Do cosmologists take spontaneous symmetry breaking seriously?

In summary, the conversation revolves around the concept of spontaneous symmetry breaking and its role in cosmology. It is believed that the vacuum state of the early Universe underwent a sudden change, potentially similar to a second order phase transition. However, the exact nature and details of this transformation are still under investigation. Vacuum energy is also discussed, with some speculation about its effects on the expansion of the Universe. It is also suggested that there may be parts of the Universe that are not causally connected with ours, but they may have experienced similar vacuum states during inflation. The conversation ends with a discussion about the potential for quantitative predictions regarding spontaneous symmetry breaking and its relation to universal classes.
  • #1
Carlos L. Janer
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I suppose that my questions are pretty basic, but I've been trying to find out the answers and not succeeded.

1.- Do cosmologists really think that the vacuum state suddenly changed in the early Universe? If so, would it be like a phase transition? If so, first or second orther?

2.- Does the vacuum energy explain anything about the Universe expansion?

3.- Are there parts of the Universe that are not causally connected with ours? If so, did these other parts choose the same vacuum state as ours?

After all, Higgs boson has been experimentally found and spontaneous symmetry breaking can't be be as artificial as it seems to be.

I'm sorry for posting three questions at the same time but I don't really undestand if the Standard Model of particle physics plays any relevant role in Cosmology or not. If this is not the right place to make this questions could you, please, let me know where can I look for answers?
 
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  • #2
1. The concept of spontaneous symmetry breaking is taken seriously - the detaiils are pretty much up for grabs. The usual analogy is to a narrow cone balanced on it's point. Any small change in the mass distribution of the cone will cause it to fall over - it's orientation state moves from unstable to one of many possible stable (lying down) states. Spontaneous state changes are well observed in Nature, ie with nuclear decay and arises from the mathematics of quantum mechanics.
Some state changes or symmetry breaking is considered to be analogous to a state change in matter and the "order" that this is treated at depends on the model being constructed.

2. Vacuum energy (afaict) is usually considered to have a small if not negligible effect on the cosmological expansion. If there is any effect, it is expected to increase expansion. It's tricky since the precise nature of vacuum energy remains under investigation. (Also see "Hawking radiation" for another effect that could have cosmological implications.)
Since there are big unknowns here, you will find a lot of speculation online that boils down to an argument from ignorance: tread carefully.

3. If I understand you correctly... It appears that there must be parts of the Universe not causally connected to ours since best evidence to date suggests an infinite flat universe. That would be any part of the Universe beyond the cosmological horizon iirc. However, since physics needs to be continuous across that horizon (it's just an artifact of where we are as observers) then it seems reasonable that anyone at or near our horizon will not see anything different from what we do. Space-time there will be subject to the same boundary conditions and so you get the same energies via the same mathematics. It's kinda like this: when I stand on a high place by the shore, looking out over the Pacific, there is a limit to how far I can see: this is the horizon. It seems reasonable to suppose, without going there myself, that a ship approaching this horizon will not experience any change in sea level when they cross it and, if they do, it will not be anything to do with my horizon.
 
  • #3
Carlos L. Janer said:
Do cosmologists really think that the vacuum state suddenly changed in the early Universe?

Yes. The basic mechanism is described briefly on the Wikipedia page:

https://en.wikipedia.org/wiki/Spontaneous_symmetry_breaking

Carlos L. Janer said:
If so, would it be like a phase transition? If so, first or second orther?

AFAIK there is no latent heat associated with spontaneous symmetry breaking, so it would be more like a second order phase transition. However, I don't know that a specific order is given to this transition.
 
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  • #4
I don't really know what to think about all this. I guess I lack background knowledge but, if SSB were to be described by a second order phase transition, shouldn't it belong to one of the universality classes? Shouldn't we then have a detailed description of what really happened? I'm probably talking nonsense. If I am, I apologize in advance.
 
