Do the cosmological expansion affect binding systems

In summary: This is an end of the universe scenario in which the expansion of the universe will cause galaxies to be too distant from each other and eventually will cause the galaxies to collide. This will cause the universe to rip apart and we will all die.
  • #1
dimilion
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It is known that in result of the cosmological expansion the distances between galaxies increase according Hubble law v=H*r. Distant SNeIa show that the dark energy accelerates the expansion. I heard in a scientific popular transmission that in result of the acceleration of expansion, every molecule, atom and even nucleus will dissipate.
I think that the binding object like planetary systems, atoms, nuclei etc. not expand. What is the true?
 
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  • #2
Well, there is some effect, but it's not quite what you're probably thinking.

First of all, no, the expansion itself has no effect whatsoever on the dynamics of bound systems. You can understand the properties of a bound system in an expanding universe without paying any attention at all to what the rest of the universe is doing.

That said, dark energy does have an effect on the stability of bound systems, though the effect is very small for most any system you might think of, just because the density of dark energy is so low.

If the dark energy is a cosmological constant its energy density will stay constant in time, and its effects today will, therefore, be the same as its effects trillions of years from now. However, because the dark energy induces a repulsive gravitational force, it causes systems to become unstable on large time scales. I don't think it'll have any effect on our solar system or galaxies, but it does have a limited effect on galaxy clusters and larger structures, which can be seen in the CMB as what is known as the Integrated Sachs-Wolfe effect.

But what if dark energy is not a cosmological constant. One very exotic possibility is that it is a type of matter that has a more negative pressure than a cosmological constant. This would mean that the energy density of the cosmological constant increases with time. While most theorists are extremely skeptical that such a thing is even possible, it is easy enough to imagine what might happen if such a thing did exist: its effects would be very much like that of a cosmological constant, but with the radius at which its effects become important continually shrinking.

So, if dark energy was made up of this very exotic stuff, it would mean that even though right now basically only galaxy clusters and larger are large enough to be effected by any noticeable amount, eventually that size will shrink, and its effects on galaxies will become apparent, eventually being blown apart by the repulsive force of this stuff. As the energy density continues to grow, smaller and smaller structures would be blown apart by the repulsive force. It would even become so strong that it wouldn't just blow apart gravitational systems, but also electromagnetic ones like atoms, and even nuclear bound systems like atomic nuclei. This would be our universe ending in a "big rip".

The difficulty, however, is that this violates some energy conditions in General Relativity, something that most theorists find rather unlikely. For a while physicists didn't even bother considering the possibility that we might measure the pressure of dark energy to be more negative than a cosmological constant, a position that was reversed only when it was discovered that if dark energy and dark matter interact, we might get something that looked like it had more negative pressure than a cosmological constant, but only because we didn't take into account the interaction between dark matter and dark energy. Most still think a big rip is pretty unlikely.
 
  • #3
Thank you very much for the comprehensive answer of my question. Most probably, the authors of the above mentioned transmission have talked about “big rip” in case of this exotic form of dark energy.
 

1. How does the cosmological expansion affect the binding systems in our universe?

The cosmological expansion is the gradual increase in the distance between galaxies, caused by the expansion of space. This expansion does not directly affect the binding systems, such as planets and atoms, within galaxies. However, it does contribute to the overall expansion of the universe and can indirectly affect the stability of these systems over long periods of time.

2. Can the cosmological expansion cause objects within galaxies to break apart?

No, the gravitational forces within galaxies are strong enough to counteract the effects of the cosmological expansion. However, the expansion may contribute to the eventual separation of galaxies and clusters of galaxies.

3. Is the cosmological expansion a constant process?

Yes, the cosmological expansion has been observed to be occurring at a constant rate. This rate is known as the Hubble constant and is estimated to be approximately 70 km/s per megaparsec.

4. How does the cosmological expansion affect the formation of new binding systems?

The cosmological expansion does not directly affect the formation of new binding systems, such as stars and planets. However, it can indirectly affect the availability of matter and energy for these systems, as well as the overall structure and distribution of galaxies in the universe.

5. Can the cosmological expansion be reversed?

At this time, there is no known process or force that can reverse the cosmological expansion. However, there are theories that suggest the expansion may eventually slow down or even reverse in the distant future as the universe continues to evolve and change.

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