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The radiation emitted by a black hole (BH) during its evaporation has to have some degree of quantum coherence to accommodate a unitary time evolution.
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S. D. Mathur, “What Exactly is the Information Paradox?,” Lect. Notes Phys. 769
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A. Giveon and N. Itzhaki, “String Theory Versus Black Hole Complementarity,” JHEP 1212
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2013
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2013
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2013
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2012
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R. Brustein and M. Hadad, “Wave function of the quantum black hole,” Phys. Lett. B 718
2012
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D. N. Page, “Black hole information,” hep-th/9305040
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N. Itzhaki, “Is the black hole complementarity principle really necessary?,” hep-th/9607028
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R. Bousso, “Complementarity Is Not Enough,” arXiv:1207.5192 [hep-th]
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K. Larjo, D. A. Lowe and L. Thorlacius, “Black holes without firewalls,” arXiv:1211.4620 [hep-th]
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Cited in the paper.
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