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Probing microstructure of black hole spacetimes with gravitational wave echoes

机译:用引力波回波探测黑洞空间的微观结构

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Quantum nature of black hole horizons has been a subject of recent interest and scrutiny. In particular, a near-horizon quantum violation of the equivalence principle has been proposed as a resolution of the black hole information paradox. Such a violation may lead to a modified dispersion relation at high energies,which could become relevant due to the intense gravitational blueshift experienced by ingoing gravitational waves.We investigate the ringdown for a perturbed black hole with such a modified dispersion relation and find that infalling gravitational waves are partially reflected near the horizon. This results in the appearance of late-time echoes in the ringdown phase of black hole merger events, with similar properties to those (arguably) seen in the Advanced LIGO observations. Current measurements suggest a Lorentz-violation scale of 10~(13±2) GeV for gravitational waves, with comparable dissipation and dispersion. Therefore, if confirmed, black hole ringdown echoes probe the microstructure of horizons and thus can test Lorentzviolating UV completions.
机译:黑洞视界量子性质一直是近期备受关注和监察的对象。特别是,近水平面量子违反了等价原理已被提议作为黑洞悖论信息的分辨率。这样的冲突可能导致在高能量修改色散关系,以强烈的引力蓝移经历由迁入引力waves.We调查振铃的扰动黑洞这种改进的色散关系,找到下落的引力可能成为因有关波地平线附近部分地反射。这将导致后期时间的回波的黑洞合并事件的振铃阶段的外观,具有类似特性的那些(可以说)出现在高级LIGO观测。电流测量建议的10〜(13±2)GeV的引力波洛伦兹违章规模,具有可比的耗散和分散。因此,如果确认,黑洞振铃呼叫回波探测视野的微观结构,因此可以测试Lorentzviolating UV完井。

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