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On arithmetic detection of grey pulses with application to Hawking radiation

dc.contributor.authorRosu Barbus, Haret-Codratian
dc.contributor.authorMichel Planat
dc.contributor.editorWorld Scientific Publishing Company
dc.date.accessioned2018-03-21T23:42:30Z
dc.date.available2018-03-21T23:42:30Z
dc.date.issued2002
dc.identifier.citationHARET C. ROSU and MICHEL PLANAT, Mod. Phys. Lett. A 17, 1377 (2002).
dc.identifier.urihttp://hdl.handle.net/11627/3502
dc.description.abstract"Micron-sized black holes do not necessarily have a constant horizon temperature distribution. The black hole remote-sensing problem means to find out the "surface" temperature distribution of a small black hole from the spectral measurement of its (Hawking) grey pulse. This problem has been previously considered by Rosu, who used Chen's modified Möbius transform inverse transform. Here, we hint on a Ramanujan generalization of Chen's modified Möbius transform inverse transform that may be considered as a special wavelet processing of the remote-sensed grey signal coming from a black hole or any other distant grey source."
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.subjectMöbius transform
dc.subjectRamanujan sums
dc.subjectGrey-body
dc.subjectHawking radiation
dc.subjectBlack hole
dc.subject.classificationFÍSICA
dc.titleOn arithmetic detection of grey pulses with application to Hawking radiation
dc.typearticle
dc.identifier.doihttps://doi.org/10.1142/S0217732302007430
dc.rights.accessAcceso Abierto


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Attribution-NonCommercial-NoDerivatives 4.0 Internacional
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivatives 4.0 Internacional