论文标题
在改进的动态方法中，量子黑色和白洞视野的不存在
Nonexistence of quantum black and white hole horizons in an improved dynamic approach
论文作者
论文摘要
在本文中，我们研究了在改进的动态方法的框架内，在爱因斯坦经典理论中曾经出现的古典黑洞地平线附近的量子几何效应，在该框架内，黑洞的内部区域由Kantowski-Sachs（ks）Spacetime（ks）Spacetime（KS）和两种聚合参数进行了函数。我们的详细分析表明，这些效果是如此强烈，以至于根本不存在有效量子理论的黑色和白孔地平线，而是被过渡表面所取代，该表面的度量系数及其对流且它们的平滑且保持有限，以及相应的曲率，包括Kretschmann标量。这些表面总是将被困的区域与反捕获的区域分开。此类表面的数量是无限的，因此相应的KS空间在地球上完成，并且该方案中没有黑色和白色孔状结构。
In this paper, we study the quantum geometric effects near the locations where classical black hole horizons used to appear in Einstein's classical theory, within the framework of an improved dynamic approach, in which the internal region of a black hole is modeled by the Kantowski-Sachs (KS) spacetime and the two polymerization parameters are functions of the phase space variables. Our detailed analysis shows that the effects are so strong that black and white hole horizons of the effective quantum theory do not exist at all and instead are replaced by transition surfaces, across which the metric coefficients and their inverses are smooth and remain finite, as are the corresponding curvatures, including the Kretschmann scalar. These surfaces always separate trapped regions from anti-trapped regions. The number of such surfaces is infinite, so the corresponding KS spacetimes become geodesically complete, and no black and white hole-like structures exist in this scheme.
