高导数引力理论中的ISCOs和弱引力猜想界

IF 4.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Adrinil Paul, Chandrasekhar Bhamidipati
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引用次数: 0

摘要

本文研究了高导数引力理论中球对称AdS黑洞中带电粒子的圆轨道及其极限ISCOs(最内层稳定圆轨道)。对偶解释是在大自旋极限下的重-轻双扭共形场理论(CFT)算符,在一定的大轨道极限下,其异常维数可以从体中带电探针的结合能中提取出来。要求异常维数的正性,得到了黑洞背景下探测粒子电荷质量比q -的精确界,该界与WGC界相匹配。我们发现,随着耦合参数的导数越高,q -值越大,这一点在高斯-邦纳重力方程中得到了明确的验证。对于现有的探测粒子在AdS背景下的计算,我们发现的异常维数和WGC界,特别是在高斯-博内理论中,与最近对史瓦西AdS[1]、带电AdS[2]和中性高斯-博内黑洞在AdS[3]中的计算在适当的极限上是一致的。最后,我们证明了isco的存在,直到WGC界所设定的极限,它们的半径随着耦合参数的增加而减小,我们明确地验证了高斯-邦纳黑洞在AdS中的情况。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
ISCOs and the weak gravity conjecture bound in higher derivative theories of gravity
We study circular orbits of charged particles in spherically symmetric AdS black holes in higher derivative theories of gravity, and their limiting ISCOs (innermost stable circular orbits). The dual interpretation is in terms of heavy-light double twist conformal field theory (CFT) operators in the large spin limit, whose anomalous dimensions can be extracted from the binding energy of charged probes in the bulk, in a certain large orbit limit. Demanding the positivity of the anomalous dimensions, leads to an exact bound for the charge to mass ratio qˆ of probe particles in the black hole backgrounds, which matches with the WGC bound. We find that qˆ increases with the higher derivative coupling parameters, which is explicitly checked in the Gauss-Bonnet gravity. For existing computations with probe particles in AdS backgrounds, the anomalous dimension and the WGC bound we find, particularly in Gauss-Bonnet theories, are in agreement in appropriate limits with the recent computations for Schwarzschild AdS [1], charged AdS [2] and neutral Gauss-Bonnet black holes in AdS [3]. Finally, we show that the ISCOs exist until the limit set by the WGC bound, with their radius decreasing with coupling parameters, which we check explicitly for the case of Gauss-Bonnet black holes in AdS.
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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