Asymptotic safety on the lattice

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SUMMARY

The forum discussion centers on the concept of asymptotic safety in quantum gravity, as presented by Jack Laiho at the Lattice 2011 conference. Asymptotic safety, introduced by Steven Weinberg, posits that a non-renormalizable theory can remain predictive if its renormalization group flow has a finite ultraviolet fixed point. Numerical evidence suggests that gravity may exhibit asymptotic safety with only three parameters. Additionally, the discussion highlights the importance of lattice studies in exploring non-Gaussian UV fixed points in higher dimensions, particularly in the context of gauge theories.

PREREQUISITES
  • Understanding of asymptotic safety in quantum field theory
  • Familiarity with renormalization group flow concepts
  • Knowledge of lattice quantum field theory techniques
  • Basic principles of gauge theories and their dimensional constraints
NEXT STEPS
  • Research the implications of asymptotic safety in quantum gravity theories
  • Explore the numerical methods used in lattice quantum field theory
  • Investigate the role of spectral dimensions in quantum gravity models
  • Study the effects of adding measure terms to the Regge action in lattice models
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The discussion is beneficial for theoretical physicists, researchers in quantum gravity, and students interested in advanced concepts of lattice field theory and asymptotic safety.

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Interesting posts from Georg von Hippel at http://latticeqcd.blogspot.com/

Monday, July 11, 2011
Lattice 2011, Day One
"Next was a talk by Jack Laiho on Asymptotic Safety and Quantum Gravity. The concept of asymptotic safety as introduced by Weinberg states that a perturbatively non-renormalisable theory may still be well-defined and possesses predictive power if its renormalisation group flow has an ultraviolet fixed point with a finite number of relevant directions. There is some numerical evidence that gravity might be asymptotically safe with only three parameters. In a Euclidean framework, asymptotic safety corresponds to the existence of a critical point. This scenario has been studied in a number of different formulations, including the Euclidean dynamical triangulations of Ambjorn et al. (which have a crumpled phase with infinite Hausdorff dimension and a branched polymer phase with Hausdorff dimension 2, separated by a first-order phase transition, and hence no hope to describe continuum physics) and the Causal Dynamical Triangulations of Ambjorn and Loll (which have a large-scale solution in the form of de Sitter space, and where the spectral dimension runs from 2 at short scales to 4 at large scales). Jack and his student have studied what happens if one adds a measure term to the Regge action, and have found that there are three phases (collapsed, extended, and branched polymer phase) with the possibility of a critical end point in the phase diagram, which could realize the scenario of asymptotic safety. There is also evidence that the spectral dimensions runs from 4 at large scales to 3/2 at short scales, where the dimension 3/2 would reconcile the requirements of holography and the Bekenstein-Hawking entropy."

Wednesday, July 13, 2011
Lattice 2011, Day Two
"The first speaker was Aleksi Kurkela, who spoke about large extra dimensions and the lattice. Extra dimensions are phenomenologically appealing, but since gauge theories in d>4 are non-renormalisable, they are defined only up to a regularisation. Results from the ε-expansion suggest the existence of a non-Gaussian UV fixed point in higher dimensions, but since d=5 is well outside of the expected convergence radius of the expansion, lattice studies are needed to check this; for the isotropic case it does not appear to be true, but for the anisotropic case there is evidence that it is indeed true."
 
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marcus has just https://www.physicsforums.com/showpost.php?p=3475973&postcount=1566":

"Although, as we are in a different regime, we cannot make direct contact to the results of [13], our results show that a non-trivial continuum limit is possible in these models and open a small window of hope on non-causal DT models."

"The link to the numerical results of [13] is unclear, and deserves further exploration, either by pushing the simulations to larger κD−2 and larger volumes, or by trying to extend the analytical tools to finite κD−2."
 
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"Supernovae evidence for foundational change to cosmological models" https://arxiv.org/pdf/2412.15143 The paper claims: We compare the standard homogeneous cosmological model, i.e., spatially flat ΛCDM, and the timescape cosmology which invokes backreaction of inhomogeneities. Timescape, while statistically homogeneous and isotropic, departs from average Friedmann-Lemaître-Robertson-Walker evolution, and replaces dark energy by kinetic gravitational energy and its gradients, in explaining...

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