Immirzi参数的扰动运行
Perturbative running of the Immirzi parameter
摘要:
我们报告通过微扰单圈计算发现的Immirzi参数的重整化。
英文摘要:
We report on the renormalization of the Immirzi parameter found through perturbative one-loop calculations.
机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。
Perturbative running of the Immirzi parameter
Dario Benedetti, Simone Speziale
我们报告通过微扰单圈计算发现的Immirzi参数的重整化。
We report on the renormalization of the Immirzi parameter found through perturbative one-loop calculations.
机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。
继续探索
Running Immirzi Parameter and Asymptotic Safety
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Perturbative quantum gravity with the Immirzi parameter
我们在一阶四分体形式下研究微扰量子引力。最低阶的作用量相当于爱因斯坦-嘉当加上宇称奇项,在文献中称为霍尔斯特作用量。奇偶奇项的耦合常数可以用圈量子引力的Immirzi参数来确定。我们计算了单圈展开中的量子有效作用量。在度量二阶公式中,我们发现在纯引力的情况下,理论是在壳有限的,牛顿常数和Immirzi参数的运行是不必要的。在费米子的存在下,情况在两个基本方面发生了变化。首先,像往常一样,出现不可重正化的对数发散。其次,Immirzi参数成为先验可观察的,我们发现,它是重整化的辐射修正产生的四费米子相互作用。我们计算它的beta函数,并讨论可能的影响。beta函数的符号取决于Immirzi参数的绝对值是大于还是小于1,加上或减去1的值是UV固定点(我们使用欧几里得签名)。最后,我们发现,霍尔斯特行动是稳定的辐射修正的情况下,最小的耦合,更高阶的不可重整化的相互作用。
Einstein-Cartan gravity, Asymptotic Safety, and the running Immirzi parameter
本文分析了Einstein-Cartan理论空间上量子引力的泛函重整化群流。后者由所有的作用泛函依赖于自旋连接和维尔拜因场(共框架),这是不变的时空同构和本地框架旋转。在本文的第一部分中,我们开发了一个通用的方法和相应的计算工具,可以用来分析相关的有效平均行动的流量方程的任何截断这个理论空间。在第二部分中,我们将其应用到一个特定的三维截断理论空间,该空间由牛顿常数,宇宙学常数和Immirzi参数参数化。对它们的尺度依赖性进行了全面的分析,并研究了在这一迄今尚未探索的理论空间上定义渐近安全理论的可能性。原则上,度量引力的渐近安全性(至少在有效平均作用量的水平上)对于爱因斯坦-嘉当理论空间上的渐近安全性来说既不是必要的,也不是充分的,因为爱因斯坦-嘉当理论空间可能容纳不同的微观量子引力理论的“普适类”。然而,我们确实找到了至少一个非高斯重整化群不动点的存在的证据,这似乎适合于在自旋连接和vielbein是基本场变量的设置中的渐近安全结构。
On the role of the Barbero-Immirzi parameter in discrete quantum gravity
Barbero和Immirzi提出的单参数变换族在量子引力的非微扰方法中起着重要作用,其中包括圈量子引力和自旋泡沫。它有利于循环量化方案,随后的Barbero-Immirzi参数(伽马)出现在两个光谱的几何算子和自旋泡沫提供的动力学。然而,关于量子物理是否应该依赖于Barbero-Immirzi参数的争论仍在继续。从离散的SO(4)-BF理论相空间出发,我们找到了两种可能的简化。第一个减少到一个相空间与伽玛相关的辛结构,更一般地与相空间的基础环量子引力限制到一个单一的图形- a.k.a.扭曲的几何体。第二,更充分的减少导致一个伽玛独立的辛结构的相空间的分段平坦的线性几何- a.k.a. Regge几何。因此,物理预测的伽马依赖性与量子化下相空间的选择有关。
Fermions in Ashtekar-Barbero Connections Formalism for Arbitrary Values of the Immirzi Parameter
将广义相对论的Ashtekar-Barbero-Immirzi公式推广到包括旋量物质场。我们的配方适用于通用值的Immirzi参数,并减少到Ashtekar-Romano-Tate的方法时,Immirzi参数取等于虚数单位。引力-费米子耦合系统的动力学过程由具有非最小耦合项的Holst加Dirac作用量描述。非最小相互作用和对Hilbert-Palatini作用量的Holst修正一起重构了Nieh-Yan不变量,使得得到的有效作用量是具有典型Fermi类相互作用项的Einstein-Cartan理论的作用量:尽管存在旋量物质场,Immirzi参数在经典的有效动力学中不起作用,结果只是总发散前面的一个乘法因子。我们减少总行动的理论的总和动态独立Ashtekar-Romano-Tate行动的自我和反自我的对偶连接,不同的权重取决于Immirzi参数。这允许以简单的方式计算完整理论的约束,只需认识到Barbero-Immirzi连接是自偶和反自偶Ashtekar连接的加权和。最后得到的分离作用量的约束结果是多项式的自和反自对偶连接,这可能有意义的旋量物质的非微扰量子引力的框架中的包含。
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In this paper, we analyse a curvature- and torsion-square quantum gravity action with an additional Holst term minimally coupled to a massive Dirac field in four dimensions. The main purpose here is to try to estimate and compare the value of the Barbero-Immirzi (BI) parameter with its currently known results. To do that, we work out the physical mass of the fermion as a function of this parameter in a perturbative one-loop calculation, assuming the scenario of a physics at the TeV-scale.
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以自旋联系和维尔本为基本场变量,研究了量子引力的重整化群性质。尺度相关的有效作用量必须在时空同构和局部坐标系旋转下都是不变的。非微扰RG方程求解显式截断的理论空间定义的Holst型行动,其中涉及一个运行的Immirzi参数的三个参数的家庭。我们发现了一个渐近安全的基本理论存在的证据,可能不等价于以同样方式构造的度规量子引力。
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