Changing shape of calabi-yau manifolds: flop transitions

In summary, according to the author, it is possible to shrink the size of the universe by transitioning from a larger universe to a smaller universe through a series of flop transitions. This theory is based on the idea that the properties of the space, described by the metric, are a result of the fluctuations of closed-string graviton states. However, this theory is still incomplete and has many unresolved problems.
  • #1
dhillonv10
84
0
Hi all,

I was reading a paper written by Brian Greene sometime ago on flop
transitions where one can essentially change the topology of the
manifold but the four-dimensional physics that applied to the older
manifold still holds. From that I am trying to extrapolate the
following: Is it possible that through a series of flop transitions
one can end up with a calabi-yau manifold that is smaller in size
than the one with which we started off from? If that's possible,
then from there we can say that since strings make up the surface
of the manifold, they too will shrink in size or distort in shape
to accommodate for the changing shape of the manifold. Does my
argument make sense? Please feel free to correct me where I am
making mistakes. Thanks :)

- Vikram
 
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  • #2
The size and shape of the compact dimensions are dynamical properties anyway, even before you consider complicated effects like flop transitions. Are you familiar with the idea of a closed universe in general relativity, and how it can expand or contract? It's the exact same phenomenon. The radius of an extra dimension in string theory can increase or decrease dynamically, and this is a major, major issue for the particle physics side of string theory, because the particle properties (masses, charges, etc) are supposed to be set by the extra dimensions, and so the extra dimensions have to be geometrically stable somehow. The relevant properties (size and shape of the extra dimensions, location of branes in the extra dimensions) are called "moduli", and this is the issue of "moduli stabilization": If the moduli changed, particle physics would change drastically, and that contradicts the observed regularity of physical law, not just in experiments on Earth, but as observed on cosmic scales of time and space. So for the time since the big bang, and at least across the billions of light-years of the observed universe, some effect has to be keeping the moduli stable.

The main idea (though not the only one) is that there are electromagnetism-like fields which take nonzero values all the way around some of the extra dimensions. Under the right conditions, they will stabilize the size of the extra dimensions at a finite radius/area/volume, preventing them from expanding to infinity or collapsing to zero. These scenarios are studied under the name of "flux compactifications".

You talked about strings changing size when the extra dimensions change size too. Here we need to distinguish between a string as something that moves through a space, and strings as objects which collectively make up the space. The first part is the easier part of string theory (relatively speaking). The properties of the space are treated as a fixed background independent of the strings, and then you just study how the strings move and interact in that background.

As for the second part, that's probably best described by string field theory, which has a lot of unsolved problems. But let me at least say how I think about this. An individual string has many distinct possible states of excitation. For the closed string, one of these is the graviton. In quantum field theory, there is a standard way to build up a field state as a superposition of many particle states. Basically, the classical waves in the field are built up from the wavefunctions of many many particles. Ever since Einstein, gravity is described geometrically, by the metric tensor, but it is also a type of field, and so the variations in the metric tensor (gravity wells, gravitational waves, etc) can be understood in this way as coherent superpositions of many "graviton wavefunctions". The quantum theory of gravitons as point particles is problematic, but that was the big attraction of string theory - the extra detail of stringlike internal structure inside all "particles" ameliorated the problems.

So, the geometry of space, as described by the metric, ought to be understood as a big coherent quantum sum of closed-string graviton states. It is a little as if there were closed strings everywhere in space, but because it's a quantum sum, it's a statement about probabilities of what the closed strings are doing everywhere. I also want to add that the electromagnetism-like fields appearing in the flux compactifications also derive from the closed strings - in the same way, but in a different sort of excited state, not a graviton state.

In other words, the background through which strings move in the "easy" version of string theory (perturbative string theory) ought itself to have a description in terms of strings, in the "hard" version of string theory (string field theory or some other approach). The metric of the extra dimensions, the "fluxes", the "branes", can all be expressed as quantum sums of very large numbers of strings, exhibiting coherent collective behavior. And you can go a long way towards realizing this ambition, but not all the way, not yet anyway. So what I'm saying is that if you ask, how do the strings change when the extra dimensions change, that's a very different question for a string in the "foreground" and a string in the "background".

I'd also better emphasize that a lot of what I'm saying, comes from a general understanding of how this all works, rather than from intimate acquaintance with the specific technical problems of representing branes in string field theory, and so on. There may be someone out there who can speak more accurately and authoritatively about the deeper issues.

