Issues regarding the expansion of the Universe at the subatomic level

In summary, the conversation discusses the expansion of the universe and its effects on different scales. The speaker suggests that the expansion may be happening at a subatomic level and could be measured by the distance between quarks. However, another participant points out that on small scales, other forces such as gravity and electromagnetism overpower the effects of expansion. The conversation also touches on the purpose of CERN and the role of gravity at the subatomic scale. Ultimately, it is concluded that the expansion of the universe does not take place at the subatomic level, but rather on larger scales.
  • #1
habarnam
2
0
Sorry for my bad English and mostly for my bad Physics.
For me it doesn't make any sense regarding the expansion of the Universe as a distant process, a sort of time&space machine which 'degulfs' more room for the known things to occupy. My guess is the expansion is happening here now at a subatomic level and it swells matter, distancing the quarks from each other within the hadron, forcing gluons to attempt linking their more and more distant quarks (and having this confinement condition as a safety measure against proton disintegration).
This could mean that the age of the Universe could be measured according to the distance between quarks. If space-time fabric has the structure of a net, its constant number of nodes get farther from each other and the ridges get longer, so the speed of light is a constant if measured by nodes but a variable if we measure the real distance it covers per time unit. Moreover, if a proton indicates the distance in time from the Big Bang by its size, maybe if one could shrink a proton to a previous size, it will necessarily transpose itself in that past moment when all the protons had this size. It's like the standard meter from Paris is getting longer each split-second. This also could lead to a critical moment when protons will break at an exponential rate and all the matter in the Universe will be shred by the tension of the space-time mesh.
How am I wrong here? I guess I must be awfully wrong, given my poor knowledge (which is hardly past the high school level and some books for dummies).
 
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  • #2
I'm fairly certain that the other fundamental forces are enough to nullify expansion. So the Earth doesn't get further from the sun due to gravity holding them together and atoms in molecules don't get further away due to electromagnetic interaction.

Hopefully an expert will wander by to confirm this.
 
  • #3
Ryan_m_b said:
I'm fairly certain that the other fundamental forces are enough to nullify expansion. So the Earth doesn't get further from the sun due to gravity holding them together and atoms in molecules don't get further away due to electromagnetic interaction.

Hopefully an expert will wander by to confirm this.

This is right. Gravitationally bound systems overcome the force of expansion on the local scale. (Local planetary systems, star systems, galaxies and clusters.) On the large scale expansion wins out but on the small scale gravity is king.
 
  • #4
habarnam said:
Sorry for my bad English and mostly for my bad Physics.
For me it doesn't make any sense regarding the expansion of the Universe as a distant process, a sort of time&space machine which 'degulfs' more room for the known things to occupy. My guess is the expansion is happening here now at a subatomic level and it swells matter, distancing the quarks from each other within the hadron, forcing gluons to attempt linking their more and more distant quarks (and having this confinement condition as a safety measure against proton disintegration).
This could mean that the age of the Universe could be measured according to the distance between quarks. If space-time fabric has the structure of a net, its constant number of nodes get farther from each other and the ridges get longer, so the speed of light is a constant if measured by nodes but a variable if we measure the real distance it covers per time unit. Moreover, if a proton indicates the distance in time from the Big Bang by its size, maybe if one could shrink a proton to a previous size, it will necessarily transpose itself in that past moment when all the protons had this size. It's like the standard meter from Paris is getting longer each split-second. This also could lead to a critical moment when protons will break at an exponential rate and all the matter in the Universe will be shred by the tension of the space-time mesh.
How am I wrong here? I guess I must be awfully wrong, given my poor knowledge (which is hardly past the high school level and some books for dummies).


i like this..

i often feel looking in rather than out is the way
 
  • #5
Habarnam,

The "dark energy" that causes the expansion of the universe is VERY weak on small scales and systems such as atoms and galaxies that are bound by strong/weak/gravity forces are NOT affected by it.

It is like an ant pushing on a house. You might think that it has a tiny effect that could add up over time, but that is not correct. It has NO effect.

On REALLY LARGE scales (billions of light years of distance) the cumulative effect of dark energy has a large effect.
 
