The renormalizability of Hořava–Lifshitz-type gravities

By D. Orlando, S. Reffert. 2009

156 citations recorded by the source corpus.

In this paper, we discuss the renormalizability of Hořava–Lifshitz-type gravity theories. Using the fact that Hořava–Lifshitz (HL) gravity is very closely related to the stochastic quantization of topologically massive gravity, we show that the renormalizability of HL gravity only depends on the renormalizability of topologically massive gravity. This is a consequence of the BRST and time-reversal symmetries pertinent to theories satisfying the detailed balance condition.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/1481932e61a370d312acfb92e3c8b1a6efd6e769

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In Astronomy and Astrophysics

1. Anzhong Wang
2. Mu-In Park
3. Emmanuel N. Saridakis

In Nuclear and High Energy Physics

1. Anzhong Wang
2. Mu-In Park
3. Emmanuel N. Saridakis

In Statistical and Nonlinear Physics

1. Anzhong Wang
2. Mu-In Park

Citations in the corpus

• Hořava gravity at a Lifshitz point: A progress report (2017, background): “21), the renormalizability of Hořava gravity was shown to reduce to the one of the corresponding (2+1)-dimensional topologically massive gravity [280], by using stochastic quantization [281–283].”
• The black hole and cosmological solutions in IR modified Hořava gravity (2009, background): “Since then various aspects and solutions have been studied [3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 23, 24, 25, 26, 27, 28, 29].”