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Locality and Deformations in Conformal Field Theories

Investigating how small changes affect properties of deformed conformal field theories.

Ruben Monten, Richard M. Myers, Konstantinos Roumpedakis

― 10 min read


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In the world of physics, there's a concept called "deformed conformal field theories" or CFTs. Imagine we're looking at these theories and how they behave when we make small changes to them. We're diving into the nitty-gritty of how these deformations can affect the properties of the theories, especially when it comes to locality-basically, whether things can interact with each other at a distance versus needing to be close together.

Our main focus is on understanding how these changes fit within a specific framework called Perturbation Theory. It's a method that helps us deal with small changes in complex systems without getting too tangled up. So, what's the deal with our findings?

First off, we managed to find a Hamiltonian Operator that works well with these deformed theories. This operator lets us map out the energy levels, which is quite handy. It turns out this operator is not just any operator; it’s also got some special features that help maintain the locality of the theory. Yet, there's a twist: this Hamiltonian isn't set in stone. There are some free parameters we can play around with, and they don't mess up the good stuff we’re trying to keep.

Next, we tackled the full conserved Stress Tensor, another crucial component in physics. This tensor gives us information about the flow of energy and momentum in our theory. Interestingly, there are certain charges-think of them as Conservation Laws-that stick around even when we make our changes. However, they start off not being local, meaning they can’t just act like your friendly neighborhood superhero saving the day from any distance. But with some clever moves, we can make them local!

Introduction and Summary

At this point, let’s step back and look at where we are. There's a brilliant piece of work by someone named Zamolodchikov. This work shows us how to generate deformations of two-dimensional quantum field theories. Now, what's important here is that these deformations, while they may seem irrelevant, still allow us to learn a lot about the original theories.

One of the main benefits is that we can directly calculate things like energy levels and how particles interact with one another in these deformed theories. This has made a big impact on various areas in theoretical physics, like string theory and understanding integrable systems. Our main goal is to dig deeper into the locality issues related to these deformed theories.

You see, while these deformed theories can behave wildly at short distances, they can be perfectly well-behaved at larger distances. So, we call them "quasi-local," meaning they only hang out nicely when you give them enough space. Our mission is to see how these deformations are structured and whether we can find ways to keep them local-even if it takes some work.

We zeroed in on the deformation of two-dimensional CFTs and used perturbation theory to calculate the Hamiltonian and stress tensor up to third order in the deformation parameter. This means we took it step by step, looking at the changes in the system as small tweaks were made.

As we progressed, we realized that the operator we were working with-let’s call it the "deformed operator"-wasn't straightforward. It had some surprising terms that we hadn’t seen before, and many of these terms are crucial for getting the correct energy spectrum. And just when we thought we had it all figured out, we found out that our Hamiltonian isn’t fixed.

It's got free parameters, which means we have options when it comes to how we write it. This might sound like we can just play around, but it’s a big deal. These choices can change the theory, but only in ways that don’t break the properties we care about.

How Does It Fit Together?

Let’s take a closer look at the main ideas we’ve touched on. The deformed theories behave differently at short distances compared to long distances, and this is tied up with how we define things like the stress tensor.

We used a standard method to define our deformation, which relates to the energy momentum tensor of the deformed theory. This involves some mathematical juggling, but at the end of the day, it leads us to meaningful conclusions.

Zamolodchikov’s work shows that certain quantities have a universal property, meaning they can be computed regardless of how we handle the math. This is a real gem because it means we can make predictions about the theory without getting bogged down in the details of how we fixed our equations.

So, we checked the energies and found that the operator we came up with aligns nicely with what we expect from Zamolodchikov’s results. This was a pleasant surprise, confirming that we were on the right track. However, not all aspects were straightforward.

When we looked at the full Hamiltonian, we realized it had terms that could mess with our calculations. This complexity is a reminder of how tricky theoretical physics can be.

Navigating through the Uncertainty

The challenge doesn’t end there. It turns out, while our Hamiltonian provides a way to understand energy levels, the stress tensor complicates things further. The demands for the stress tensor to be conserved are high, and they don’t always line up with the Hamiltonian in the way we’d like.

As we explored this relationship, we found that the KdV Charges-another layer of conservation-related goodies-could also be affected. They’re essential for ensuring that the whole theory remains integrable. This means that we could potentially maintain regularity in how particles behave over time, even with our deformations in play.

The added layers mean we have to be careful. Each bit we calculate has the potential to shift our understanding and lead us into new territory.

Building the Deformed Hamiltonian

Our primary goal was to construct the deformed Hamiltonian operator through small steps. This meant working through the Hilbert space of our original CFT and crafting an operator that preserves local properties.

We decided to make an auxiliary operator-the “fake” Hamiltonian-first. Now, don’t get too hung up on the name. It’s just a way to build a solid foundation before we tackle the real deal. This fake Hamiltonian is important because it’s easy to handle; it sets us up for more sophisticated calculations later.

It’s non-local, which means it doesn’t fit the neat local definition we want. However, it allows us to maintain control, which is crucial for our end goal.

