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Regular self-consistent geometries with infinite quantum backreaction in 2D dilaton gravity and black hole thermodynamics: unfamiliar features of familiar models

机译:二维dilaton引力和黑洞热力学中具有无限量子反向反应的规则自洽几何:熟悉模型的不熟悉特征

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摘要

We analyze the rather unusual properties of some exact solutions in 2D dilaton gravity for which infinite quantum stresses on the Killing horizon can be compatible with regularity of the geometry. In particular, the Boulware state can support a regular horizon. We show that such solutions are contained in some well-known exactly solvable models (for example, RST). Formally, they appear to account for an additional coefficient $B$ in the solutions (for the same Lagrangian which contains also ''traditional'' solutions) that gives rise to the deviation of temperature $T$ from its Hawking value $T_{H}$. The Lorentzian geometry, which is a self-consistent solution of the semiclassical field equations, in such models, is smooth even at $B\neq 0$ and there is no need to put B=0 ($T=T_{H}$) to smooth it out$.$ We show how the presence of $B\neq 0$ affects the structure of spacetime. In contrast to ''usual'' black holes, full fledged thermodynamic interpretation, including definite value of entropy, can be ascribed (for a rather wide class of models) to extremal horizons, not to nonextreme ones. We find also new exact solutions for ''usual'' black holes (with $T=T_{H}$). The properties under discussion arise in the \QTR{it}{weak}-coupling regime of the effective constant of dilaton-gravity interaction. Extension of features, traced in 2D models, to 4D dilaton gravity leads, for some special models, to exceptional nonextreme black holes having no own thermal properties.
机译:我们分析了二维Dilaton重力中某些精确解的相当不寻常的性质,对于这些精确解,在Killing视界上的无限量子应力可以与几何规律性兼容。特别是,Boulware状态可以支持规则范围。我们证明了这样的解决方案包含在一些众所周知的完全可解决的模型中(例如RST)。形式上,它们似乎在解中考虑了一个额外的系数$ B $(对于同样包含“传统”解的拉格朗日数),这会导致温度$ T $与其Hawking值$ T_ {H } $。在此类模型中,洛伦兹几何是半经典场方程的自洽解,即使在$ B \ neq 0 $时也很光滑,无需放置B = 0($ T = T_ {H} $ )使其平滑$。$我们展示$ B \ neq 0 $的存在如何影响时空的结构。与“通常的”黑洞相反,可以将成熟的热力学解释(包括一定的熵值)归因于极端的视野(而不是非极端的视野)(对于相当广泛的模型)。我们还找到了针对“通常”黑洞($ T = T_ {H} $)的新精确解决方案。讨论中的属性出现在Dilaton重力相互作用的有效常数的\ QTR {it} {weak}耦合机制中。对于某些特殊模型,将2D模型中跟踪到的特征扩展到4D dilaton引力会导致异常的非极端黑洞,这些黑洞没有自己的热特性。

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  • 作者

    Zaslavskii, O B;

  • 作者单位
  • 年度 2002
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  • 原文格式 PDF
  • 正文语种 eng
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