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arXiv 2012.02355hep-thgr-qc

软引力子交换与信息悖论

Soft graviton exchange and the information paradox

Nava Gaddam, Nico Groenenboom

AI总结:

本文提出黑洞 eikonal 相,通过在视界附近对无穷多虚软引力子阶梯图重求和,非微扰地计算了 $2 \rightarrow 2$ 散射 S 矩阵,发现其为纯相位,从而揭示霍金几何光学近似所忽略的引力相互作用对信息悖论的影响。

摘要:

我们证明,量子引力中存在一个显著的相:当碰撞参数 $b$ 满足 $L_{Pl}\ll b \lesssim R_S$(其中 $R_S$ 为史瓦西半径)时,由虚引力子传递的引力散射振幅可以在有效场论中显式计算。该相描述的是视界附近能量满足 $\sqrt{s}\gg γM_{Pl}$(其中 $γ\sim M_{Pl}/M_{BH}$)的碰撞。我们称之为黑洞 eikonal 相,以区别于其平直空间对应物——那里碰撞是跨普朗克能量的。霍金的几何光学近似忽略了视界附近的引力相互作用,并导致 Bogoliubov 系数中出现热占据数。我们证明,这些相互作用由视界附近 $2 \rightarrow 2$ 散射中的引力子交换传递,并在 $M_{Pl}/M_{BH}$ 中非微扰地显式计算了 S 矩阵。这涉及对视界附近无穷多阶梯图的重求和,所有这些图都由虚软引力子传递。经过这一重求和后,S 矩阵表现为一个纯相位,并且对普朗克物理和任何具体的紫外完备不敏感。与平直空间 eikonal 极限不同,黑洞 eikonal 相描述的是视界附近极低能量的碰撞。

英文摘要:

We show that there is a remarkable phase in quantum gravity where gravitational scattering amplitudes mediated by virtual gravitons can be calculated explicitly in effective field theory, when the impact parameter $b$ satisfies $L_{Pl}\ll b \lesssim R_S$, with $R_S$ being the Schwarzschild radius. This phase captures collisions with energies satisfying $\sqrt{s}\gg γM_{Pl}$ (with $γ\sim M_{Pl}/M_{BH}$) near the horizon. We call this the black hole eikonal phase, in contrast to its flat space analogue where collisions are trans-Planckian. Hawking's geometric optics approximation neglects gravitational interactions near the horizon, and results in thermal occupation numbers in the Bogoliubov coefficients. We show that these interactions are mediated by graviton exchange in $2 \rightarrow 2$ scattering near the horizon, and explicitly calculate the S-matrix non-perturbatively in $M_{Pl}/M_{BH}$. This involves a re-summation of infinitely many ladder diagrams near the horizon, all mediated by virtual soft gravitons. The S-matrix turns out to be a pure phase upon this re-summation and is agnostic of Planckian physics and any specific ultraviolet completion. In contrast to the flat space eikonal limit, the black hole eikonal phase captures collisions of extremely low energy near the horizon.

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