Is Integration in d-Dimension Well Defined for 1<|q|<∞

  • Thread starter Thread starter kassem84
  • Start date Start date
  • Tags Tags
    Integration
kassem84
Messages
11
Reaction score
0
Hello,
As you may know in the context of dimensional regularization, integration is performed in d-dimension where d can take non-integer values. For example:
\int d^{d}q f(q^2)=S_{D}\int_{0}^{∞}q^{q-1}f(q^2)dq
My questions are:
1) Is the integration in d-dimension performed is well defined in the mathematical sense when integration is done for: 1<|q|<∞ rather than 0<q<∞:
\int_{|q|&gt;1} d^{d}q f(q^2)=S_{D}\int_{1}^{∞}q^{q-1}f(q^2)dq

2)Are tadpole mass-less integrals still equal to zero in DR?
\int_{|q|&gt;1} d^{d}q (q^2)^{β}= 0 for β=1,2,...

Thanks in advance.
Best regards.
 
Physics news on Phys.org
With regards to 1) I think that the integral should be fine. Just imagine
f(q2) = θ(q2-1)g(q2)

But as for 2) and the massless tadpoles, no, you can no longer consistently set them to zero.

Normally, for the integral over all q, you can argue for its vanishing in two ways:

a) Dimensional analysis: The only dimensional quantity is q, with [q]=1. So The integral has dimension d + 2β. Since you integrate out q, no dimensional quantities remain, so the only consistent result is that the integral must be 0.
b) The integral does not converge for any particular choice of d. But splitting the integral in half (or wherever) and choosing different d's for each half so that it converges in both UV and IR, then recombining the integral, the UV and IR poles cancel and the result is zero.

With your integral, both arguments don't work. For a), your "1" actually has the dimensions of mass (since otherwise |q|>1 would not make sense) and so the argument fails.
For b), you no longer have an IR limit, so there is no cancellation with the UV.

Hope that helps,
Simon
 
Thanks Simon for your answers.
 
Thread 'Why is there such a difference between the total cross-section data? (simulation vs. experiment)'
Well, I'm simulating a neutron-proton scattering phase shift. The equation that I solve numerically is the Phase function method and is $$ \frac{d}{dr}[\delta_{i+1}] = \frac{2\mu}{\hbar^2}\frac{V(r)}{k^2}\sin(kr + \delta_i)$$ ##\delta_i## is the phase shift for triplet and singlet state, ##\mu## is the reduced mass for neutron-proton, ##k=\sqrt{2\mu E_{cm}/\hbar^2}## is the wave number and ##V(r)## is the potential of interaction like Yukawa, Wood-Saxon, Square well potential, etc. I first...
Toponium is a hadron which is the bound state of a valance top quark and a valance antitop quark. Oversimplified presentations often state that top quarks don't form hadrons, because they decay to bottom quarks extremely rapidly after they are created, leaving no time to form a hadron. And, the vast majority of the time, this is true. But, the lifetime of a top quark is only an average lifetime. Sometimes it decays faster and sometimes it decays slower. In the highly improbable case that...
I'm following this paper by Kitaev on SL(2,R) representations and I'm having a problem in the normalization of the continuous eigenfunctions (eqs. (67)-(70)), which satisfy \langle f_s | f_{s'} \rangle = \int_{0}^{1} \frac{2}{(1-u)^2} f_s(u)^* f_{s'}(u) \, du. \tag{67} The singular contribution of the integral arises at the endpoint u=1 of the integral, and in the limit u \to 1, the function f_s(u) takes on the form f_s(u) \approx a_s (1-u)^{1/2 + i s} + a_s^* (1-u)^{1/2 - i s}. \tag{70}...

Similar threads

Replies
13
Views
5K
Replies
1
Views
1K
Replies
19
Views
2K
Replies
2
Views
2K
Replies
4
Views
2K
Replies
3
Views
1K
Replies
12
Views
3K
Replies
2
Views
959
Back
Top