  • #5
As already noted symmetry breaking is demanded by modern cosmology. For a basic discussion see http://abyss.uoregon.edu/~js/ast123/lectures/lec18.html. Assuming the universe is spatially infinite, as suspected, there are regions of the universe that are causally disconnected from our observable universe. Yet, curiously enough, these regions may have been in causal contact with our universe prior to inflation. Vacuum energy in the modern, observable universe is either zero or incredibly close to zero [this is the favored point of view]. Under inflation, however, it should have been very large initially before undergoing a phase change at the end of inflation and relaxing to its current negligible value. Sean Carroll offers some discusion on this here https://www.preposterousuniverse.com/encyc.
 
  • #6
I think we're not all speaking about the same thing here. There seems to be some kind of language (jargon) barrier here. When I refer to spontaneous symmetry breaking I'm talking about the electroweak symmetry breaking, the only one that has a precise theoretical formulation and phenomenological proof in the Standard Model of particle physics. I was wondering if this SSB could be regarded as a second order phase transition because, if this were indeed the case, I'm inclined to think that this phase transition should belong to one of the universal classes and, therefore, quantitative predictions could, in principle, be made.
 
  • #7
Carlos L. Janer said:
I was wondering if this SSB could be regarded as a second order phase transition because, if this were indeed the case, I'm inclined to think that this phase transition should belong to one of the universal classes and, therefore, quantitative predictions could, in principle, be made.

Electroweak symmetry breaking has features in common with a phase transition (the term "electroweak phase transition" is sometimes used to describe it), but I don't know that the entire mathematical theory of it is exactly the same.

What sorts of quantitative predictions are you thinking of?
 
  • #8
As far as I know there's no mathematical proof, but it is widely believed that all 2nd order phase transitions do belong to one of the so called "universal classes". Universal classes depend only on very general properties of the Lagrangian density, such as number of dimensions and symmetries. Since the low energy (T=2.7 K) vacuum energy state is known, as well as the physical quantum fields (Standard Model of particle physics), I kind of expected that physicists had already figured out the university class electroweak SSB (or "EW phase transition") belonged to. I also kind of expected the high temperature (T>10^15 K) quantum fields (before EW-SSB) and the vacuum state to be known and its cosmological consequences also to be widely known.

Most probably I haven't been able to find that information because I'm an ignorant and my reasoning is completely flawed.
 
  • #9
The general consensus is electroweak symmetry breaking is a first order phase transition. See https://arxiv.org/abs/1401.1827, Higgs Couplings and Electroweak Phase Transition, and https://arxiv.org/abs/1604.04526, A First-Order Electroweak Phase Transition in the Standard Model from Varying Yukawas for discussion.
 
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  • #10
Carlos L. Janer said:
As far as I know there's no mathematical proof, but it is widely believed that all 2nd order phase transitions do belong to one of the so called "universal classes". Universal classes depend only on very general properties of the Lagrangian density, such as number of dimensions and symmetries. Since the low energy (T=2.7 K) vacuum energy state is known, as well as the physical quantum fields (Standard Model of particle physics), I kind of expected that physicists had already figured out the university class electroweak SSB (or "EW phase transition") belonged to. I also kind of expected the high temperature (T>10^15 K) quantum fields (before EW-SSB) and the vacuum state to be known and its cosmological consequences also to be widely known.

Most probably I haven't been able to find that information because I'm an ignorant and my reasoning is completely flawed.
I think the problem is that there are multiple possible high-energy configurations which may potentially have resulted in the current vacuum state. In short, we don't know the Langrangian that was active at the time of the symmetry breaking, which makes it rather difficult to make many statements.

To put a lot of this in more concrete terms, the nature of the spontaneous symmetry breaking events that happened in the distant past of our universe depends critically upon physics at higher energies than the standard model of particle physics currently describes.
 
  • #11
I would have expected that the physics described by the Standard Model above EW unification energies to be well known. I'm aware that there's no hope of any direct experimental confirmation, but I thought that, even though the energy extrapolation is really wild, it was a model that cosmologists could work with. It seems clear to me now that it's not. Sorry for wasting your time and thanks for your posts!
 
  • #12
Chronos said:
The general consensus is electroweak symmetry breaking is a first order phase transition.

