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A more relevant Samir Mathur paper?
I was checking out other Samir mathur papers and saw this.
"It will be interesting to address dynamical questions with the above picture. It is possible that infalling matter falls straight through the ‘fuzzball’ towards r = 0 (as if it were falling through a conventional horizon), but over the Hawking evaporation time information is transferred to the ‘light fractional modes’ and into the radiation."
No mechanism is proposed for how matter plummeting to the center of the hole should give up its information to the "giant tangle of strings" or whatever dwells in the hole.
but it is "possible" that it some how does transfer its information to the fuzzball or whatever dwelleth in the hole.
Now how might such information be transferred out thru the event horizon and percolate into the Hawking radiation witnessed by the outsider world?
"... we have argued that bound states swell upto a size of order the horizon radius; thus the interior of the horizon is not just ‘empty space with a central singularity’. This makes it possible for radiation from the hole to pick up information from the ‘hair’ and avoid the information paradox."
Again it is suggested to be possible for Hawking radiation leaving the hole to have "picked up"---perhaps the idea is "to be infected by" as one picks up a flu germ---information encoded in the tangle that dwells in the hole.
I guess the possibility is shown by proximity---because the tangle extends out to the horizon where the radiation is. But again no mechanism.
The above quotes are from the conclusions of
"Where are the states of a black hole?"
Samir D. Mathur
7 pages
http://arxiv.org/hep-th/0401115
Abstract: "We argue that bound states of branes have a size that is of the same order as the horizon radius of the corresponding black hole. Thus the interior of a black hole is not `empty space with a central singularity', and Hawking radiation can pick up information from the degrees of freedom of the hole."
My comment:
As yet no mechanism for the info to seep out thru the event horizon and be transcribed into the Hawking radiation.
Hawking radiation is usually considered on theoretical grounds to be "thermal" which means it doesn't carry information----thermal blackbody radiation is the nondescript generic glow corresponding to a given temperature.
thanks to MadIce for calling attention to Mathur's interesting work
I hope everyone checks it out and sees what it actually says.
Salutes to Mathur for ingeniously proposing some string theory getaway
routes---though as yet without means for the information to travel them.
I remain skeptical as to anyone actually having resolved the Info Paradox, at least in the way Mathur and others appear to want it resolved
I was checking out other Samir mathur papers and saw this.
"It will be interesting to address dynamical questions with the above picture. It is possible that infalling matter falls straight through the ‘fuzzball’ towards r = 0 (as if it were falling through a conventional horizon), but over the Hawking evaporation time information is transferred to the ‘light fractional modes’ and into the radiation."
No mechanism is proposed for how matter plummeting to the center of the hole should give up its information to the "giant tangle of strings" or whatever dwells in the hole.
but it is "possible" that it some how does transfer its information to the fuzzball or whatever dwelleth in the hole.
Now how might such information be transferred out thru the event horizon and percolate into the Hawking radiation witnessed by the outsider world?
"... we have argued that bound states swell upto a size of order the horizon radius; thus the interior of the horizon is not just ‘empty space with a central singularity’. This makes it possible for radiation from the hole to pick up information from the ‘hair’ and avoid the information paradox."
Again it is suggested to be possible for Hawking radiation leaving the hole to have "picked up"---perhaps the idea is "to be infected by" as one picks up a flu germ---information encoded in the tangle that dwells in the hole.
I guess the possibility is shown by proximity---because the tangle extends out to the horizon where the radiation is. But again no mechanism.
The above quotes are from the conclusions of
"Where are the states of a black hole?"
Samir D. Mathur
7 pages
http://arxiv.org/hep-th/0401115
Abstract: "We argue that bound states of branes have a size that is of the same order as the horizon radius of the corresponding black hole. Thus the interior of a black hole is not `empty space with a central singularity', and Hawking radiation can pick up information from the degrees of freedom of the hole."
My comment:
As yet no mechanism for the info to seep out thru the event horizon and be transcribed into the Hawking radiation.
Hawking radiation is usually considered on theoretical grounds to be "thermal" which means it doesn't carry information----thermal blackbody radiation is the nondescript generic glow corresponding to a given temperature.
thanks to MadIce for calling attention to Mathur's interesting work
I hope everyone checks it out and sees what it actually says.
Salutes to Mathur for ingeniously proposing some string theory getaway
routes---though as yet without means for the information to travel them.
I remain skeptical as to anyone actually having resolved the Info Paradox, at least in the way Mathur and others appear to want it resolved
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