Emission rates, the Correspondence Principle and the Information Paradox

Samir D. Mathur

doi:10.1016/s0550-3213(98)00336-8

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arXiv · hep-th/9706151

Emission rates, the Correspondence Principle and the Information Paradox

Samir D. Mathur

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Abstract

When we vary the moduli of a compactification it may become entropically favourable at some point for a state of branes and strings to rearrange itself into a new configuration. We observe that for the elementary string with two large charges such a rearrangement happens at the `correspondence point' where the string becomes a black hole. For smaller couplings it is entropically favourable for the excitations to be vibrations of the string, while for larger couplings the favoured excitations are pairs of solitonic 5-branes attached to the string; this helps resolve some recently noted difficulties with matching emission properties of the string to emission properties of the black hole. We also examine the change of state when a black hole is placed in a spacetime with an additional compact direction, and the size of this direction is varied. These studies suggest a mechanism that might help resolve the information paradox.

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Samir D. Mathur. 1997-06-23. Emission rates, the Correspondence Principle and the Information Paradox. https://doi.org/10.1016/s0550-3213(98)00336-8

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