I don't think these papers describe a "general consensus". I think they describe possible models for a first order transition, but those models require physics beyond the SM which has not (yet) been observed experimentally.

The first paper explicitly says, on p. 2:

If physics up to the TeV scale is completely described by the SM, it is well known that the electroweak phase transition (EWPT) is second-order

So any model including a first-order transition would have to go beyond the SM.
 
  • #13
Cosmologists certainly do take spontaneous symmetry breaking in the very early universe seriously and the concept of it being 'spontaneous' (in other words stochastic - 'by chance') is contingent on there being an infinite ensemble of other possible outcomes that inevitably lead to the concept of a multiverse.

The analogous example of a pencil standing on its point and then tipping over in one particular direction implies that it is free to fall in any other direction, and in our analogy these other directions represent the other universes with different physical properties that would arise out of the process.

There is a caveat here though.

Unless we have explicit proof that these other universes exist the concept of the multiverse has dubious value within science. For it to be something more than a speculative hypothesis we have to show that the symmetry breaking is truly spontaneous and not an example of an explicit symmetry breaking process. If it were the latter then there would be some physical process that made the universe turn out the way it has.

The problem with the hypothesis of spontaneous symmetry breaking in the very early universe, and its associated multiverse, is that we can explain everything and anything by it: anthropic coincidences, the physical nature of the observed universe etc. They have turned out this way in our universe, by chance, but It is otherwise in other universes.

The problem with this is that a hypothesis that explains everything and anything actually explains nothing and moreover short circuits the scientific inquiry that might have found the real reason for things being as they are.

Just a thought...
Garth
 
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  • #14
SSB has a very precise and different meaning in particle physics: it's the way in which the intermediate vector bosons (and, by extension, many of the rest of elementary particles) became massive. It's a well defined and experimentally proven hypothesis (Higgs boson and, therefore, Higgs field, do seem to really exist).

I'm not a physicists, just an engineer, but it really frightens me to see that high energy physicists and cosmologists can't understand each other. I'm not criticising it (the same thing happens in my own field), I'm just acknowledging a fact.

I sometimes think that specialization and the "publish or perish" paradigms are killing Science.
 
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  • #15
Carlos L. Janer said:
high energy physicists and cosmologists can't understand each other. I'm not criticising it (the same thing happens in my own field), I'm just acknowledging a fact.

What led you to make these uncharitable, unfair, and untrue statements.
 
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  • #16
Garth said:
Unless we have explicit proof that these other universes exist the concept of the multiverse has dubious value within science. For it to be something more than a speculative hypothesis we have to show that the symmetry breaking is truly spontaneous and not an example of an explicit symmetry breaking process. If it were the latter then there would be some physical process that made the universe turn out the way it has.
Argument from consequences. Just because spontaneous symmetry breaking implies things about the universe you don't like doesn't mean it isn't likely.

Explicit symmetry breaking processes are generically more complex than spontaneous symmetry breaking processes (as you need not only a mechanism to break a symmetry, but also a mechanism to break it in a specific way), and are therefore less likely.

More importantly, there were probably a large number of symmetry breaking events in the past of our universe, and it's highly unlikely that they all would be explicit.
 
  • #17
Chalnoth said:
Argument from consequences. Just because spontaneous symmetry breaking implies things about the universe you don't like doesn't mean it isn't likely.

Explicit symmetry breaking processes are generically more complex than spontaneous symmetry breaking processes (as you need not only a mechanism to break a symmetry, but also a mechanism to break it in a specific way), and are therefore less likely.

More importantly, there were probably a large number of symmetry breaking events in the past of our universe, and it's highly unlikely that they all would be explicit.
Obviously spontaneous symmetry breaking events take place, it's just when they are invoked in speculative theory about the very early universe to "predict" the existence of a multiverse that I have reservations.

Its not that I don't like the implication of a multiverse, it's just that I think its not very scientific.

We need to be transparent about when theory is founded on testable hypotheses and when it is simply building speculation upon speculation, as discussed by George Ellis in this article in 'Nature' Cosmology: The untestable multiverse.

