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|a (TOE)ost861193
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|a E 1.99:lbnl--54209
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|a E 1.99:lbnl--54209
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|a lbnl--54209
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|a Massive gravity on a brane
|h [electronic resource]
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|a Berkeley, Calif. :
|b Lawrence Berkeley National Laboratory ;
|a Oak Ridge, Tenn. :
|b distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy,
|c 2003.
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|a text
|b txt
|2 rdacontent.
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|a computer
|b c
|2 rdamedia.
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|a online resource
|b cr
|2 rdacarrier.
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|a Published through the Information Bridge: DOE Scientific and Technical Information.
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|a 12/11/2003.
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|a "lbnl--54209"
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|a ": KA1401020"
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|a Physical Review D 70 FT.
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|a Journal Publication Date: 2004.
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|a Graesser, M.L.; Chacko, Z.; Grojean, C.; Pilo, L.
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|a USDOE Director. Office of Science. Office of High EnergyPhysics. Contracts DE-AC03-76SF00098 and DE-FG03-92ER40701.
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| 500 |
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|a ResearchTraining Network European Program HPRN-CT-2000-00148, Actions ConcerteesIncitatives Jeunes Chercheurs 2068.
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| 520 |
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|a At present no theory of a massive graviton is known that is consistent with experiments at both long and short distances. The problem is that consistency with long distance experiments requires the graviton mass to be very small. Such a small graviton mass however implies an ultraviolet cutoff for the theory at length scales far larger than the millimeter scale at which gravity has already been measured. In this paper we attempt to construct a model which avoids this problem. We consider a brane world setup in warped AdS spacetime and we investigate the consequences of writing a mass term for the graviton on a the infrared brane where the local cutoff is of order a large (galactic) distance scale. The advantage of this setup is that the low cutoff for physics on the infrared brane does not significantly affect the predictivity of the theory for observers localized on the ultraviolet brane. For such observers the predictions of this theory agree with general relativity at distances smaller than the infrared scale but go over to those of a theory of massive gravity at longer distances. A careful analysis of the graviton two-point function, however, reveals the presence of a ghost in the low energy spectrum. A mode decomposition of the higher dimensional theory reveals that the ghost corresponds to the radion field. We also investigate the theory with a brane localized mass for the graviton on the ultraviolet brane, and show that the physics of this case is similar to that of a conventional four dimensional theory with a massive graviton, but with one important difference: when the infrared brane decouples and the would-be massive graviton gets heavier than the regular Kaluza-Klein modes, it becomes unstable and it has a finite width to decay off the brane into the continuum of Kaluza-Klein states.
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|b DE-AC02-05CH11231.
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|b PTHOPS.
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|a Gravitons.
|2 local.
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|a Space-time.
|2 local.
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|a Physics.
|2 local.
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|a Decay.
|2 local.
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| 650 |
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|a Physics Of Elementary Particles And Fields.
|2 edbsc.
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| 710 |
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|a Lawrence Berkeley National Laboratory.
|4 res.
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| 710 |
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|a United States.
|b Department of Energy.
|b Office of Scientific and Technical Information.
|4 dst.
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| 856 |
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|u http://www.osti.gov/servlets/purl/861193-3NusRS/
|z Online Access
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| 907 |
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|a .b69990335
|b 03-06-23
|c 03-31-12
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| 998 |
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|a web
|b 03-31-12
|c f
|d m
|e p
|f eng
|g cau
|h 0
|i 1
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|a Information bridge
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|s 3c1d6b4f-7960-5c7d-9935-ef864302f9da
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| 952 |
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|p Can circulate
|a University of Colorado Boulder
|b Online
|c Online
|d Online
|e E 1.99:lbnl--54209
|h Superintendent of Documents classification
|i web
|n 1
|