P.S. And speaking of deeper issues, thinking about this question made me realize a very basic deficiency in my own understanding, to do with https://www.physicsforums.com/showthread.php?t=419450&page=21#post2934361". T-duality swaps radius R for radius 1/R, and swaps the (quantized) momentum of the string along the closed direction with the winding number of the string along that direction - OK. But it hadn't quite dawned on me what this means for space-time distance. Yes, we can interpret this to mean that there's a smallest distance, because when R is less than "one", it's equivalent to a situation in a dual theory with R greater than "one". But how exactly do you translate that intuition into something at the level of operators and measurements? Is there a T-duality-invariant, operational definition of length which applies on both sides of the duality? It seems like it should relate to what I've called the hard part of string theory, where you understand everything metrical in terms of closed string field theory.
 
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  • #3
thanks a lot for your valuable reply, to be precise i was talking about the strings that make up an object, perhaps i should have written that in the original message :) but any how from what i understand, flop transitions are simply topological changes, but what i wanted to inquire was that whether during these changes, does the volume change? Here's some text from a book I am currently reading:

"Aspinwall, Greene, and Morrison wanted to know whether something like a
flop transition could occur in nature and whether space itself would rip apart,
despite general relativity’s picture of a smoothly curved spacetime that is not
prone to rupture. Not only did the trio want to determine whether this type of
transition could occur in nature, they also wanted to know whether it could
occur in string theory.

To find out, they took a Calabi-Yau manifold with a sphere (rather than foot-
ball) sitting inside it, put it through a flop transition, and used the resultant
(topologically altered) manifold to compactify six of spacetime’s ten dimensions
to see what kind of four-dimensional physics it yielded. In particular, they
wanted to predict the mass of a certain particle, which, in fact, they were able
to compute. They then repeated the same process, this time using the mirror
partner of the original Calabi-Yau space. In the mirror case, however, the sphere
did not shrink down to zero volume as it went through the flop transition. In
other words, there was no tearing of space, no singularity; the string physics, as
Greene puts it, was “perfectly well behaved.”14"

This states that the sphere must have decreased in volume. That's where the ambiguity lies...
 
  • #4
The issue here is what is meant by "volume". In string theory notions of ordinary geometry become modified at small distances. By carefully investigating as to what the proper definition of volume is, it turns out that it does not shrink to zero size. This is because it is corrected by non-perturbatiive instanton effects that become strong and dominant in this regime. One wouldn't know about this were it not for mirror symmetry: it allows to map the situation to another one which gets no quantum corrections and is exactly computable. By mapping back one can thus infer what happens to the geometry in a deeply quantum regime.
 
  • #5
Yes I see your point there, so how about a re-phrase of the question: say for instance it was possible to change the "quantum volume" of a calabi-yau manifold, then it makes sense that you can shrink it through a flop transition, right?
 
  • #6
Morally speaking, right...the volumes of the various cycles can be changed by changing the Kahler moduli, and despite the "classical" volumes appear to shrink to zero size, the quantum corrected do not. That's an example of resolution of singularities by quantum effects.
 

1. What is the significance of studying the changing shape of Calabi-Yau manifolds?

The study of Calabi-Yau manifolds is crucial in understanding the mathematical structure of string theory, which is a theoretical framework for describing the fundamental building blocks of the universe. The changing shape, or flop transitions, of these manifolds can provide insights into the behavior of strings and their interactions.

2. What are Calabi-Yau manifolds and why are they important in physics?

Calabi-Yau manifolds are complex, six-dimensional spaces that play a central role in string theory. They are important because they provide a geometric framework for unifying the theories of general relativity and quantum mechanics, and offer a potential explanation for the four fundamental forces of nature.

3. How do flop transitions occur in Calabi-Yau manifolds?

Flop transitions occur when certain geometric properties of a Calabi-Yau manifold change abruptly, resulting in a different topological structure. This can happen when there is a change in the complex structure or the Kähler structure of the manifold.

4. What are the implications of flop transitions in string theory?

Flop transitions can have significant implications in string theory, as they can change the behavior and properties of strings. They can also lead to the emergence of new particles and interactions, providing a deeper understanding of the fundamental building blocks of the universe.

5. How does the study of flop transitions in Calabi-Yau manifolds contribute to our understanding of the universe?

The study of flop transitions in Calabi-Yau manifolds can contribute to our understanding of the universe by providing insights into the structure and behavior of strings and their interactions. It also offers a potential avenue for unifying the theories of general relativity and quantum mechanics, which could ultimately lead to a more complete understanding of the fundamental laws of nature.

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