Garth
 
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  • #18
Garth said:
Obviously spontaneous symmetry breaking events take place, it's just when they are invoked in speculative theory about the very early universe to "predict" the existence of a multiverse that I have reservations.

Its not that I don't like the implication of a multiverse, it's just that I think its not very scientific.

We need to be transparent when theory is founded on testable hypotheses and when it is simply building speculation upon speculation, as discussed by George Ellis in this article in 'Nature' Cosmology: The untestable multiverse.

Garth
Except what you wrote is that explicit symmetry breaking is the preferred default hypothesis because it doesn't lead to a multiverse.
 
  • #19
Chalnoth said:
Except what you wrote is that explicit symmetry breaking is the preferred default hypothesis because it doesn't lead to a multiverse.
Not because it doesn't lead to a multiverse but because the symmetry breaking process might have been explicit.

We haven't observed any of the other universes of the multiverse.

Therefore, if we explain features of the early universe simply by chance, by the stochastic process of spontaneous symmetry breaking, thereby requiring the ensemble of other non-observed possibilities, we may be missing the real physical reason why the universe has turned out the way it has.

I've no objection to doing this as long as we are transparent about the enormous implicit assumption (a multiverse) that has been surreptitiously adopted and the consequential short-circuiting of the scientific method.

Garth
 
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  • #20
An idea devoid of observational evidence lacks any tangible scientific basis.
 
  • #21
Chronos said:
An idea devoid of observational evidence lacks any tangible scientific basis.
I'm quite sure there are galaxies today at a distance of 35 billion light years. We can never observe them, because our future light cones do not intersect, so there is no observational evidence for their existence today.
We saw those galaxies forming earlier, however, and we can see the evolution of galaxies closer to us. Unless there is some magical galaxy-eating thing they should still exist.

If you have observational evidence for a theory (e. g. "galaxies form, and stay around for a while"), and this theory predicts something (e. g. "the galaxies at a distance of 35 billion light years are still around), then you can still discuss those implications of the theory in a scientific way, even if you cannot observe some of them.
 
  • #22
mfb said:
We saw those galaxies forming earlier, however, and we can see the evolution of galaxies closer to us.
In which case I would not call such galaxies beyond our light cone "devoid of observational evidence".

Exactly what observational evidence is there for other universes?

Garth
 
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  • #23
Garth said:
In which case I would not call such galaxies beyond our light cone "devoid of observational evidence".
Okay.
Garth said:
Exactly what observional evidence is there for other universes?
If we can find evidence for things like eternal inflation, then this theory predicts the existence of other regions which could be called "different universes". If SSB happens within those universes, then different universes will have different laws of physics. Same thing as with the galaxies, just on an earlier timescale.
 
  • #24
mfb said:
If we can find evidence for things like eternal inflation, then this theory predicts the existence of other regions which could be called "different universes". If SSB happens within those universes, then different universes will have different laws of physics. Same thing as with the galaxies, just on an earlier timescale.
Agreed - but that is a big "if". Primordial B-Mode polarisation in the BICEP 2 data perhaps? :wink:

Garth
 
  • #25
Carlos L. Janer said:
SSB has a very precise and different meaning in particle physics: it's the way in which the intermediate vector bosons (and, by extension, many of the rest of elementary particles) became massive.
No, that is specifically the electroweak phase transition that happens to involve the spontaneous (as Garth says above, "by chance") breaking of the electroweak gauge symmetry. SSB is a general phenomenon referring to any such "chance" breaking of symmetry, whether it be in the formation of domain walls in the freezing of water to form ice, the falling of a pencil perched at its tip, or the reduction in gauge symmetry enjoyed by a sector of the Standard Model.

There is no separate language between cosmologists and high energy folk: in fact, they are quite integrated fields.
 
  • #26
I object to the claim
mfb said:
... there is no observational evidence for their existence today.
applied to galaxies at 35 gly distant.

