TY - JOUR
T1 - White holes as remnants
T2 - A surprising scenario for the end of a black hole
AU - Bianchi, Eugenio
AU - Christodoulou, Marios
AU - D'Ambrosio, Fabio
AU - Haggard, Hal M.
AU - Rovelli, Carlo
N1 - Funding Information:
CR thanks Ted Jacobson, Steve Giddings, Gary Horowitz, Steve Carlip, and Claus Kiefer for very useful exchanges during the preparation of this work. EB and HMH thank Tommaso De Lorenzo for discussion of time scales. EB thanks Abhay Ashtekar for discussion of remnants. HMH thanks the CPT for warm hospitality and support, Bard College for extended support to visit the CPT with students, and the Perimeter Institute for Theoretical Physics for generous sabbatical support. MC acknowledges support from the SM Center for Space, Time and the Quantum and the Leventis Educational Grants Scheme. This work is supported by Perimeter Institute for Theoretical Physics. Research at Perimeter Institute is supported by the Government of Canada through Industry Canada and by the Province of Ontario through the Ministry of Research and Innovation.
Publisher Copyright:
© 2018 IOP Publishing Ltd.
PY - 2018/10/19
Y1 - 2018/10/19
N2 - Quantum tunneling of a black hole into a white hole provides a model for the full life cycle of a black hole. The white hole acts as a long-lived remnant, providing a possible resolution to the information paradox. The remnant solution of the paradox has long been viewed with suspicion, mostly because remnants seemed to be such exotic objects. We point out that (i) established physics includes objects with precisely the required properties for remnants: white holes with small masses but large finite interiors; (ii) non-perturbative quantum gravity indicates that a black hole tunnels precisely into such a white hole, at the end of its evaporation. We address the objections to the existence of white-hole remnants, discuss their stability, and show how the notions of entropy relevant in this context allow them to evade several no-go arguments. A black hole's formation, evaporation, tunneling to a white hole, and final slow decay, form a unitary process that does not violate any known physics.
AB - Quantum tunneling of a black hole into a white hole provides a model for the full life cycle of a black hole. The white hole acts as a long-lived remnant, providing a possible resolution to the information paradox. The remnant solution of the paradox has long been viewed with suspicion, mostly because remnants seemed to be such exotic objects. We point out that (i) established physics includes objects with precisely the required properties for remnants: white holes with small masses but large finite interiors; (ii) non-perturbative quantum gravity indicates that a black hole tunnels precisely into such a white hole, at the end of its evaporation. We address the objections to the existence of white-hole remnants, discuss their stability, and show how the notions of entropy relevant in this context allow them to evade several no-go arguments. A black hole's formation, evaporation, tunneling to a white hole, and final slow decay, form a unitary process that does not violate any known physics.
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U2 - 10.1088/1361-6382/aae550
DO - 10.1088/1361-6382/aae550
M3 - Article
AN - SCOPUS:85056142659
SN - 0264-9381
VL - 35
JO - Classical and Quantum Gravity
JF - Classical and Quantum Gravity
IS - 22
M1 - 225003
ER -