Expanding Spacetime - Inside an Atom?

Click For Summary

Discussion Overview

The discussion revolves around the concept of spacetime expansion and its potential effects within atomic structures. Participants explore whether the expansion of spacetime influences the size of atoms, particularly the distances between electrons and nuclei, and the implications of this on fundamental physics.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants propose that spacetime is expanding everywhere, questioning if this expansion affects the radii of electrons within atoms.
  • Others argue that we cannot measure this expansion within atoms because the measuring tools (rulers) would also be expanding, suggesting a potential non-homogeneity in spacetime expansion.
  • It is noted that atoms do not partake in the universe's expansion, as their size is determined by fundamental constants that have remained stable over time.
  • A participant expresses confusion about why spacetime near matter does not expand like intergalactic space, seeking clarification on the differences in behavior.
  • Another participant clarifies that while spacetime itself may not be different, the forces within an atom keep it from expanding, as the electron and nucleus maintain a constant distance due to their mass and electric fields.
  • It is suggested that any bound system, including atoms and galaxies, does not expand due to the overwhelming strength of the forces holding them together compared to the weak cosmic expansion.
  • A thought experiment involving pennies on a balloon illustrates that bound objects do not increase in size despite the expansion of the surrounding space.
  • One participant introduces the Einstein-Strauss model, which posits that expansion occurs only outside certain vacuoles, but acknowledges criticisms of this model and its limitations in light of dark energy considerations.
  • There is a recognition that the effects of expansion on scales smaller than cosmological significance remain an open question in cosmology.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the effects of spacetime expansion on atomic scales, with no consensus reached on the matter.

Contextual Notes

Limitations include the dependence on definitions of expansion and the unresolved nature of how dark energy might influence atomic scales.

EskWIRED
Messages
99
Reaction score
0
I think that it is correct to say that everywhere, spacetime is expanding.

Is it expanding within the radius of electrons within atoms? Are the radii getting larger over time?

I believe it correct that the distance from the nucleus to an electron exceeds the diameter of either one by many orders of magnitude. So mostly the volume of an atom is composed of "empty space". Is that stuff in those locations expanding like any normal intergalactic space?
 
Physics news on Phys.org
We would not be able to measure the expansion because our rulers are expanding as well. Unless you are saying the space-time is not expanding homogeneously...
 
To the best of our knowledge, atoms do not partake in the expansion of the universe. The radius of an atom is proportional to the Bohr radius, ħ2/me2, and this depends only on the fundamental constants of nature. To considerable accuracy, these have not changed over the lifetime of the universe.
 
Bill_K said:
To the best of our knowledge, atoms do not partake in the expansion of the universe. The radius of an atom is proportional to the Bohr radius, ħ2/me2, and this depends only on the fundamental constants of nature. To considerable accuracy, these have not changed over the lifetime of the universe.

That makes sense, given that physical objects do not grow lager as the universe expands.

But I can't understand why not. What is different about the spacetime in the proximity of matter, making it such that it does not expand along with intergalactic space?
 
I didn't say the spacetime inside an atom was different. What I said was, the atom itself does not expand. The electron and nucleus are not pegged to particular locations in space and dragged along by the cosmic expansion. The atom remains the same size because the mass of the electron remains the same, and the electric field of the nucleus remains the same, so they remain (on average) a constant distance apart.

The same reasoning applies to any bound system, even a galaxy or a cluster of galaxies. They don't expand either.
 
Anything bound by any of the fundamental forces will overcome the expansion of the universe. This includes gravity, which is extremely weak. The expansion of the universe is even weaker.

The gravity within galaxies, and even between galaxies is easily strong enough to overwhelm the expansion. That's why the only place we observe this expansion is on huge scales, such as between galaxy clusters, where gravity is infinitesimally small.

Think of this thought experiment. Tape a dozen pennies in random places on a partially inflated balloon, then blow up the balloon. Do the pennies get larger? No. The forces holding each penny together are far, far larger than the expansion of the balloon.
 
The answer to the question isn't really known. For example in an Einstein-Strauss model, expansion only takes place place outisde of the vacuoles. As the vacuoles in this model are meant to represent stars and their surrounding space, in this model expansion only takes place inbetween stars.

However I think recently (the last decade or two) some criticisms have been made of the Einstein-Strauss model which means it should not be taken as a serious physical model of the Universe and secondly the model was conceived long before dark energy was postulated.

We might reasonably expect dark energy to act as a general repulsive influence on scales even as small as the atomic, on the other hand we have no way of knowing that that is the case.

All this just goes to underline the fact that it is still an open question in cosmology as to what exactly is the effect of expansion on scales smaller than what might be called 'cosmologically significant'.
 

Similar threads

  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 51 ·
2
Replies
51
Views
6K
  • · Replies 23 ·
Replies
23
Views
5K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 19 ·
Replies
19
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 14 ·
Replies
14
Views
3K
  • · Replies 27 ·
Replies
27
Views
4K
  • · Replies 4 ·
Replies
4
Views
5K