What is the effect of singularity on the calculation of charge density?

In summary: The charge density is also easy to calculate:##\displaystyle{{\bf{C}} = -\frac{\rho}{4\pi^2} }####\displaystyle{= -\frac{\rho}{4\pi^2} }##However, you can't just take the charge on the surface of the sphere:##\displaystyle{= -\frac{\rho}{4\pi^2} }####\displaystyle{= -\frac{\rho}{4\pi^2} }##You have to take the charge that's inside the sphere as well.
  • #1
spaghetti3451
1,344
33

Homework Statement



Determine the electric field and the charge density associated with the potential ##\displaystyle{V(r)=A\frac{\exp{-\lambda r}}{r}}##, where ##A## and ##\lambda## are constants.

Homework Equations



The Attempt at a Solution



The electric field is easy to determine:

##\displaystyle{{\bf{E}} = -\nabla V}##
##\displaystyle{= -A\ \nabla\left(\frac{\exp\left(-\lambda r\right)}{r}\right)}##
##\displaystyle{= -A\ \left(\frac{\partial}{\partial r}\left(\frac{\exp\left(-\lambda r\right)}{r}\right),0,0\right)}##
##\displaystyle{= A\ \left(\frac{(1+\lambda r)\exp\left(-\lambda r\right)}{r},0,0\right)}##

But the electric field is singular at the origin.

How does this affect the calculation of the charge density?
 
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  • #2
Well, that means you have a point charge at the origin - recall that ##\nabla \cdot \left(\frac{\vec{r}}{r^2}\right) = 4 \pi \delta(r)##.
 
  • #3
In which step have I made the mistake?

##\rho = \epsilon_{0}\ \nabla\cdot{{\bf{E}}}##

##= \epsilon_{0}\ A\ \nabla\cdot{\left((1+\lambda r)\frac{\exp\left(-\lambda r\right)}{r},0,0\right)}##

##= \epsilon_{0}\ \frac{A}{r^{2}}\ \frac{\partial}{\partial r} \left(r^{2}(1+\lambda r)\left(\frac{\exp\left(-\lambda r\right)}{r}\right)\right)##

##= \epsilon_{0}\ \frac{A}{r^{2}}\ \frac{\partial}{\partial r} \left[(r+\lambda r^{2})\exp\left(-\lambda r\right)\right]##

##= \epsilon_{0}\ \frac{A}{r^{2}}\ \left[(1+2\lambda r)\exp\left(-\lambda r\right)-\lambda(r+\lambda r^{2})\exp\left(-\lambda r\right)\right]##

##= \epsilon_{0}\ \frac{A}{r^{2}}\ \left[(1+2\lambda r)-\lambda(r+\lambda r^{2})\right]\exp\left(-\lambda r\right)##

##= \epsilon_{0}\ A\ \left[1+\lambda r-(\lambda r)^{2})\right]\frac{\exp\left(-\lambda r\right)}{r^{2}}##
 
  • #4
failexam said:
In which step have I made the mistake?
Here:
failexam said:
##\displaystyle{= -A\ \left(\frac{\partial}{\partial r}\left(\frac{\exp\left(-\lambda r\right)}{r}\right),0,0\right)}##
##\displaystyle{= A\ \left(\frac{(1+\lambda r)\exp\left(-\lambda r\right)}{r},0,0\right)}##
 
  • #5
I only missed a negative sign in the electric field, right?
 
  • #6
No, the signs are right; its the denominator that should be ##r^2##, no?
 

1. What is the singularity of potential?

The singularity of potential refers to a point in a physical system where the potential energy becomes infinite. It can also refer to a point where the potential energy becomes undefined or non-existent, such as at the center of a black hole.

2. Why is the singularity of potential important in physics?

The singularity of potential is important because it can have significant effects on the behavior and dynamics of a physical system. It can also provide insights into the fundamental laws of physics, such as the theory of general relativity.

3. How is the singularity of potential different from the singularity of density?

The singularity of potential and the singularity of density are two different concepts. The singularity of potential refers to a point where the potential energy becomes infinite, while the singularity of density refers to a point where the density becomes infinite.

4. Can the singularity of potential be observed or measured?

No, the singularity of potential cannot be directly observed or measured. It is a theoretical concept that helps in understanding certain physical phenomena, such as black holes.

5. Are there any real-life examples of the singularity of potential?

Yes, the most commonly known example of the singularity of potential is the singularity at the center of a black hole. It is also theorized to exist in other extreme physical systems, such as the Big Bang and the early universe.

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