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Skyrmion black hole hair: Conservation of baryon number by black holes and observable manifestations

机译:Skyrmion黑洞毛发:通过黑洞和可观察到的表现来保护重子数

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We show that the existence of black holes with classical skyrmion hair invalidates standard proofs that global charges, such as the baryon number, cannot be conserved by a black hole. By carefully analyzing the standard arguments based on a Gedankenexperiment in which a black hole is seemingly-unable to return the baryon number that it swallowed, we identify inconsistencies in this reasoning, which does not take into the account neither the existence of skyrmion black holes nor the baryon/skyrmion correspondence. We then perform a refined Gedankenexperiment by incorporating the new knowledge and show that no contradiction with conservation of baryon number takes place at any stage of black hole evolution. Our analysis also indicates no conflict between semi-classical black holes and the existence of baryonic gauge interaction arbitrarily-weaker than gravity. Next, we study classical cross sections of a minimally-coupled massless probe scalar field scattered by a skyrmion black hole. We investigate how the skyrmion hair manifests itself by comparing this cross section with the analogous cross section caused by a Schwarzschild black hole which has the same ADM mass as the skyrmion black hole. Here we find an order-one difference in the positions of the characteristic peaks in the cross sections. The peaks are shifted to smaller scattering angles when the skyrmion hair is present. This comes from the fact that the skyrmion hair changes the near horizon geometry of the black hole when compared to a Schwarzschild black hole with same ADM mass. We keep the study of this second aspect general so that the qualitative results which we obtain can also be applied to black holes with classical hair of different kind. (C) 2016 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license.
机译:我们证明了古典天sky头发的黑洞的存在使标准证据无效,即黑洞不能守恒诸如重子数之类的全局电荷。通过基于Gedanken实验仔细分析标准参数,在该实验中黑洞似乎无法返回吞下的重子数,因此我们在这种推理中发现了不一致之处,这既没有考虑到存在色子黑洞也没有考虑到重子/ skyrmion对应。然后,我们通过吸收新知识进行完善的Gedanken实验,并表明在黑洞演化的任何阶段都不会发生与重子数守恒的矛盾。我们的分析还表明,半经典黑洞与重子规相互作用的存在比重力任意弱之间没有冲突。接下来,我们研究由天rm黑洞散射的最小耦合无质量探针标量场的经典截面。通过比较该横截面与由Schwarzschild黑洞引起的类似横截面,该横截面具有与Skyrmion黑洞相同的ADM质量,我们研究了该横截面是如何表现出来的。在这里,我们发现截面中特征峰的位置存在一阶差异。当存在天敌头发时,峰移动到较小的散射角。这是因为与具有相同ADM质量的Schwarzschild黑洞相比,天蝎子的头发会改变黑洞的近视层几何形状。我们将继续对第二方面进行研究,以便将获得的定性结果也可以应用于具有不同类型经典头发的黑洞。 (C)2016作者。由Elsevier B.V.发布。这是CC BY许可下的开放获取文章。

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