Can quantum fluctuations differentiate between standard and unimodular gravity?
From MaRDI portal
Publication:2085273
DOI10.1007/JHEP12(2021)090OpenAlexW3170649101MaRDI QIDQ2085273
A. D. Pereira, Gustavo P. de Brito, Oleg Melichev, Roberto Percacci
Publication date: 14 October 2022
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2105.13886
Related Items
Scaling solutions for asymptotically free quantum gravity ⋮ The one-loop unimodular Graviton propagator in any dimension ⋮ Asymptotic freedom and safety in quantum gravity
Cites Work
- Monodromy inflation and an emergent mechanism for stabilising the cosmological constant
- Do the gravitational corrections to the beta functions of the quartic and Yukawa couplings have an intrinsic physical meaning?
- Unimodular gauge in perturbative gravity and supergravity
- Investigating the ultraviolet properties of gravity with a Wilsonian renormalization group equation
- Forks in the road, on the way to quantum gravity
- Gauges and functional measures in quantum gravity. I: Einstein theory
- Essential nature of Newton's constant in unimodular gravity
- Unimodular quantum gravity and the cosmological constant
- Non-minimal tinges of unimodular gravity
- Unimodular quantum gravity: steps beyond perturbation theory
- The nonperturbative functional renormalization group and its applications
- A link that matters: towards phenomenological tests of unimodular asymptotic safety
- The trace-free Einstein equations and inflation
- Aspects of the functional renormalisation group
- Quantum corrections to unimodular gravity
- On unimodular quantum gravity
- Introduction to the Functional RG and Applications to Gauge Theories
- On the trace-free Einstein equations as a viable alternative to general relativity
- Unimodular theory of gravity and the cosmological constant
- Renormalization group flow in scalar-tensor theories: I
- Possible solution to the cosmological-constant problem
- Gauge-invariant quantum gravitational corrections to correlation functions
- The cosmological constant problem
