Time for ring of equidistant particles to collapse (gravity)

In summary, the problem involves n identical particles of mass m distributed equi-distantly around the circumference of a ring of radius r in space. The particles are initially at rest and the ring is not rotating. The goal is to determine how long it will take for the particles to meet at the center of the ring under the force of gravitational attraction between them. This can be solved using the "time to meet function" which takes into account the universal gravitational constant, initial distance between particles, and their masses. By considering one particle attracted to another, we can find the component of force acting towards the common center and solve for the time it takes for the particles to meet.
  • #1
jjalexand
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(I assume that the three section headings below form the template referred to below)

1. Homework Statement

n identical equi-distant particles are distributed equi-distantly around the circumference of a ring of radius r in space. Each particles is of mass m, so the total mass of the ring is n*m. External gravitational fields are negligible and there is no other mass within the ring. The particles are initially at rest and the ring is not rotating. How long will it take the particles to meet at the center of the ring under gravitational attraction between the particles?


Homework Equations



"Time to meet function" for two particles at rest to meet under the force of gravity:

t = time to meet function = pi * (8 * G)^(-1/2) * x^(3/2) * (m1 + m2)^(-1/2)[/B]

where

t is the time to meet
G is the universal gravitational constant
x is the initial distance between the two particles
m1 and m2 are the masses of the two particles


Ref: Answers to Physics Forums question

The Attempt at a Solution

radius of ring = r
n particles of mass m
total mass n*m
the centre of mass of the ring is at the physical center of the ring
there are n^2 unique pairs of particles where each pair includes two particles attracting one another
the mutual gravitational attraction of each unique pair is independent of every other pair, i.e. the mutual attractions can be combined linearly and additively

Result for two particles is pi * (8 * G)^(-1/2) * (2r)^(3/2) * (m + m)^(-1/2)
Result for three particles is:[/B]

Side of an equilateral triangle inscribed in a circle of radius 1 is approx 1.732
There are three identical pairs each 1.732r, but the infall direction is towards the center of the ring not along the straight line between the particles, and it is hard to see how to use the time to meet function in this situation and also to generalize to n particles
 
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  • #2
jjalexand said:
there are n^2 unique pairs of particles
No, less than half that. Each pair consists of choosing 2 from n.
jjalexand said:
the mutual attractions can be combined linearly
Yes, but as vectors, so there will be cancellation. By symmetry, you only care about the forces pulling the particles to the common centre.

Just consider one particle A attracted to another, B, k steps around the circle.
Each step around the circle subtends what angle at the centre?
What angle do these two particles subtend?
How far is it between these two particles?
What is the force on A from B?
What is the component of that force acting towards the common centre?
 
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  • #3
haruspex said:
No, less than half that. Each pair consists of choosing 2 from n.

Yes, but as vectors, so there will be cancellation. By symmetry, you only care about the forces pulling the particles to the common centre.

Just consider one particle A attracted to another, B, k steps around the circle.
Each step around the circle subtends what angle at the centre?
What angle do these two particles subtend?
How far is it between these two particles?
What is the force on A from B?
What is the component of that force acting towards the common centre?

Dear Haruspex, thanks so much for your help, I really appreciate it very much, and I think I can do it given your excellent assistance, and thanks to Berkeman too :-)
 

1. How does gravity affect the time it takes for a ring of equidistant particles to collapse?

Gravity is the force that pulls objects towards each other. In the case of a ring of equidistant particles, the force of gravity between each particle will cause them to move closer together. This will result in the ring collapsing over time.

2. What factors influence the time it takes for a ring of equidistant particles to collapse under gravity?

The time it takes for a ring of equidistant particles to collapse under gravity is influenced by several factors, including the mass and density of the particles, the distance between each particle, and the strength of the gravitational force between them.

3. How can we calculate the time it takes for a ring of equidistant particles to collapse under gravity?

The time it takes for a ring of equidistant particles to collapse under gravity can be calculated using the formula t = √(3π/2Gρ), where t is the time in seconds, G is the gravitational constant, and ρ is the density of the particles.

4. Can the time for a ring of equidistant particles to collapse under gravity be affected by other forces?

Yes, the time for a ring of equidistant particles to collapse under gravity can be affected by other forces, such as electromagnetic or nuclear forces. These forces can counteract the force of gravity and potentially slow down or prevent the collapse of the ring.

5. What real-life examples can help us understand the concept of a ring of equidistant particles collapsing under gravity?

One real-life example of a ring of equidistant particles collapsing under gravity is the formation of planets and other celestial bodies. In this process, particles in a disk of dust and gas are pulled together by the force of gravity, forming a more dense and compact object over time.

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