Charge distribution in the universe

In summary, the conversation discusses the concept of a uniformly charged distribution in an infinite universe and whether the field at any point would be zero. It is argued that the infinite universe cannot be considered to have a specific center and that the sum of electrostatic forces exerted by all the parts of the universe can converge to any real number due to conditional convergence. The idea of the universe being infinite is also challenged and it is concluded that the observable universe has a finite limit and what lies beyond it is irrelevant to the discussion.
  • #1
patiladitya98
4
1

Homework Statement


Can we consider the universe to have a uniformly charged distribution?
If so, shouldn't the field at any point in space be zero? Since the universe is infinite, will it be symmetrical about any point, field should be zero right? Why is this not true?[/B]2. The attempt at a solution
Can we argue that the infinite universe may be considered to be a sphere?
Thus if at any two points the field is zero, can we obtain a contradiction saying that, field is zero only at the centre of a uniformly charged sphere, and there cannot be two centres, so its absurd to say field at any 2 points is zero?

Thanks!
 
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  • #2
Your argument that the infinite universe "may be considered to be a sphere" so has a specific center is wrong. An infinite universe does not have a "center".
 
  • #3
I agree, that was the part I was not convinced about, anyway.
But then how do we explain the fact?
Is there any other argument that we may put forward to explain it?
 
  • #4
Are you aware of infinite series which are conditionally convergent? Such a series has terms which get smaller and smaller. If you add them all up in order, the sequence of partial sums converges to a particular number. For instance, 1 - 1/2 + 1/3 - 1/4 + 1/5 + ... But if you rearrange the series in a different order you can make the sum come out differently. It turns out that for a conditionally convergent series, it is possible to attain any sum you like with some suitable rearrangement of terms.

So how does that apply to an infinite universe? If the universe were infinite, homogeneous and flat (it's not) then you could partition it into a bunch of pieces. Say, for instance that you parcelled it out as a set of cubes each 1 light year on a side. Each of those cubes, by hypothesis, has the same charge as every other one. Each one exerts some net force on a test charge placed at the center of any chosen coordinate system. What result could you get if you added up the electrostatic forces exerted by all of those parcelled-out cubes?
 
  • #5
Wait, are you implying that the sum of the electrostatic forces may be converged to any real number?
It still seems to me that, by symmetry, that it would sum up to be zero, always :/
Still not too clear..
 
  • #6
patiladitya98 said:
Wait, are you implying that the sum of the electrostatic forces may be converged to any real number?
Yes, that is what I am saying. Since any number can be determined, the mathematical result is not defined.

It still seems to me that, by symmetry, that it would sum up to be zero, always :/
Indeed, if a result were uniquely determinable, that result would have to be zero. But first you have to show that the result is uniquely determinable. There's the rub.
 
  • #7
patiladitya98 said:
... Since the universe is infinite ...
Whoever told you that the universe is infinite misled you. It MAY be infinite, and in fact it evidence continues to pile up that it probably is, but there is not yet any such conclusion, so such questions can only be correctly phrased as "IF the universe is infinite ... "
 
  • #9
andrevdh said:
The expansion from the Big Bang over a limited amount of time
, 13.82 billion years, suggests that the universe should limit its size.
That is a limit to the size of the observable universe -- we can only see light that is 13.82 billion years old, so we can only see 13.82 billion light-years out. In the context of the question at hand this does indeed put a finite limit on the influence of a uniformly charged expanding universe.

Question is what is on the other side.
Whatever it is, it can't affect a test charge here. So it is irrelevant in this thread.
 

Related to Charge distribution in the universe

1. What is charge distribution in the universe?

Charge distribution in the universe refers to the way that electric charge is spread out and distributed throughout the vast expanse of space. This includes the distribution of charged particles, such as protons and electrons, as well as the larger-scale distribution of electric fields and magnetic fields.

2. How is charge distributed in the universe?

Charge distribution in the universe is not uniform or evenly spread out. It is influenced by many factors, including the movement of charged particles, interactions between particles, and the presence of cosmic structures like stars and galaxies. The distribution of charge also varies on different scales, from the atomic level to the level of entire galaxies.

3. What causes charge distribution in the universe?

The distribution of charge in the universe is primarily driven by the electromagnetic force, which is one of the four fundamental forces in nature. This force causes charged particles to interact with each other, leading to the formation of charged structures and the spread of electric fields. The distribution of charge is also influenced by gravity, which can affect the movement and clustering of charged particles.

4. How does charge distribution in the universe affect other phenomena?

The distribution of charge in the universe has a significant impact on many other phenomena, including the behavior of light and other electromagnetic radiation. Electric and magnetic fields play a crucial role in shaping the structure of the universe, from the formation of stars and galaxies to the dynamics of cosmic objects like black holes.

5. Can we observe charge distribution in the universe?

Yes, we can observe charge distribution in the universe through various methods, including telescopes, particle accelerators, and measurements of the cosmic microwave background radiation. These observations provide valuable insights into the structure and evolution of the universe, as well as the fundamental forces and particles that govern the behavior of charged matter.

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