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arXiv 2310.03483hep-thgr-qc

CFT$_2$中运动镜的相对论动力学:量子反作用与黑洞

Relativistic dynamics of moving mirrors in CFT$_2$: quantum backreaction and black holes

Piyush Kumar, Ignacio A. Reyes, Jakob Wintergerst

AI总结:

本文研究1+1维CFT中与相对论性边界粒子相互作用的运动镜动力学,求解其轨迹与场的反射能量-动量,发现量子反作用可避免经典层面的视界形成,还分析了平均类光能量条件的边界项形式。

摘要:

黑洞蒸发物理学与量子场论(QFT)中运动镜的物理学之间存在众所周知的对应关系。然而,该领域的大多数分析都依赖于预设的镜轨迹。本文中,我们研究了1+1维共形场论(Conformal Field Theories, CFT)与一个质量为$m$、充当理想镜的相对论性边界粒子相互作用时的平直空间动力学。该边界粒子的轨迹并非固定,而是遵循其自身的相对论运动方程$F^μ=ma^μ$。对于过去类光无穷远处的给定初始条件,我们求出了边界粒子的轨迹以及量子场的反射能量-动量。对于入射真空态,该解给出了对应于极端黑洞的镜轨道。对于一类在经典层面上会产生在有限固有时内变为类光的轨道(对应于视界的形成)的入射态,量子反作用会避免这一终点,使得镜在光锥坐标下的速度保持有限。我们还研究了平均类光能量条件(Averaged Null Energy Condition)的行为,在该设定下它可简化为一个边界项。

英文摘要:

There is a well-known correspondence between the physics of black hole evaporation and that of moving mirrors in QFT. However, most analyses in this subject rely on prescribed mirror trajectories. Here, we study the flat-space dynamics of $1+1$-dimensional Conformal Field Theories interacting with a relativistic boundary particle of mass $m$ acting as a perfect mirror. The trajectory of the latter is not fixed but follows its own relativistic equation of motion $F^μ=ma^μ$. For given initial conditions at past null infinity, we find the boundary particle's trajectory and the reflected energy-momentum of the quantum fields. For incoming vacuum states, the solution yields mirror orbits that correspond to extremal black holes. For the class of incoming states that produce orbits becoming null in finite proper time -- corresponding to the formation of a horizon -- at the classical level, the quantum backreaction avoids this endpoint rendering the mirror's velocity in lightcone coordinates finite. We investigate the behavior of the Averaged Null Energy Condition, which in this setup reduces to a boundary term.

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。

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