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Gravitational waves and higher dimensions: Love numbers and Kaluza-Klein excitations

机译:引力波和更高的尺寸:爱情数字和kaluza-klein刺激

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摘要

Gravitational-wave observations provide a wealth of information on the nature and properties of black holes. Among these, tidal Love numbers or the multipole moments of the inspiraling and final objects are key to a number of constraints. Here, we consider these observations in the context of higher-dimensional scenarios, with flat large extra dimensions. We show that—as might be anticipated, but not always appreciated in the literature—physically motivated setups are unconstrained by gravitational-wave data. Dynamical processes that do not excite the Kaluza-Klein (KK) modes lead to a signal identical to that in four-dimensional general relativity in vacuum. In addition, any possible excitation of the KK modes is highly suppressed relative to the dominant quadrupolar term; given existing constraints on the extra dimensions and the masses of the objects seen in gravitational-wave observations, KK modes appear at post-Newtonian order ~10~(11). Finally, we recompute the tidal Love numbers of spherical black holes in higher dimensions. We confirm that these are different from zero, but comparing with previous computations we find a different magnitude and sign.
机译:引力波观察提供了关于黑洞的性质和性质的丰富信息。其中,潮汐的最佳号码或普遍存器和最终对象的多极矩是许多限制的关键。在这里,我们考虑在高度方案的背景下的这些观察,具有平坦的额外尺寸。我们展示了 - 如可能预期的那样,但在文学 - 物理上动机的设置中并不总是通过引力波数据的无关。不会激发Kaluza-Klein(KK)模式的动态过程导致与真空中的四维一般相对性相同的信号。此外,相对于显性Quadrupolar术语,KK模式的任何可能的激发高度抑制;鉴于在引力波观察中看到的额外尺寸和物体的群体上存在现有约束,KK模式出现在牛顿后〜10〜(11)。最后,我们重新计算了更高尺寸的球形黑洞的潮汐。我们确认这些与零不同,但与先前的计算相比,我们找到了不同的幅度和标志。

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