Galaxies exiting our cosmological horizon resemble bob falling into a black hole as viewed by alice - they redshift into obscurity, but, never appear to cross the EH. I would argue such galaxies are still detectable with sufficiently sensitive instruments. Unless, of course, you are prepared to argue there is no observational evidence for the existence today of galaxies currently beyond about z=2 [re: Davis and Lineweaver, Expanding Confusion]. The big problem with 'other' universes under multiverse theories [at least in the versions with which I am familiar] is they were born causally disconnected from 'our' universe, otherwise I would argue relics of their interactions with 'our' universe would still, in principle, be observationally accessible.
 
  • #27
Garth said:
Not because it doesn't lead to a multiverse but because the symmetry breaking process might have been explicit.

We haven't observed any of the other universes of the multiverse.
The problem is that you're promoting the concept of a unique universe to the status of a default hypothesis. There's no good reason for that.

"The universe has the same physical laws everywhere outside our horizon" is every bit as non-observable as the idea of a multiverse. Worse, a unique universe generically requires more assumptions than a diverse one. So what you're saying is that it's better to admit the additional assumptions required to get a unique universe (in this case explicit symmetry breaking) just because it doesn't lead to a multiverse.

In other words, you seem to be focusing on the conclusion rather than the argument that leads up to it. If we examined high-energy physics, given current knowledge, and asked, "Are there spontaneous symmetry breaking events?" The answer seems to be almost certainly yes. There might be some explicit symmetry breaking, but there's no reason to believe that all symmetry breaking events in our past were explicit. There is no reason whatsoever to even consider whether or not there is a multiverse when thinking through this, and bringing it into the discussion of whether there was explicit or spontaneous symmetry breaking is specious.
 
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  • #28
Chalnoth said:
The problem is that you're promoting the concept of a unique universe to the status of a default hypothesis. There's no good reason for that..
Really? I would have thought any scientist would have said the fact that we can presently observe our universe (unique or not) but not any others would be quite a good reason...

Garth
 
  • #29
Chronos said:
Unless, of course, you are prepared to argue there is no observational evidence for the existence today of galaxies currently beyond about z=2
That is exactly what I said.
We see them in their earlier stages, and we have theories that predict that the galaxies are still around, but we cannot see them in their current state (13.7 Gy after the big bang).
Chronos said:
The big problem with 'other' universes under multiverse theories [at least in the versions with which I am familiar] is they were born causally disconnected from 'our' universe, otherwise I would argue relics of their interactions with 'our' universe would still, in principle, be observationally accessible.
You can easily extend that example to matter a few meters behind the particle horizon. Is there matter? Well, probably. It would be extremely odd if the universe would end right at our (Earth) range of causal interaction.
 
  • #30
Garth said:
Really? I would have thought any scientist would have said the fact that we can presently observe our universe (unique or not) but not any others would be quite a good reason...
Again, you're arguing the conclusion rather than considering the models that would lead to the conclusion.

Whether or not there are different regions with different low-energy laws of physics depends upon the underlying physical laws. If there are spontaneous symmetry breaking events, such that the vacuum has either multiple metastable local minima or has a class of degenerate states, then those laws of physics generically give rise to different regions with different low-energy laws of physics.

If, on the other hand, the underlying potential is relatively steep and monatonic, so that we don't have degenerate states or many metastable local minima, and the universe we observe is right at the global minimum of the vacuum energy, then there very likely would not be any other regions of space-time with different low-energy physics.

What you're saying is that until we have evidence to point one way or the other, we should always prefer the second set of models, because it predicts a unique universe. And I'm sorry, but I really don't think that's good science.
 
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  • #31
mfb said:
That is exactly what I said.
We see them in their earlier stages, and we have theories that predict that the galaxies are still around, but we cannot see them in their current state (13.7 Gy after the big bang).You can easily extend that example to matter a few meters behind the particle horizon. Is there matter? Well, probably. It would be extremely odd if the universe would end right at our (Earth) range of causal interaction.

I'm really not seeing your point. Evidence of past causal interaction is as good as it gets. Even light from the sun is causally removed from us by about 8 minutes, and I'm unaware of any doubts about causal connections between the Earth and sun.
 
