Can Two Stars in a Static Universe Ever Collide Due to Gravitational Influence?

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Discussion Overview

The discussion revolves around the hypothetical scenario of two stars in a static universe and whether they could ever collide due to gravitational influence. Participants explore the implications of gravitational attraction, the nature of static conditions, and the mathematical relationships governing such interactions.

Discussion Character

  • Exploratory
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant questions how much distance would need to be between two stars to ensure they never collide, given that they are initially at rest in a static universe.
  • Another participant states that gravitational influence diminishes with distance, suggesting it approaches zero at infinity.
  • Some participants propose that even at extreme distances, such as 50 billion light years, gravitational attraction could still lead to eventual collision, although this is debated.
  • Concerns are raised about the validity of the inverse square law under extreme conditions, referencing phenomena like the Pioneer Anomaly and MOND theories.
  • There is a discussion about the quantization of gravitational fields and how this might affect the interaction between distant particles.
  • Participants explore the concept of angular velocity and how it could influence whether two grains of sand would collide or miss each other.
  • One participant argues that if two objects are in orbit and do not collide on their first pass, they will not collide in subsequent passes, while another counters that orbits can decay over time due to gravitational radiation.
  • Mathematical expressions are provided to describe the potential energy and momentum conditions necessary for the grains of sand to be in a bound state.
  • There is a mention of the uncertainty principle and how it applies to the initial conditions of the system, suggesting that the spread of the wavefunction could impact the likelihood of collision.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the gravitational influence between distant objects, the validity of classical gravitational laws in extreme scenarios, and the implications of quantum mechanics on the behavior of such systems. The discussion remains unresolved with no consensus reached.

Contextual Notes

Participants note limitations in the assumptions made about the static nature of the universe and the implications of gravitational decay over time. The discussion also highlights the dependence on definitions of static conditions and the complexities introduced by quantum mechanics.

Holocene
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Gravitational influence?

Suppose for a senond that the only objects in the entire univesre are 2 stars, both about as massive as the sun.

Also, this univesre is completely static. It is not expanding.

The stars, at least initially, are not moving relative to each other.

Under these conditions, about how much distance would need to be between the stars so as to ensure that they never collide?

Or does gravitational influence never deminish to zero, no matter how far away you get?
 
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gravity=1/d^2
it equals zero at infinity
 


granpa said:
gravity=1/d^2
it equals zero at infinity

So 2 grains of sand, 50 Billion light years apart, will eventually collide, even under static conditions?

That is pretty interesting when you think about it.
 


Holocene said:
So 2 grains of sand, 50 Billion light years apart, will eventually collide, even under static conditions?

That is pretty interesting when you think about it.

Thinking of all this Pioneer Anomaly and MOND mumbo jumbo, I would not bet my life that the equation given by granpa is really correct under such extreme conditions as you specified. A few decades later we may be smarter - or maybe not... All we can say now is yes, there is wide agreement that the 1/r^2 relation is correct and yes, the 2 grains of sand will eventually collide (but don't hold your breath for it...)
 


Oberst Villa said:
Thinking of all this Pioneer Anomaly and MOND mumbo jumbo, I would not bet my life that the equation given by granpa is really correct under such extreme conditions as you specified.
Well, 1] even if there is any substance to the Pioneer anomaly, then they still will collide. At worst, we might have the delay wrong.

2] It will take more than one anomaly to overturn centuries of verification and countless confirming experiment after countless confirming experiment of gravity's effect.
 


Holocene said:
So 2 grains of sand, 50 Billion light years apart, will eventually collide, even under static conditions?

That is pretty interesting when you think about it.

yes, its actually very interesting. the gravitational field presumably like all fields is quantized both spatially and in intensity (I think that's called second quantization or something more or less like that) so what happens when the gravitational field from a particle diminishes to the level of one quanta?
 


Holocene said:
So 2 grains of sand, 50 Billion light years apart, will eventually collide, even under static conditions?

That is pretty interesting when you think about it.
unless you define static conditions for me, i guess those grains of sand would just explode because theyre in a vacuum... or am i wrong here?
 


joris20 said:
unless you define static conditions for me, i guess those grains of sand would just explode because theyre in a vacuum... or am i wrong here?
Grains of sand explode in vacuum?? Awesome!

:rolleyes:
 


Holocene said:
The stars, at least initially, are not moving relative to each other.
I have a hard-time seeing how this configuration is a valid GR solution.
 
  • #10


The amount of time will be

t \approx 2\pi\sqrt{\frac{(0.5 d)^{3}}{G(m_{1}+m_{2})}}

where d is the distance that separates them, and m1 and m2 are their masses.
 
  • #11


So 2 grains of sand, 50 Billion light years apart, will eventually collide, even under static conditions?

If the grains of sand have a small angular velocity relative to each other, they'll miss. The farther away they are relative to each other, the smaller that angular velocity can be for the grains to hit each other. Now, the initial state will be some so-called coherent state in which the initial position is described by some wavefunction that corresponds to both position and momentum being in some small uncertainty interval.

So, you can simply use the uncertainty relation to estimate the maximum distance beyond which it becomes impossible to let the grains hit each other with reasonable probability.
 
  • #12


but even if they mis they could re-attract each other and have a "second chance"

etc. etc.
 
  • #13


joris20 said:
but even if they mis they could re-attract each other and have a "second chance"

etc. etc.
No. They are in orbit. If they didn't collide on the first pass, they never will. There's nothing to change their paths from the orbit.

In fact, one orbit will bring them back to their initial starting point, 50Gly apart and stopped wrt each other.


BTW, this whole problem makes the assumption that the universe is of infinite age (which, I guess, if there are only two particles in it, is pretty much a given) because these passes will take longer than our current universe's likely age.
 
  • #14


DaveC426913 said:
No. They are in orbit. If they didn't collide on the first pass, they never will. There's nothing to change their paths from the orbit.
That is simply not true under general relativity. The orbit will decay slowly.
 
  • #15


MeJennifer said:
That is simply not true under general relativity. The orbit will decay slowly.

Yes, but really really really slowly. They will only come close to each other every [too lazy to put the numbers in tony873004's equation] billion years, and even during this short encounter the loss of energy due to gravitational radiation will be soooooo tiny.
 
  • #16


well were tqlking about 'in the end' so technically, we have eternity which seems long enough :p
 
  • #17


Take two grains of sand a distance of r (say about 50 billion lightyears) apart at rest. The mass of a grain of sand is m
(say 10^-6 Kg) . The potential energy is:


E = G m^2/r

For the system to be in a bound state, the momentum of the grains must not exceed P, given by:

P^2/m = G m^2/r ----------->


P = Sqrt[G m^3/r]



If the intital state is given by some wavepacket then in momentum space the spread must be significantly less than P. The uncertainty relation then gives a spread of the wavefunction in configuration space of:

Delta X = hbar/2 Sqrt[r/(G m^3)]

This is about 140 nm for the two dust grains placed 50 billion lightyears apart. I don't think it is realistic to assume that this wavefunction won't decohere into a statistical mixture of wavefunctions with much sharper defined positions.
 

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