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Title: Can we observe fuzzballs or firewalls?

Journal Article · · Journal of High Energy Physics (Online)
 [1];  [1];  [1]
  1. The Ohio State Univ., Columbus, OH (United States). Dept. of Physics

In the fuzzball paradigm the information paradox is resolved because the black hole is replaced by an object with no horizon. One may therefore ask if observations can distinguish a traditional hole from a fuzzball. We give arguments for why the fuzzball structure should lie close to the horizon; i.e., it should be a ‘tight’ fuzzball. We find: (a) It is very difficult to reflect quanta off the surface of such a fuzzball, mainly because geodesics starting near the horizon radius cannot escape to infinity unless their starting direction is very close to radial. (b) If infalling particles interact with the emerging radiation before they are engulfed by the horizon, then we say that we have a ‘firewall behavior’. Here, we consider several types of interactions, but find no evidence for firewall behavior in any theory that obeys causality. (c) Photons with wavelengths larger than the black hole radius can be scattered off the emerging radiation, but a very small fraction of the backscattered photons will be able to escape back to infinity.

Research Organization:
The Ohio State Univ., Columbus, OH (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
SC0011726
OSTI ID:
1499185
Journal Information:
Journal of High Energy Physics (Online), Vol. 2018, Issue 7; ISSN 1029-8479
Publisher:
Springer BerlinCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 48 works
Citation information provided by
Web of Science

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Cited By (11)

Testing the nature of dark compact objects: a status report journal July 2019
Classical properties of non-local, ghost- and singularity-free gravity journal September 2018
Nonlocal star as a blackhole mimicker journal July 2019
Towards nonsingular rotating compact object in ghost-free infinite derivative gravity journal October 2018
Weak and strong deflection gravitational lensing by a renormalization group improved Schwarzschild black hole journal December 2019
Are quantum corrections on horizon scale physically motivated? journal October 2019
Classical properties of non-local, ghost- and singularity-free gravity text January 2018
Towards nonsingular rotating compact object in ghost-free infinite derivative gravity text January 2018
Nonlocal star as a blackhole mimicker text January 2019
Testing the nature of dark compact objects: a status report text January 2019
Quasinormal modes of supersymmetric microstate geometries from the D1-D5 CFT text January 2019

Figures / Tables (4)


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