RG-flow, gravity and the cosmological constant

RG-flow, gravity and the cosmological constant
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RG-流、重力和宇宙常数

DOI:
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发表时间:
1999
期刊:
影响因子:
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通讯作者:
H. Verlinde
H. Verlinde
中科院分区:
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文献类型:
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作者:
E. Verlinde;H. Verlinde

文献摘要

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我们研究了低能量的有效作用的重力,诱导整合出规范和物质领域,在一般类的Randall-Sundrum型弦紧化的情况下,指数翘曲因子。我们的方法结合降维与全息映射之间的5-D超引力和4-D大N场理论。利用经典的超引力近似,我们推导出一个有效作用量S的流动方程,它控制着尺度变换下的行为。我们发现,作为一个结果,每个极值的S自动描述了一个完整的RG轨迹的经典解决方案。这意味着,如果在高能理论中取消宇宙学常数,经典平坦空间背景在RG流下自然保持稳定。负责这种稳定性的机制是,由可能的相变产生的非零真空能量,被扭曲因子的收缩率的动态调整所吸收。
We study the low energy effective action S of gravity, induced by integrating out gauge and matter fields, in a general class of Randall-Sundrum type string compactification scenarios with exponential warp factors. Our method combines dimensional reduction with the holographic map between 5-d supergravity and 4-d large-N field theory. Using the classical supergravity approximation, we derive a flow equation of the effective action S that controls its behavior under scale transformations. We find that as a result each extremum of S automatically describes a complete RG trajectory of classical solutions. This implies that, provided the cosmological constant is canceled in the high energy theory, classical flat space backgrounds naturally remain stable under the RG-flow. The mechanism responsible for this stability is that the non-zero vacuum energy generated by possible phase transitions, is absorbed by a dynamical adjustment of the contraction rate of the warp factor.