Once we had this foundation, we could start looking at how to relate it to our desired local Hamiltonian, ensuring we preserve the spectrum we were chasing after while moving through the deformations.

The All-Important Unitary Transformation

A major part of our endeavor involves something known as a unitary transformation. Essentially, it’s a fancy way of changing perspectives while keeping the essence of the theory intact. Think of it as rearranging the furniture without changing the house.

By carefully manipulating the terms in our Hamiltonian, we can ensure that it maps correctly onto what we expect. This transformation helps us maintain the right properties and aligns our results with the underlying physics.

As we moved along, we put together equations that capture this transformation order by order. It’s a bit like peeling back the layers of an onion: with each layer, we see more clearly how the different parts interact and fit together.

Dealing with Higher Orders

The deeper we go, the more intricate things become. We started looking at higher orders, where more complexity arises. This is where the rubber meets the road, and we see how the parameters and terms we introduced really influence the behavior of the Hamiltonian.

At second order, more operators emerge, which means we need to be cautious about how they interact. We must be careful to ensure that the conservation laws still apply, which can quickly become complicated.

We’re not just doing math for the sake of it. Each term has potential physical implications, and they can tell us about how energy and momentum behave in this deformed landscape.

As we navigate through these higher orders, we find that multiple theories can coexist, all claiming to be valid versions of the original theory. Each different choice leads to different insights and perspectives, which adds richness and diversity to our understanding of the subject.

The Role of the Stress Tensor and Energy Spectrum

The stress tensor plays a critical role in this whole picture. It helps us understand how quantities like energy and momentum flow within our deformed theories. Yet, this tensor isn't just a mere spectator; it actively helps us uncover hidden aspects of the Hamiltonian.

When we compute the energy spectrum using our deformed Hamiltonian, things start to solidify. We compare predictions with known results, and it’s comforting to find consistency with previous theoretical work.

There’s an adventurous spirit to all of this; each result leads us to new questions, new ideas, and new ways of thinking about the underlying physics.

Current Conservation

Now, let’s take a moment to appreciate the conservation aspects. When we computed the stress tensor densities, we confirmed that they satisfy the flow equations we’ve been discussing. This is reassuring because it means our theory behaves well and respects the fundamental conservation laws that physicists hold dear.

Imposing these conservation equations leads to exciting new insights about how our deformed theories can evolve. It’s as if we’re piecing together a complex puzzle where each piece fits perfectly into the overall design.

The KdV Charges Weigh In

We've touched on something called KdV charges before, which are like the superheroes of our theoretical framework. They're conserved quantities that help us maintain the integrity of our theories even when we introduce deformations.

As we explored these charges further, we found that they can also be non-local. But don’t worry; we’ve got tricks up our sleeves. With clever combinations and crafting, we can still define local versions of these KdV charges that fit snugly into our theories and respect the properties we aim to preserve.

In a sense, this part feels like a dance: balancing local and non-local properties while ensuring that everything remains coherent and consistent.

Generalized Deformations

Finally, we have to mention the broader implications of what we’ve been discussing. While our focus has been on the specific case of deformation, these concepts extend to other generalized deformations as well.

By studying how various functions of conserved charges behave, we uncover new layers of understanding that enrich the overall framework of theoretical physics. Each exploration opens doors to potentially exciting new theories and insights that push the boundaries of what we know.

Conclusion: So, What Have We Learned?

In wrapping up, we’ve taken quite a journey-one that blends clever mathematics with deep physical insights. We’ve explored how locality behaves in deformed theories, navigated through complexities to construct Hamiltonians, and connected back to fundamental principles of conservation.

The takeaway? Even though theoretical physics can seem like a daunting puzzle, with the right tools and approaches, we can make sense of it and uncover the beautiful interconnectedness that underlies all the complexities. What lies ahead? Only time will tell, but the adventure continues, full of possibilities and new horizons to explore!

Original Source

Title: Locality and Conserved Charges in $T\overline{T}$-Deformed CFTs

Abstract: We investigate the locality properties of $T \overline T$-deformed CFTs within perturbation theory. Up to third order in the deformation parameter, we find a Hamiltonian operator which solves the flow equation, reproduces the Zamolodchikov energy spectrum, and is consistent with quasi-locality of the theory. This Hamiltonian includes terms proportional to the central charge which have not appeared before and which are necessary to reproduce the correct spectrum. We show that the Hamiltonian is not uniquely defined since it contains free parameters, starting at second order, which do not spoil the above properties. We then use it to determine the full conserved stress tensor. In our approach, the KdV charges are automatically conserved to all orders but are not a priori local. Nevertheless, we show that they can be made local to first order. Our techniques allow us to further comment on the space of Hamiltonians constructed from products of KdV charges which also flow to local charges in the deformed theory in the IR.

Authors: Ruben Monten, Richard M. Myers, Konstantinos Roumpedakis

Last Update: 2024-11-09 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.06261

Source PDF: https://arxiv.org/pdf/2411.06261

Licence: https://creativecommons.org/licenses/by/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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