Houthoff W B, Kurov A, Saueressig F
Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University Nijmegen, 6525 AJ Nijmegen, The Netherlands.
Department of Theoretical Physics, Moscow State University, Moscow, Russia.
Eur Phys J C Part Fields. 2017;77(7):491. doi: 10.1140/epjc/s10052-017-5046-8. Epub 2017 Jul 24.
We use a functional renormalization group equation tailored to the Arnowitt-Deser-Misner formulation of gravity to study the scale dependence of Newton's coupling and the cosmological constant on a background spacetime with topology [Formula: see text]. The resulting beta functions possess a non-trivial renormalization group fixed point, which may provide the high-energy completion of the theory through the asymptotic safety mechanism. The fixed point is robust with respect to changing the parametrization of the metric fluctuations and regulator scheme. The phase diagrams show that this fixed point is connected to a classical regime through a crossover. In addition the flow may exhibit a regime of "gravitational instability", modifying the theory in the deep infrared. Our work complements earlier studies of the gravitational renormalization group flow on a background topology [Formula: see text] (Biemans et al. Phys Rev D 95:086013, 2017, Biemans et al. arXiv:1702.06539, 2017) and establishes that the flow is essentially independent of the background topology.
我们使用一个针对引力的阿诺维特 - 德塞 - 米斯纳(Arnowitt-Deser-Misner)形式量身定制的泛函重整化群方程,来研究在具有拓扑结构[公式:见原文]的背景时空上牛顿耦合和宇宙学常数的标度依赖性。所得的β函数具有一个非平凡的重整化群不动点,它可能通过渐近安全机制为该理论提供高能完备性。该不动点在改变度规涨落的参数化和调节器方案时是稳健的。相图表明,这个不动点通过一个交叉与一个经典区域相连。此外,流可能会展现出一个“引力不稳定性”区域,在深红外区域修改该理论。我们的工作补充了早期关于背景拓扑结构[公式:见原文]上引力重整化群流的研究(比曼斯等人,《物理评论D》第95卷:086013,2017年;比曼斯等人,arXiv:1702.06539,2017年),并确定该流本质上与背景拓扑无关。