  • #6
lostprophets said:
i like this..

i often feel looking in rather than out is the way

The way to where/what? We cannot observe expansion at the subatomic scale. Period. So we learn nothing about it by doing so. Similarly we didn't learn about gravity by looking at the subatomic scale because, like expansion, the other forces are many many orders of magnitude stronger at that scale.
 
  • #7
Drakkith said:
Similarly we didn't learn about gravity by looking at the subatomic scale because, like expansion, the other forces are many many orders of magnitude stronger at that scale.

I guess we did, because it happens in black holes and armies of physicists try to 'look' for the gravity at the subatomic scale.
And, if I'm not wrong, the main purpose of CERN these days is exactly to probe gravity at small scales.
 
  • #8
We cannot observe expansion at the subatomic scale

We do observer expansion from the subatomic scale how else do you explain light? :confused:
 
  • #9
petm1 said:
We do observer expansion from the subatomic scale how else do you explain light? :confused:

What they mean is that the expansion of the universe does not take place on small scales. Distances between subatomic particles are not increasing. It's only on scales of galaxy clusters and larger that objects are moving away from each other.

Your question about light is a bit too vague for me to address.
 
  • #10
habarnam said:
I guess we did, because it happens in black holes and armies of physicists try to 'look' for the gravity at the subatomic scale.

We are trying to learn about gravity at that scale now, but our current and previous main theories on gravitation did not. (GR and Newtonian)

And, if I'm not wrong, the main purpose of CERN these days is exactly to probe gravity at small scales.

I don't believe so. CERN has multiple experiments running, one of the main is the LHC, who's "main" purpose is searching for new particles such as the higgs and trying to understand why antimatter is so much less dominant than normal matter in the universe. If quantum gravity is involved I doubt that it is its "main" purpose.
 
  • #11
What they mean is that the expansion of the universe does not take place on small scales. Distances between subatomic particles are not increasing. It's only on scales of galaxy clusters and larger that objects are moving away from each other.

A photon even when thought of as a packet of energy is subatomic, and when we measure it as "longer" we think of space expanding because the photon is older. This is a measure of distances between subatomic particles increasing. :confused:
 
  • #12
petm1 said:
A photon even when thought of as a packet of energy is subatomic, and when we measure it as "longer" we think of space expanding because the photon is older. This is a measure of distances between subatomic particles increasing. :confused:

We can measure red-shifts of distant galaxies. And such galactic red-shifts are caused by the wave crests (and troughs) slowly spreading apart, due to expansion, as the light wave traveled through the gradually expanding cosmos. This cosmic expansion has the effect of increasing a photon's wavelength. So yes, that's kind of on a microscopic scale. But I would not say that it is due to the distance between subatomic particles increasing. The crests and troughs of a given photon are not individual particles.

But particles that are interacting due to other forces (such as in the case of solids, liquids, solar systems, etc.) are overwhelmed by the other forces compared to whatever force is causing [edit: accelerated] expansion.

For example, take a meter stick and place one hand near each end and try to pull it apart. Give it a good yank, and try to stretch the meter stick making it longer. If you're only using your hands and arms, it probably won't budge. What's keeping it together? Essentially, it's the electromagnetic force in this case (it also involves the minutia of atomic bonds between atoms and molecules, but these bonds are ultimately a manifestation of the electromagnetic force, is my point). Pull on that meter stick until you're 100 years old, and it's not going to make a difference. Find a way to keep it up for 10 billion years and that meter stick still won't pull apart (ignoring things like corrosion, fire, natural disasters, etc.)

The force you're applying with your arms is many, many orders of magnitude greater than the cosmic expansion force acting on that meter stick. So if you are not able to increase the length of the meter stick (with your hands and arms), the expansive force certainly won't either.
 
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  • #13
phinds said:
Habarnam,

The "dark energy" that causes the expansion of the universe is VERY weak on small scales and systems such as atoms and galaxies that are bound by strong/weak/gravity forces are NOT affected by it.

It is like an ant pushing on a house. You might think that it has a tiny effect that could add up over time, but that is not correct. It has NO effect.

