We discuss the entropy-area relation for the small black holes with highercurvature corrections by using the entropy function formalism and fieldredefinition method. We show that the entropy $S_{BH}$ of small black hole isproportional to its horizon area $A$. In particular we find a universal resultthat $S_{BH}=A/2G$, the ratio is two times of Bekenstein-Hawking entropy-areaformula in many cases of physical interest. In four dimensions, the universalrelation is always true irrespective of the coefficients of the higher-orderterms if the dilaton couplings are the same, which is the case for stringeffective theory, while in five dimensions, the relation again holdsirrespective of the overall coefficient if the higher-order corrections are inthe GB combination. We also discuss how this result generalizes to knownphysically interesting cases with Lovelock correction terms in variousdimensions, and possible implications of the universal relation.
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机译:我们使用熵函数形式和场重新定义方法讨论了曲率校正较高的小黑洞的熵-面积关系。我们表明,小黑洞的熵$ S_ {BH} $与视界区域$ A $成正比。特别是,我们发现一个普遍的结果,即$ S_ {BH} = A / 2G $,在许多有实际意义的情况下,该比率是Bekenstein-Hawking熵-面积公式的两倍。在四个维度中,如果dilaton耦合相同,则无论高阶项的系数如何,普适关系始终是正确的,这是字符串有效理论的情况;而在五个维度中,如果更高,则该关系仍然成立,而与总系数无关-订单更正在GB组合中。我们还将讨论此结果如何推广到使用Lovelock校正术语的各个维度的已知物理有趣案例,以及通用关系的可能含义。
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