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Correspondence Principle for Black Holes in Plane Waves

Akikazu Hashimoto·Leopoldo Pando Zayas
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Abstract

We compare the entropy as a function of energy of excited strings and black strings in an asymptotically plane wave background at the level of the correspondence principle. For the plane wave supported by the NSNS 3-form flux, neither the entropy formula nor the cross-over scale is affected by the presence of the flux and the correspondence is found to hold. For the plane wave supported by the RR 3-form flux, both the entropy and the cross-over point are modified, but the correspondence is still found to hold.

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Akikazu Hashimoto, Leopoldo Pando Zayas. 2004-04-21. Correspondence Principle for Black Holes in Plane Waves. https://doi.org/10.1088/1126-6708%2F2004%2F03%2F014

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