Dirac-delta function in spherical polar coordinates

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The discussion focuses on the application of the Dirac-delta function in spherical polar coordinates, particularly how to transition between integrals involving angular variables. The key point is the substitution from the integral form involving sine to one involving cosine, which is achieved through the relationship dcos(θ) = -sin(θ)dθ. Participants clarify that the delta function can be expressed in spherical coordinates, but caution that it cannot be done directly due to singularities along the polar axis. Additionally, a general formula for delta functions of composite variables is introduced, emphasizing the importance of understanding the derivatives involved in such transformations. The conversation highlights the complexities of working with delta functions in different coordinate systems.
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< Mentor Note -- thread moved from the Homework physics forums to the technical math forums >[/color]

Hello.I was reading recently barton's book.I reached the part corresponding to dirac-delta functions in spherical polar coordinates.
he let :##(\theta,\phi)=\Omega## such that ##f(\mathbf {r})=f(r,\Omega)##

##\int d^3r...=\int_0^{\infty}drr^2\int_0^{2π }dφ\int_0^π dθsinθ...##

define
##\int_0^{2π}dφ\int_0^πdθsinθ=\int_0^{2π}dφ\int_{-1}^{1}dcosθ=\int d\Omega##
then## δ(\mathbf {r-r^{'}})=\frac {1}{r^2} δ(r-r')δ(\Omega-\Omega^{'})##>>>(1)
where ##δ(\Omega-\Omega^{'})=δ(φ-φ')δ(cosθ-cosθ')##>>>(2)

My problem is that I really didn't get how he switched from ##\int_0^{2π }dφ\int_0^π dθsinθ## into ##\int_{-1}^{1}dcosθ##

same thing corresponding to relations (1) and (2), I didn't get how he obtained them?
If somebody can give me a hint for obtaining them? thanks.

Relevant equations

##\int d^3rf(\mathbf{r})δ(\mathbf{r})=f(0)##
where##δ(r)=δ(x)δ(y)δ(z)##
such that ##δ(r)=1/(2π)^3\int d^3kexp(i\mathbf{k}.\mathbf{r})##

The Attempt at a Solution


I need hints to know where yo start.
 
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amjad-sh said:
My problem is that I really didn't get how he switched from ##\int_0^{2π }dφ\int_0^π dθsinθ## into ##\int_{-1}^{1}dcosθ##
That is just a regular variable substitution. Note that ##d\cos(\theta) = -\sin(\theta)d\theta##. Also, the ##\phi## integral is still there.

amjad-sh said:
same thing corresponding to relations (1) and (2), I didn't get how he obtained them?
If somebody can give me a hint for obtaining them?
The three-dimensional delta function should have the property
$$
\int f(\vec r) \delta(\vec r - \vec r_0) dV = f(\vec r_0).
$$
You know that the delta function is zero everywhere except for at ##\vec r'## so make the ansatz ##\delta(\vec r - \vec r_0) = N \delta(r-r_0)\delta(\theta - \theta_0) \delta(\phi - \phi_0)## and start computing.
 
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Orodruin said:
The three-dimensional delta function should have the property

∫f(⃗r)δ(⃗r−⃗r0)dV=f(⃗r0).∫f(r→)δ(r→−r→0)dV=f(r→0).​

\int f(\vec r) \delta(\vec r - \vec r_0) dV = f(\vec r_0).
You know that the delta function is zero everywhere except for at ⃗r′r→′\vec r' so make the ansatz δ(⃗r−⃗r0)=Nδ(r−r0)δ(θ−θ0)δ(ϕ−ϕ0)δ(r→−r→0)=Nδ(r−r0)δ(θ−θ0)δ(ϕ−ϕ0)\delta(\vec r - \vec r_0) = N \delta(r-r_0)\delta(\theta - \theta_0) \delta(\phi - \phi_0) and start computing.

I started by the relation
##\int f(\vec r)δ(\vec r- \vec r')dV=f(\vec r')##
we have## f(\vec r)=f(r,θ,φ)##
##dV=drr^2sinθdθdφ##
##\int f(\vec r)δ(\vec r -\vec r')drr^2sinθdθdφ=f(\vec r')##
Then I let## δ(\vec r -\vec r')=A_1δ(r-r')A_2δ(θ-θ')A_3δ(φ-φ')##
then I let ##f(r,θ,φ)=f(r)f(θ)f(φ)## ... I don't know if this is allowed.
Then
##\int_0^{\infty}f(r)r^2drA_1δ(r-r')\int_0^πA_2f(θ)sin(θ)dθδ(θ-θ')\int_0^{2π}A_3f(φ)δ(φ-φ')dφ=f(r',θ',φ')##
then by doing the change of variable ##u=sinθdθ## ##\int_0^πA_2f(θ)sinθδ(θ-θ')dθ=\int_{-1}^{1}f(θ)dcosθδ(cosθ-cosθ')A_2## (*)
This will lead to ##A_1=1/r^2 and A_2=1 and A_3=1##
and then ##δ(\vec r-\vec r')=1/r^2δ(r-r')δ(φ-φ')δ(cosθ-cosθ')##
What I'm not convinced about is relation (*),how the change of variable let ##δ(θ-θ')=δ(cosθ-cosθ')## If you can clarify it to me?
 
No, it is not true that ##\delta(\theta - \theta') = \delta(\cos\theta - \cos\theta')## (there is a constant factor between the two). However, you can just as well assume a factor of ##\delta(\cos\theta -\cos\theta')## instead of a factor of ##\delta(\theta-\theta')##. This is in effect what you have done.
 
One should clarify a few further things. First of all you cannot express ##\delta^{(3)}(\vec{x})## in spherical coordinates since spherical coordinates are singular along the entire polar axis and particularly at the origin.

Second you can use the general formula
$$\delta[f(x)]=\sum_{j} \frac{1}{|f'(x_j)|} \delta(x-x_j),$$
where ##f## is a function that has only 1st-order roots ##x_j##.

Thus for ##\vartheta, \vartheta' \in ]0,\pi[## you have
$$\delta(\cos \vartheta-\cos \vartheta')=\frac{1}{\sin \vartheta} \delta(\vartheta-\vartheta').$$
 

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