Abstract
We give general overview of a novel approach, recently developed by us, to address the issue black hole information paradox. This alternative viewpoint is based on theories involving modifications of standard quantum theory, known as “spontaneous dynamical state reduction” or “wave-function collapse models” which were historically developed to overcome the notorious foundational problems of quantum mechanics known as the “measurement problem”. We show that these proposals, when appropriately adapted and refined for this context, provide a self-consistent picture where loss of information in the evaporation of black holes is no longer paradoxical.
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Notes
- 1.
More precisely, region I’, although flat, is also part of the interior of the event horizon as nothing in that region can ever reach \({\mathscr {I}}_R^+\).
- 2.
Up to the regime where we expect the validity of standard space-time notions as provided by General Relativity.
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Acknowledgements
We want to thank our collaborators E. Okon, L. Ortíz, I. Peña, D. Bedingham for their involvement and contribution towards this project. SKM is an International Research Fellow of Japan Society for the Promotion of Science. This research is partly funded by Grant-in-Aid to JSPS fellows (KAKENHI-PROJECT-15F15021). DS acknowledges partial financial support from DGAPA-UNAM project IG100316 and by CONACyT project 101712.
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Modak, S.K., Sudarsky, D. (2017). Modelling Non-paradoxical Loss of Information in Black Hole Evaporation. In: Bagla, J., Engineer, S. (eds) Gravity and the Quantum. Fundamental Theories of Physics, vol 187. Springer, Cham. https://doi.org/10.1007/978-3-319-51700-1_18
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