黑洞及其它巨洞的低频量子引力辐射
Quantized Gravitational Radiation from Black Holes and other Macro Holeums in the Low Frequency Domain
摘要：
引力束缚态，称为巨洞，是由大量的原初或非原初起源的微观黑洞产生的。在重力的作用下，它们都绕着共同的质心作轨道运动。出现了四种类型的巨洞：H，BH，HH和LH。后者是以光速运动的无质量引力能束。其他的是暗物质物体。BH发射霍金辐射，而其他的则没有。目前存在的黑洞被认为是BH。除了LH，所有的都由于内部量子跃迁而发射引力辐射。本文仅用两个可由引力谱确定的参数，导出了巨洞引力辐射的能量本征值、质量、半径、密度和频率的简单解析公式。我们预测，黑洞有内部结构，他们和其他的巨洞，具有57太阳质量的范围内870太阳质量，将发出类似氢的引力辐射在LIGO频率范围内的带或线光谱的形式与相当大的重叠带。这将叠加在来自距离大于100 Mpc的巨洞的均匀背景辐射上。04.60.-公元前四时六十分，四时三十分w，04.30.Tv，95.35.+ d，95.36。+ X
英文摘要：
A gravitational bound state, called a Macro Holeum, is created from a very large number of microscopic black holes of primordial or a non-primordial origin. All of them undergo orbital motion, under the action of gravity, around their common center of mass. Four classes of Macro Holeum emerge: H, BH, HH and LH. The latter is a massless bundle of gravitational energy moving at the speed of light. The others are Dark Matter objects. BH emits Hawking radiation but the others do not. The presently existing black holes are identified with BH. All, except LH, emit gravitational radiation due to internal quantum transitions. Simple analytic formulae are derived for the energy eigenvalues, mass, radius, density and the frequency of the gravitational radiation emitted by Macro Holeums in terms of just two parameters which can be determined from the gravitational spectra. We predict that black holes have internal structure and that they and other Macro Holeums, having masses in the range 57 solar masses to 870 solar masses, would emit hydrogen-like gravitational radiation in the LIGO frequency range in the form of band or line spectra with a considerable overlapping of the bands. This will be superposed on a uniform background radiation coming from Macro Holeums at large distances greater than 100 Mpc. 04.60.-m, 04.60.Bc, 04.30.-w, 04.30.Tv, 95.35.+d, 95.36.+x
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