论文标题

将“大”黑洞分为七个家庭

Classification of "large" black holes into seven families

论文作者

Li, Dafa, Cheng, Maggie, Li, Xiongrong, Li, Shuwang

论文摘要

事实证明,黑洞 - Qubit对应关系是``可用于通过利用其他方法的方法来获取弦黑洞理论和量子信息理论的更多见解。与本文的三个量子位的分类相比,我们在当地的单一操作(LU)下得出了三个Quibits的纠缠家族,并使用黑洞 - Qubit-Qubit对应\ TextQuotedBllleft the theckequotedblleft the feftledequotedblright \尤其是七个黑孔($ quan)。 $p^{1}$, $p^{2}$, and $p^{3}$) are LU equivalent if their difference is only in the signs of charges. Thus, the classification of black holes is independent of the signs of charges and is only related to the ratio of the absolute values of charges. This observation simplifies the classification task, as one would only need to consider either the classification of non-BPS black holes or the classification BPS的黑洞,但两者都可以通过LU分类,可以观察到这种黑洞的物理基础,而黑洞熵与von Neumann的距离之间的关系可以揭示出与Slocc分类相比,我们的物理连接更加直接。七个家庭,找到具有最大的冯·诺伊曼纠缠熵的黑洞。

The black-hole--qubit correspondence has been proven to be ``useful for obtaining additional insight into one of the string black hole theory and quantum information theory by exploiting approaches of the other"[Phys. Rev. D 82, 026003 (2010)]. Though different classes of stringy black holes can be related to the well-known stochastic local operations and classical communication (SLOCC) entanglement classes of pure states, the string theory requires a more detailed classification than the SLOCC classification of three qubits. In this paper, we derive the entanglement family of three qubits under local unitary operations (LU), and use the black-hole--qubit correspondence to classify \textquotedblleft large\textquotedblright\ black holes into seven inequivalent families. In particular, we show that two black holes with 4 non-vanishing charges ($q_{0}$, $p^{1}$, $p^{2}$, and $p^{3}$) are LU equivalent if their difference is only in the signs of charges. Thus, the classification of black holes is independent of the signs of charges and is only related to the ratio of the absolute values of charges. This observation simplifies the classification task, as one would only need to consider either the classification of non-BPS black holes or the classification of BPS black holes, but not both. Moreover, through the LU classification, the physical basis for this black-hole--qubit correspondence can be observed, and a relation between the black-hole entropy and the von Neumann entanglement entropy is revealed. Therefore, the LU classification offers a more straightforward physical connection than the SLOCC classification. Based on the LU classification, we further study the properties of von Neumann entanglement entropy for each of the seven families, and find the black holes with the maximal von Neumann entanglement entropy.

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