Sunday, 24 September 2017

quantum field theory - Loop integral using Feynman's trick


I am trying to show for the one-loop integral with three propagators with different internal masses m1, m2, m3, and all off-shell external momenta p1, p2, p3 the following formula appearing in 't Hooft(1979), Bardin (1999), Denner (2007): (unfortunate metric ,+,+,+)


ddq1(q2+m21)((q+p1)2+m22)((q+p1+p2)2+m23)

=iπ210dxx0dy1ax2+by2+cxy+dx+ey+f



where a, b, c, ... are coefficients depending on the momenta in the following way:


a=p22,


b=p21,


c=2p1.p2,


d=m22m23+p22,


e=m21m22+p21+2(p1.p2),


f=m23iϵ.


I don't really care about factors in fromt like iπ2. My simple problem is: I am totally unable to reproduce coefficients d, e and f. The problem is, when I integrate over the third Feynman parameter, m3 appears in all three coefficients d, e and f. How do I squeeze the denominators to reproduce this formula?



Answer



Define the LHS of the equation above:



I=ddq1(q2+m21)((q+p1)2+m22)((q+p1+p2)2+m23)


The first step is to squeeze the denominators using Feynman's trick:


I=10dxdydzδ(1xyz)ddq2[y(q2+m21)+z((q+p1)2+m22)+x((q+p1+p2)2+m23)]3


The square in q2 may be completed in the denominator by expanding:


[denom]=q2+2q.(zp1+x(p1+p2))+ym21+z(p21+m22)+x(m23+(p1+p2)2)

=q2+2q.Q+A2


where Qμ=zpμ1+x(p1+p2)μ and A2=ym21+z(p21+m22)+x(m23+(p1+p2)2), and by shifting the momentum, qμ=(kQ)μ as a change of integration variables. Upon performing the k integral, we are left with integrals over Feynman parameters (because this integral has three propagators, it is UV finite):


I=iπ210dxdydzδ(1xyz)1[Q2+A2]


Now integrate over z with the help of the Dirac delta:


I=iπ210dx1x0dy1[Q2+A2]z1yz


To arrive at the RHS of the OP's equation(which is the part I forgot to do), we make a final change of variables: x=1x:



So that the denominator reads ax2+by2+cxy+dx+ey+f, with the coefficients a,b,c, exactly defined in the question of OP. Note the change in the range of integration in y.


I=iπ210dxx0dy1ax2+by2+cxy+dx+ey+f


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