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Compact scalar field solutions in EiBI gravity

机译:EIBI重力中紧凑的标量场解决方案

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摘要

We discuss exact scalar field solutions describing gravitating compact objects in the Eddington-inspired Born-Infeld (EiBI) gravity, a member of the class of (metric-affine formulated) Ricci-based gravity (RBG) theories. We include a detailed account of the RBGs/GR correspondence exploited to analytically solve the field equations. The single parameter epsilon of the EiBI model defines two branches for the solution. The epsilon > 0 branch may be described as a "shell with no interior", and constitutes an ill-defined, geodesically incomplete spacetime. The more interesting epsilon < 0 branch admits the interpretation of a "wormhole membrane", an exotic horizonless compact object with the ability to transfer particles and light from any point on its surface (located slightly below the would-be Schwarzschild radius) to its antipodal point, in a vanishing fraction of proper time. This is a single example illustrating how the structural modifications introduced by the metric-affine formulation may lead to significant departures from General relativity (GR) even at astrophysically relevant scales, giving rise to physically plausible objects radically different from those we are used to think of in the metric approach, and that could act as a black hole mimickers whose shadows might present distinguishable signals.
机译:我们讨论了描述Eddington-Inspired-Infeld(EIBI)重力中引力的精确标量现场解决方案,这是(公制仿射制定的)基于RICCI的重力(RBG)理论的成员。我们包括利用分析字段方程的RBGS / GR对应的详细说明。 EIBI模型的单个参数epsilon定义了解决方案的两个分支。 epsilon> 0分支可以被描述为“没有内部的壳”,并且构成了一个不定的高音点不完整的时空。更有趣的epsilon <0分支承认了一个“虫孔膜”的解释,一个异国风景的紧凑型物体,具有转移颗粒和光从其表面上的任何点的颗粒和光线(位于略低于什瓦尔兹氏士半径)到其对倾斜的能力点,在适当时间的消失的分数。这是一个例子,其说明了由公制仿射制剂引入的结构修改如何导致通用相对论(GR)的显着偏离,即使在天体物理学相关的尺度上,也产生了与我们习惯的那些完全不同的物理似品对象在公制方法中,这可以充当黑洞模仿者,其阴影可能出现可区分信号。

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