Verify Newtonian Potential of Thin Spherical Shell

O if:\Phi(r) = A r^{-1} + B r^2 + C + \frac{1}{2 \pi \sigma a} ( A \ln(r+a) - A \ln(r-a) + 2 B a^2 + 2 C a )In summary, we can verify that the external potential due to the shell will be equal to that due to a point of the same mass as the shell located at O if the gravitational potential is given by the expression \Phi(r) = A r^{-1} + B r^2 + C + \frac{1}{2 \pi \sigma a} ( A \ln(r+a) - A \ln
  • #1
latentcorpse
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Consider a thin spherical shell of radius a and mass per unit area [itex]\sigma[/itex] whose centre at O lies a distance r from an external point P. If the gravitational potential r is [itex]\Phi(r)[/itex], verify that the external potential due to the shell will be equal to that due to a point of the same mass as the shell ([itex]4 \pi a^2 \sigma[/itex]) located at O if

[itex]\Phi(r) = A r^{-1} + B r^2 + C[/itex] where A,B and C are all constants.Hint: Show [itex]M(a) \Phi(r) + 2 \pi \sigma a \lambda(a) = \frac{2 \pi \sigma a}{r} \int_{r-a}^{r+a} x \Phi(x) dx[/itex] where [itex]\lambda(a)[/itex] is a constant which can be added without altering the force law.

I literally cannot seem to get anywhere with this problem!
 
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  • #2
I have tried deriving the potential due to the shell from its mass per unit area and then trying to equate it to that due to a point of the same mass, but can't seem to move forward.Answer:We start by calculating the gravitational potential due to the shell at a point P located at a distance r from the centre of the shell:M(a) \Phi(r) = \sigma \int_0^a 4 \pi r^2 dr \Phi(r) = 4 \pi \sigma \int_0^a r^2 \Phi(r) drNow we consider the potential due to a point of the same mass as the shell located at O:\frac{2 \pi \sigma a}{r} \int_{r-a}^{r+a} x \Phi(x) dx To show that these two potentials are equal, we add a constant \lambda(a) to the potential due to the shell such that:M(a) \Phi(r) + 2 \pi \sigma a \lambda(a) = \frac{2 \pi \sigma a}{r} \int_{r-a}^{r+a} x \Phi(x) dxThe constant \lambda(a) can be found by substituting the given expression for \Phi(r):M(a) (A r^{-1} + B r^2 + C) + 2 \pi \sigma a \lambda(a) = \frac{2 \pi \sigma a}{r} \int_{r-a}^{r+a} x (A x^{-1} + B x^2 + C) dxBy evaluating the integral on the right hand side and equating coefficients of like powers of r on both sides, we get:\lambda(a) = \frac{1}{2 \pi \sigma a} ( A \ln(r+a) - A \ln(r-a) + 2 B a^2 + 2 C a )Therefore, the external potential due to the shell will be equal to that due to a point of the same mass as the shell (4 \pi
 

FAQ: Verify Newtonian Potential of Thin Spherical Shell

What is the Newtonian potential of a thin spherical shell?

The Newtonian potential of a thin spherical shell refers to the gravitational potential energy created by a thin, hollow spherical object. It is based on Newton's law of universal gravitation, which states that the force of gravity between two objects is directly proportional to their masses and inversely proportional to the square of the distance between them.

How is the Newtonian potential of a thin spherical shell calculated?

The Newtonian potential of a thin spherical shell can be calculated by using the formula V = -GM/r, where G is the gravitational constant, M is the mass of the shell, and r is the distance from the center of the shell. This formula assumes that the shell has a uniform mass distribution and is thin enough to be treated as a point mass.

What is the significance of verifying the Newtonian potential of a thin spherical shell?

Verifying the Newtonian potential of a thin spherical shell is important because it confirms the validity of Newton's law of universal gravitation and the principles of classical mechanics. It also allows for accurate predictions of the gravitational effects of spherical objects, such as planets and stars, on other objects.

Can the Newtonian potential of a thin spherical shell be used to calculate the gravitational force at any point outside the shell?

No, the Newtonian potential of a thin spherical shell can only be used to calculate the gravitational force at points outside the shell that are located on the shell's central axis. This is because the potential is dependent on the distance from the center of the shell, and the potential is not constant at all points outside the shell.

What are some potential sources of error when verifying the Newtonian potential of a thin spherical shell?

Potential sources of error when verifying the Newtonian potential of a thin spherical shell include inaccuracies in measuring the mass and radius of the shell, deviations from a perfectly uniform mass distribution, and external factors such as the gravitational influence of nearby objects. Additionally, the assumption of a thin shell may not hold true in all cases, leading to discrepancies in the calculated potential.

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