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The Schwarzschild singularity's resolution has key values in cracking the key mysteries related with black holes, the origin of their horizon entropy and the information missing puzzle involved in their evaporations. We provide in this work the general dynamic inner metric of collapsing stars with horizons and with non-trivial radial mass distributions. We find that static central singularities are not the final state of the system. Instead, the final state of the system is a periodically zero-cross breathing ball. Through 3+1 decomposed general relativity and its quantum formulation, we establish a functional Schrdinger equation controlling the micro-state of this breathing ball and show that, the system configuration with all the matter concentrating on the central point is not the unique eigen-energy-density solution. Using a BohrSommerfield like "orbital" quantisation assumption, we show that for each black hole of horizon radius r(h), there are about e(r2h/l2pl) allowable eigen-energy-density profiles. This naturally leads to physic interpretations for the micro-origin of horizon entropy, as well as solutions to the information missing puzzle involved in Hawking radiations. (C) 2017 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license
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Source :
NUCLEAR PHYSICS B
ISSN: 0550-3213
Year: 2017
Volume: 917
Page: 178-192
2 . 8 0 0
JCR@2022
ESI Discipline: PHYSICS;
ESI HC Threshold:158
CAS Journal Grade:3
Cited Count:
WoS CC Cited Count: 9
SCOPUS Cited Count: 9
ESI Highly Cited Papers on the List: 0 Unfold All
WanFang Cited Count:
Chinese Cited Count:
30 Days PV: 1
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