论文标题

重组中重力的重组条件

Conditions for graviton emission in the recombination of a delocalized mass

论文作者

Pesci, Alessandro

论文摘要

在已知的Gedanken实验中,将其重组重组时,由另一个(遥远)粒子探测的重力。在其中,这用于探索互补性和因果关系之间可能的张力,以防引力场与超塑位置纠缠在一起,提出的分辨率是四极矩的重力发射。在这里,我们专注于离域粒子(忘记了探针和Gedanken实验),并探讨了重力发射的条件(就质量,分离和重组时间而言)。通过这种情况,我们发现,如果磁场纠缠在一起,则重组中四极力矩的变化通常会大大增强,而不是通过到达态度的能量动量期望值(Moment Moment $ \ sim M \,sim m m \,d^2 $ n y sath sand the ys $ m $ $ $,$ d $,$ d $ sapeption nate nate contriation $ \ sim m \,d^2 $)。此外,我们还获得了(上)限制重组时间的重组时间,将其增长为$ m $,以代替幼稚的期望$ \ sqrt {m} $。在这种情况下,普朗克质量充当阈值质量(巨大,用于离域物体):在其下方没有重力发射,无论重组是否会发生速度。如果将其与Diósi和Penrose(基本形式)的塌陷模型中预见的衰减时间进行了比较,则发现其中可能没有重组会产生(四极杆)的引力。的确,当$ m $变得足够大以允许排放时,它也变得太大,无法在倒塌的情况下生存足够长以重组。

In a known gedanken experiment, a delocalized mass is recombined while the gravitational field sourced by it is probed by another (distant) particle; in it, this is used to explore a possible tension between complementarity and causality in case the gravitational field entangles with the superposed locations, a proposed resolution being graviton emission from quadrupole moments. Here, we focus on the delocalized particle (forgetting about the probe and the gedanken experiment) and explore the conditions (in terms of mass, separation, and recombination time) for graviton emission. Through this, we find that the variations of quadrupole moments in the recombination are generically greatly enhanced if the field is entangled compared to if it is sourced instead by the energy momentum expectation value on the delocalized state (moment variation $\sim m \, d^2$ in the latter case, with $m$ mass, $d$ separation). In addition, we obtain the (upper) limit recombination time for graviton emission growing as $m$ in place of the naive expectation $\sqrt{m}$. In this, the Planck mass acts as threshold mass (huge, for delocalized objects): no graviton emission is possible below it, however fast the recombination occurs. If this is compared with the decay times foreseen in the collapse models of Diósi and Penrose (in their basic form), one finds that no (quadrupole) graviton emission from recombination is possible in them. Indeed, right when $m$ becomes large enough to allow for emission, it also becomes too large for the superposition to survive collapse long enough to recombine.

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