{ "id": "1406.0807", "version": "v1", "published": "2014-06-03T18:21:09.000Z", "updated": "2014-06-03T18:21:09.000Z", "title": "Remnants, Fuzzballs or Wormholes?", "authors": [ "Samir D. Mathur" ], "comment": "7 pages, 4 figures (Essay awarded an honorable mention in the Gravity Research Foundation essay competition 2014)", "categories": [ "hep-th", "gr-qc" ], "abstract": "The black hole information paradox has caused enormous confusion over four decades. But in recent years, the theorem of quantum strong-subaddditivity has sorted out the possible resolutions into three sharp categories: (A) No new physics at $r\\gg l_p$; this necessarily implies remnants/information loss. A realization of remnants is given by a baby Universe attached near $r\\sim 0$. (B) Violation of the `no-hair' theorem by nontrivial effects at the horizon $r\\sim M$. This possibility is realized by fuzzballs in string theory, and gives unitary evaporation. (C) Having the vacuum at the horizon, but requiring that Hawking quanta at $r\\sim M^3$ be somehow identified with degrees of freedom inside the black hole. A model for this `extreme nonlocality' is realized by conjecturing that wormholes connect the radiation quanta to the hole.", "revisions": [ { "version": "v1", "updated": "2014-06-03T18:21:09.000Z" } ], "analyses": { "subjects": [ "04.70.-s" ], "keywords": [ "black hole information paradox", "necessarily implies remnants/information loss", "extreme nonlocality", "freedom inside", "unitary evaporation" ], "tags": [ "journal article" ], "publication": { "doi": "10.1142/S0218271814420243", "journal": "International Journal of Modern Physics D", "year": 2014, "month": "Nov", "volume": 23, "number": 12, "pages": 1442024 }, "note": { "typesetting": "TeX", "pages": 7, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1298977, "adsabs": "2014IJMPD..2342024M" } } }