Area law corrections from state counting and supergravity
Area law corrections from state counting and supergravity
复制标题
来自状态计数和超重力的面积定律修正
DOI：
10.1088/0264-9381/17/5/310
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发表时间：
1999
影响因子：
3.5
通讯作者：
T. Mohaupt
中科院分区：
文献类型：
--
作者：
G. Cardoso;B. Wit;T. Mohaupt
为了找到基于状态计数的微观熵与基于有效场论计算的宏观熵之间的一致性，修正黑洞的贝肯斯坦-霍金面积定律是至关重要的。我们在四维N = 2超对称黑洞的情况下讨论了这一问题和相关问题。我们还简要地评论了N = 4和8黑洞的状态计数。
Modifications of the Bekenstein-Hawking area law for black holes are crucial in order to find agreement between the microscopic entropy based on state counting and the macroscopic entropy based on an effective field theory computation. We discuss this and related issues for the case of four-dimensional N = 2 supersymmetric black holes. We also briefly comment on the state counting for N = 4 and 8 black holes.