  • #32
mfb said:
but we cannot see them in their current state (13.7 Gy after the big bang).
This is based on a particular foliation of space-time with cosmological time determining what is "current". The coordinate independent statement is that the object at some point passes a horizon. There is nothing particularly special about your choice of "current".
 
  • #33
Chronos said:
I'm really not seeing your point. Evidence of past causal interaction is as good as it gets. Even light from the sun is causally removed from us by about 8 minutes, and I'm unaware of any doubts about causal connections between the Earth and sun.
We can test the hypothesis "the sun is still there" in 8 minutes from now.
Orodruin said:
This is based on a particular foliation of space-time with cosmological time determining what is "current".
Yes, and it should be clear from the context what I mean.Edit: I think this is getting off-topic.
 
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  • #34
Chalnoth said:
Again, you're arguing the conclusion rather than considering the models that would lead to the conclusion.

Whether or not there are different regions with different low-energy laws of physics depends upon the underlying physical laws. If there are spontaneous symmetry breaking events, such that the vacuum has either multiple metastable local minima or has a class of degenerate states, then those laws of physics generically give rise to different regions with different low-energy laws of physics.

If, on the other hand, the underlying potential is relatively steep and monatonic, so that we don't have degenerate states or many metastable local minima, and the universe we observe is right at the global minimum of the vacuum energy, then there very likely would not be any other regions of space-time with different low-energy physics.

What you're saying is that until we have evidence to point one way or the other, we should always prefer the second set of models, because it predicts a unique universe. And I'm sorry, but I really don't think that's good science.

What I am saying is that, without evidence, the hypothesis of a multiverse based on the assumption of the characteristics of this universe being determined solely by a stochastic process is not good science.

And I'm not the only one Are Parallel Universes Unscientific Nonsense? Insider Tips for Criticizing the Multiverse (Max Tegmark), Paul Steinhardt Disowns Inflation, the Theory He Helped Create (Paul Steinhardt).

As Paul says, (in the Inflation + Landscape scenario giving rise to Level II parallel universes,) with an enormously flexible Inflation theory and ~10500 varieties of String theory one can explain anything and everything - but such theories don't actually explain anything while giving the false impression that they do.

Garth
 
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  • #35
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Edit: the thread will remain closed.
 
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1. What is spontaneous symmetry breaking in cosmology?

Spontaneous symmetry breaking is a concept in cosmology that explains how the universe transitions from a state of symmetry to a state of asymmetry. It is believed to have occurred during the early stages of the universe's formation, and is responsible for the formation of the different fundamental forces and particles we observe today.

2. How does spontaneous symmetry breaking affect our understanding of the universe?

Spontaneous symmetry breaking is an important concept in cosmology because it helps us understand how the fundamental forces and particles in the universe came to be. It also provides a possible explanation for the unequal distribution of matter and antimatter in the universe, and the formation of cosmic structures such as galaxies and clusters.

3. Is there evidence to support the theory of spontaneous symmetry breaking?

Yes, there is strong evidence to support the theory of spontaneous symmetry breaking. One of the most significant pieces of evidence is the discovery of the Higgs boson, which is a particle predicted by the theory of spontaneous symmetry breaking. Additionally, observations of the cosmic microwave background radiation and the distribution of matter in the universe also support the concept.

4. Are there any alternative theories to explain the phenomena of spontaneous symmetry breaking?

Yes, there are alternative theories that attempt to explain the same phenomena as spontaneous symmetry breaking. For example, the theory of inflation suggests that the universe underwent a rapid expansion in the early stages, which could also explain the formation of the different fundamental forces and particles we observe today.

5. How does the concept of spontaneous symmetry breaking tie in with other theories in cosmology?

Spontaneous symmetry breaking is closely tied to other theories in cosmology, such as the Big Bang theory and inflation theory. It is also related to the concept of symmetry breaking in particle physics. These theories work together to provide a comprehensive understanding of the universe and its evolution from the early stages to the present day.

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