Multi-scale entanglement renormalization ansatz Tensor network

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SUMMARY

The discussion centers on the multi-scale entanglement renormalization ansatz (MERA) as a representation of the ground state of a many-body Hamiltonian, utilizing tensor network renormalization (TNR). Glen Evenbly and Guifre Vidal's approach, submitted on February 18, 2015, effectively circumvents the energy minimization challenges of previous MERA algorithms by applying TNR to the Euclidean time evolution operator for infinite inverse temperature. This method not only extends the MERA formalism to classical statistical systems but also integrates concepts from the AdS/CFT conjecture, linking entanglement, geometry, and renormalization in a coherent framework.

PREREQUISITES
  • Tensor network renormalization (TNR)
  • Multi-scale entanglement renormalization ansatz (MERA)
  • AdS/CFT conjecture
  • Euclidean time evolution operator
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  • Explore the implications of the AdS/MERA framework in condensed matter physics
  • Study the Ryu-Takayanagi proposal and its relation to entanglement entropy
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  • Learn about the connections between renormalization and holography in quantum gravity
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Researchers and students in theoretical physics, particularly those focused on quantum gravity, condensed matter physics, and the study of entanglement in quantum systems.

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as a new proposal for QGhttp://arxiv.org/abs/1502.05385
Tensor network renormalization yields the multi-scale entanglement renormalization ansatz
Glen Evenbly, Guifre Vidal
(Submitted on 18 Feb 2015)
We show how to build a multi-scale entanglement renormalization ansatz (MERA) representation of the ground state of a many-body Hamiltonian H by applying the recently proposed \textit{tensor network renormalization} (TNR) [G. Evenbly and G. Vidal, arXiv:1412.0732] to the Euclidean time evolution operator e−βH for infinite β. This approach bypasses the costly energy minimization of previous MERA algorithms and, when applied to finite inverse temperature β, produces a MERA representation of a thermal Gibbs state. Our construction endows TNR with a renormalization group flow in the space of wave-functions and Hamiltonians (and not just in the more abstract space of tensors) and extends the MERA formalism to classical statistical systems.
 
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It is not a new proposal. It is mainly about the AdS/CFT conjecture of string theory. If the conjecture is right, are there relatively simple ways we can understand how it works? The AdS/MERA picture was proposed by Brian Swingle (Physics Monkey) to help understand AdS/CFT using tools from condensed matter physics. Among the key papers preceding AdS/MERA are Juan Maldacena's thermofield double paper, the Ryu-Takayanagi proposal linking entanglement entropy and area, and Guifre Vidal's MERA. Also, there are many papers linking renormalization and holography, and the MERA is a form of renormalization. What the MERA seems to offer is a simple picture of how the various ideas (entanglement, geometry, renormalization) can be linked together.
 

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