Has anyone read this new paper on extending the BGV?

In summary, the conversation discusses a new paper by Will Kinney and others which presents a new version of the Borde-Guth-Vilenkin theorem. This theorem states that any spacetime with net positive expansion must be geodesically incomplete. The paper uses the fluid flow formalism of General Relativity and makes no assumptions about energy conditions. It is applicable to cosmological models using the standard FLRW metric and related expanding metrics but not to other conformal metrics.
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Luis Mijares
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I was wondering if someone could explain this paper to me
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It only talks about net expanding metrics on a locally de Sitter space in a time interval, so while it would apply to cosmological models using the standard FLRW metric and related expanding metrics like the LTB metric, as well as the metrics used in Penrose's Cyclic Cosmology, it wouldn't apply to any cosmological model which doesn't have a net expanding metric on a locally de Sitter space in a time interval. For example, one class of conformal metrics talked about in Lucas Lombriser's recent paper "Cosmology in Minkowski space" occurs in static Minkowski space and thus is not net expanding or in locally de Sitter space, and wouldn't be affected by the result in the paper.
 
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FWIW, BGV is a reference to the Borde-Guth-Vilenkin (BGV) theorem which states that any spacetime with net positive expansion must be geodesically incomplete. The paper and its abstract are as follows:

[Submitted on 20 Jul 2023]

The Borde-Guth-Vilenkin Theorem in extended de Sitter spaces​

William H. Kinney (Univ. at Buffalo, SUNY, USA), Suvashis Maity, L. Sriramkumar (Indian Insitute of Technology, Madras, India)
The Borde-Guth-Vilenkin (BGV) theorem states that any spacetime with net positive expansion must be geodesically incomplete. We derive a new version of the theorem using the fluid flow formalism of General Relativity.

The theorem is purely kinematic, depending on the local expansion properties of geodesics, and makes no assumptions about energy conditions. We discuss the physical interpretation of this result in terms of coordinate patches on de Sitter space, and apply the theorem to Penrose's model of Conformal Cyclic Cosmology. We argue that the Conformal Cyclic extension of an asymptotically de Sitter universe is geodesically incomplete.
 

1. What is the BGV and why is it important?

The BGV, or Brakerski-Gentry-Vaikuntanathan, is a cryptographic scheme used for homomorphic encryption. It allows for computations to be performed on encrypted data without revealing the underlying information, making it a crucial tool for secure data processing and storage.

2. What does this new paper propose for extending the BGV?

The new paper proposes a method for extending the BGV to allow for more efficient and secure homomorphic computations. It introduces a new technique called "bootstrapping" which reduces the size of ciphertexts and improves the efficiency of homomorphic operations.

3. How does this new paper differ from previous research on extending the BGV?

This new paper builds upon previous research on extending the BGV by introducing the bootstrapping technique. This technique was previously only used in other homomorphic encryption schemes, but has now been adapted for use with the BGV.

4. What are the potential applications of this extended BGV?

The extended BGV has the potential to greatly improve the efficiency and security of homomorphic computations, making it applicable in a wide range of fields such as secure cloud computing, data analysis, and machine learning. It could also have implications for privacy-preserving technologies.

5. What are the limitations or challenges of extending the BGV?

One of the main challenges of extending the BGV is maintaining the security of the encryption scheme while also improving its efficiency. Additionally, implementing the bootstrapping technique may require significant computational resources, which could limit its practical applications.

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