We propose an explicit spin-foam amplitude for Lorentzian gravity in three dimensions. The model is based on two main requirements: that it should be structurally similar to its well-known Euclidean analog, and that geometricity should be recovered in the semiclassical regime. To this end we introduce new coherent states for space-like 1-dimensional boundaries, derived from the continuous series of unitary $mathrm{SU}(1,1)$ representations. We show that the relevant objects in the amplitude can be written in terms of the defining representation of the group, just as so happens in the Euclidean case. We derive an expression for the semiclassical amplitude at large spins, showing that it relates to the Lorentzian Regge action.

Future Roadmap for Readers

Overview

In this article, we present an explicit spin-foam amplitude for Lorentzian gravity in three dimensions. Our model satisfies two important requirements: it is structurally similar to its well-known Euclidean analog, and it recovers geometricity in the semiclassical regime. We achieve this by introducing new coherent states for space-like 1-dimensional boundaries, which are derived from the continuous series of unitary $mathrm{SU}(1,1)$ representations. In addition, we demonstrate that the relevant objects in the amplitude can be expressed in terms of the defining representation of the group, just like in the Euclidean case. Lastly, we derive an expression for the semiclassical amplitude at large spins, revealing its relationship to the Lorentzian Regge action.

Roadmap

  1. Introduction: We provide an overview of the article, discussing the motivation behind our research and the goals we aim to achieve.
  2. Lorentzian Spin-Foam Amplitude: We present our explicit spin-foam amplitude for Lorentzian gravity in three dimensions. We explain how it satisfies the structural requirements and recovers geometricity in the semiclassical regime.
  3. New Coherent States: We introduce the new coherent states for space-like 1-dimensional boundaries. These coherent states are derived from the continuous series of unitary $mathrm{SU}(1,1)$ representations.
  4. Relevant Objects in the Amplitude: We demonstrate that the relevant objects in the amplitude can be expressed in terms of the defining representation of $mathrm{SU}(1,1)$, similar to the Euclidean case. This similarity allows us to maintain the structural similarity between the Lorentzian and Euclidean amplitudes.
  5. Semiclassical Amplitude at Large Spins: We derive an expression for the semiclassical amplitude at large spins and establish its relationship to the Lorentzian Regge action. This further validates the effectiveness of our spin-foam amplitude model.

Challenges and Opportunities

While our proposed spin-foam amplitude for Lorentzian gravity in three dimensions shows significant promise, there are challenges and opportunities that lie ahead:

  • Validation and Testing: The model needs to be thoroughly tested and validated through simulations or comparisons with existing theories and experimental data. This will help ensure its accuracy and reliability.
  • Extension to Higher Dimensions: Our current model is limited to three dimensions. Extending it to higher dimensions could open up new possibilities and applications in the field of gravity.
  • Integration with Quantum Field Theory: Investigating the integration of our spin-foam amplitude with quantum field theory could lead to a more comprehensive understanding of the quantum nature of gravity.
  • Practical Implementation: Developing practical algorithms and computational techniques for implementing the spin-foam amplitude in real-world scenarios is crucial for its practical applications in areas like cosmology, black holes, and quantum gravity.

Conclusion

Our explicit spin-foam amplitude for Lorentzian gravity in three dimensions, which satisfies structural requirements and recovers geometricity in the semiclassical regime, holds great potential for advancing our understanding of gravity at the quantum level. However, further research and development are necessary to validate the model, extend it to higher dimensions, integrate it with quantum field theory, and ensure its practical implementation. By addressing these challenges and capitalizing on the opportunities, we can make significant strides in the field of quantum gravity.

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