On REALLY LARGE scales (billions of light years of distance) the cumulative effect of dark energy has a large effect.

I strongly agree with you. Its so weak that the expansion is termed by a fraction of 1 followed by 100 zeros. If its anything less than that, then our universe will shrink away and anything greater causes the disappearance of universe within seconds. Its constant. But, the wonder here is that Even though the expansion rate is constant, the universe expansion is not slowing down. In fact, its accelerating towards its edges. That led to the theory of Inflation.

You are right bro. Gravity is never, of course negiligibly, effected by the dark energy. It only pushes one part of matter away from another unlike gravity, but doesn't break the fundamental part of the matter. I am not sure on this, because its not yet experimented or theorized to full extent. Super symmetry theory discusses this better
 
  • #14
sheshank said:
I strongly agree with you. Its so weak that the expansion is termed by a fraction of 1 followed by 100 zeros. If its anything less than that, then our universe will shrink away and anything greater causes the disappearance of universe within seconds. Its constant. But, the wonder here is that Even though the expansion rate is constant, the universe expansion is not slowing down. In fact, its accelerating towards its edges. That led to the theory of Inflation.

Prior to the bolded part, you are referring to the accelerated expansion of the universe. Inflation is a totally different thing ... something that happened in a very early and very tiny fraction of the first second after the singularity.
 
  • #15
phinds said:
Prior to the bolded part, you are referring to the accelerated expansion of the universe. Inflation is a totally different thing ... something that happened in a very early and very tiny fraction of the first second after the singularity.

I don't think so. I read that Inflation theory is also extended to explain the concept of ever accelerating universe. Look at wikipedia to avoid confusions. I don't think wikipedia can get confused like me. I watched a documentary (The Fabric of Cosmos), which said the same. Check it out.
 
  • #16
Wiki agrees w/ me:

In physical cosmology, cosmic inflation, cosmological inflation or just inflation is the theorized extremely rapid exponential expansion of the early universe by a factor of at least 1078 in volume, driven by a negative-pressure vacuum energy density.[1] The inflationary epoch comprises the first part of the electroweak epoch following the grand unification epoch. It lasted from 10−36 seconds after the Big Bang to sometime between 10−33 and 10−32 seconds. Following the inflationary period, the universe continued to expand, but at a slower rate.

The term "inflation" is also used to refer to the hypothesis that inflation occurred, to the theory of inflation, or to the inflationary epoch. The inflationary hypothesis was originally proposed in 1980 by American physicist Alan Guth, who named it "inflation".[2] It was also proposed by Katsuhiko Sato in 1981.[3]
 

1. What is the subatomic level and how does it relate to the expansion of the universe?

The subatomic level refers to the realm of particles and interactions that occur on a scale smaller than an atom. This level is important in understanding the expansion of the universe because it allows us to study the fundamental building blocks of matter and their behavior.

2. How does the expansion of the universe affect subatomic particles?

The expansion of the universe does not directly affect subatomic particles. However, it does influence the space in which these particles exist, causing it to stretch and expand over time. This expansion can impact the behavior and interactions of these particles.

3. What role do quantum mechanics play in understanding the expansion of the universe at the subatomic level?

Quantum mechanics is essential in understanding the behavior of subatomic particles and their interactions. It allows us to study the universe at the smallest scales and provides insights into how particles may behave in the expanding universe.

4. How does the expansion of the universe impact the formation of subatomic particles?

The expansion of the universe can impact the formation of subatomic particles in several ways. For example, as the universe expands, it cools down, which can affect the energy levels of particles and influence their formation. Additionally, the expansion can also impact the density of matter in the universe, which can affect the likelihood of particle interactions and formation.

5. Are there any ongoing studies or experiments exploring the expansion of the universe at the subatomic level?

Yes, there are ongoing studies and experiments examining the behavior of subatomic particles in the expanding universe. For example, the Large Hadron Collider at CERN is colliding particles at high energies to test theories about the fundamental nature of matter and the expansion of the universe. Other experiments, such as the IceCube Neutrino Observatory, are also studying the behavior of subatomic particles in the vastness of space.

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