on the interval
, leading to:
=
| du |
\left[(1+u)A+(1-u)B\right]2 |
.
Notes and References
- Feynman . R. P. . 1949-09-15 . Space-Time Approach to Quantum Electrodynamics . Physical Review . 76 . 6 . 769–789 . 10.1103/PhysRev.76.769.
- Book: Weinberg, Steven. The Quantum Theory of Fields, Volume I. 2008. Cambridge University Press. Cambridge. 497. 978-0-521-67053-1.
- Web site: Notes on Feynman Parametrization and the Dirac Delta Function. Kristjan Kannike. https://web.archive.org/web/20070729015208/http://www.physic.ut.ee/~kkannike/english/science/physics/notes/feynman_param.pdf. 2007-07-29. 2011-07-24.