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相关论文: Ho\v{r}ava gravity is asymptotically free (in 2+1 …

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We investigate the renormalization group flow of projectable Horava gravity in $(3+1)$ dimensions generated by marginal operators with respect to the Lifshitz scaling. The flow possesses a number of asymptotically free fixed points. We find…

高能物理 - 理论 · 物理学 2024-12-03 Andrei O. Barvinsky , Alexander V. Kurov , Sergey M. Sibiryakov

We report a comprehensive numerical study of the renormalization group flow of marginal couplings in $(3+1)$-dimensional projectable Ho\v{r}ava gravity. First, we classify all fixed points of the flow and analyze their stability matrices.…

广义相对论与量子宇宙学 · 物理学 2024-11-22 Andrei O. Barvinsky , Alexander V. Kurov , Sergey M. Sibiryakov

We give a review of UV renormalization of Ho\v{r}ava gravity (HG) models introduced as a remedy against violation of unitarity in quantum gravity theory. Projectable and non-projectable low-dimensional HG models and the spectra of their…

高能物理 - 理论 · 物理学 2023-02-07 Andrei O. Barvinsky

We compute the renormalization group running of the Newton constant and the parameter $\lambda$ in $(3+1)$-dimensional projectable Horava gravity. We use the background field method expanding around configurations with flat spatial metric,…

高能物理 - 理论 · 物理学 2019-07-31 Andrei O. Barvinsky , Mario Herrero-Valea , Sergey M. Sibiryakov

Horava gravity is a proposal for a UV completion of gravitation obtained by endowing the space-time manifold with a preferred foliation in space-like hypersurfaces. This allows for a power-counting renormalizable theory free of ghosts, at…

广义相对论与量子宇宙学 · 物理学 2023-07-26 M. Herrero-Valea

We study the non-perturbative renormalization group flow of higher-derivative gravity employing functional renormalization group techniques. The non-perturbative contributions to the $\beta$-functions shift the known perturbative…

高能物理 - 理论 · 物理学 2009-10-08 Dario Benedetti , Pedro F. Machado , Frank Saueressig

The functional renormalization group equation for projectable Ho\v{r}ava-Lifshitz gravity is used to derive the non-perturbative beta functions for the Newton's constant, cosmological constant and anisotropy parameter. The resulting coupled…

高能物理 - 理论 · 物理学 2015-06-17 Adriano Contillo , Stefan Rechenberger , Frank Saueressig

Violations of Lorentz (and specifically boost) invariance can make gravity renormalizable in the ultraviolet, as initially noted by Ho\v{r}ava, but are increasingly constrained in the infrared. At low energies, Ho\v{r}ava gravity is…

广义相对论与量子宇宙学 · 物理学 2021-04-13 Nicola Franchini , Mario Herrero-Valea , Enrico Barausse

Recently Horava proposed a renormalizable gravity theory with higher derivatives by abandoning the Lorenz invariance in UV. Here, I study the Horava model at $\lambda=1/3$, where an anisotropic Weyl symmetry exists in the UV limit, in…

高能物理 - 理论 · 物理学 2015-05-14 Mu-in Park

We derive the full set of beta functions for the marginal essential couplings of projectable Horava gravity in (3 + 1)-dimensional spacetime. To this end we compute the divergent part of the one-loop effective action in static background…

高能物理 - 理论 · 物理学 2024-12-03 Andrei O. Barvinsky , Alexander V. Kurov , Sergey M. Sibiryakov

Horava gravity is a proposal for completing general relativity in the ultraviolet by interactions that violate Lorentz invariance at very high energies. We focus on (2+1)-dimensional projectable Horava gravity, a theory which is…

广义相对论与量子宇宙学 · 物理学 2021-12-20 Guillermo Lara , Mario Herrero-Valea , Enrico Barausse , Sergey M. Sibiryakov

We use functional renormalization group methods to study gravity minimally coupled to a free scalar field. This setup provides the prototype of a gravitational theory which is perturbatively non-renormalizable at one-loop level, but may…

高能物理 - 理论 · 物理学 2009-10-06 Dario Benedetti , Pedro F. Machado , Frank Saueressig

For any fundamental quantum field theory, unitarity, renormalizability, and relativistic invariance are considered to be essential properties. Unitarity is inevitably connected to the probabilistic interpretation of the quantum theory,…

高能物理 - 理论 · 物理学 2021-04-27 Christian F. Steinwachs

We review and extend in several directions recent results on the asymptotic safety approach to quantum gravity. The central issue in this approach is the search of a Fixed Point having suitable properties, and the tool that is used is a…

高能物理 - 理论 · 物理学 2013-08-28 Alessandro Codello , Roberto Percacci , Christoph Rahmede

In the framework of the power-counting renormalizable theory of gravitation, recently proposed by Ho\v{r}ava, we study the limit $\lambda\to\infty$, which is arguably the most natural candidate for the ultraviolet fixed point of the…

高能物理 - 理论 · 物理学 2011-06-27 A. Emir Gumrukcuoglu , Shinji Mukohyama

We propose a new extended theory of Ho\v{r}ava gravity based on the following three conditions: (i) UV completion, (ii) healthy IR behavior and (iii) a stable vacuum state in quantized version of the theory. Compared with other extended…

高能物理 - 理论 · 物理学 2010-09-21 Fu-Wen Shu

We use the Wetterich equation for foliated spacetimes to study the RG flow of projectable Horava-Lifshitz gravity coupled to n Lifshitz scalars. Using novel results for anisotropic heat kernels, the matter-induced beta functions for the…

广义相对论与量子宇宙学 · 物理学 2014-10-29 Giulio D'Odorico , Frank Saueressig , Marrit Schutten

We investigate the ultraviolet behaviour of quantum gravity within a functional renormalisation group approach. The present setup includes the full ghost and graviton propagators and, for the first time, the dynamical graviton three-point…

高能物理 - 理论 · 物理学 2016-05-23 Nicolai Christiansen , Benjamin Knorr , Jan Meibohm , Jan M. Pawlowski , Manuel Reichert

We explore whether quantum gravity effects within the asymptotic safety paradigm can provide a predictive ultraviolet completion for Abelian gauge theories. We evaluate the effect of quantum gravity fluctuations on the running couplings in…

高能物理 - 理论 · 物理学 2017-05-18 Nicolai Christiansen , Astrid Eichhorn

We analyze the electromagnetic-gravity interaction in a pure Ho\v{r}ava-Lifshitz framework. To do so we formulate the Ho\v{r}ava-Lifshitz gravity in $4+1$ dimensions and perform a Kaluza-Klein reduction to $3+1$ dimensions. We use this…

高能物理 - 理论 · 物理学 2018-11-21 Jorge Bellorin , Alvaro Restuccia , Francisco Tello-Ortiz
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