000069757 001__ 69757 000069757 005__ 20190709135618.0 000069757 0247_ $$2doi$$a10.1103/PhysRevD.96.105001 000069757 0248_ $$2sideral$$a104790 000069757 037__ $$aART-2017-104790 000069757 041__ $$aeng 000069757 100__ $$0(orcid)0000-0003-3669-6241$$aAsorey, M.$$uUniversidad de Zaragoza 000069757 245__ $$aLocalization of observables in the Rindler wedge 000069757 260__ $$c2017 000069757 5060_ $$aAccess copy available to the general public$$fUnrestricted 000069757 5203_ $$aOne of the striking features of QED is that charged particles create a coherent cloud of photons. The resultant coherent state vectors of photons generate a nontrivial representation of the localized algebra of observables that do not support a representation of the Lorentz group: Lorentz symmetry is spontaneously broken. We show in particular that Lorentz boost generators diverge in this representation, a result shown also by Balachandran et al. [Eur. Phys. J. C 75, 89 (2015)EPCFFB1434-604410.1140/epjc/s10052-015-3305-0] (see also the work by Balachandran et al. [Mod. Phys. Lett. A 28, 1350028 (2013)MPLAEQ0217-732310.1142/S0217732313500284]. Localization of observables, for example in the Rindler wedge, uses Poincaré invariance in an essential way [Int. J. Geom. Methods Mod. Phys. 14, 1740008 (2017).0219-887810.1142/S0219887817400084]. Hence, in the presence of charged fields, the photon observables cannot be localized in the Rindler wedge. These observations may have a bearing on the black hole information loss paradox, as the physics in the exterior of the black hole has points of resemblance to that in the Rindler wedge. 000069757 536__ $$9info:eu-repo/grantAgreement/ES/DGA/E24-2$$9info:eu-repo/grantAgreement/ES/MINECO/FPA2015-65745-P 000069757 540__ $$9info:eu-repo/semantics/openAccess$$aAll rights reserved$$uhttp://www.europeana.eu/rights/rr-f/ 000069757 590__ $$a4.394$$b2017 000069757 591__ $$aASTRONOMY & ASTROPHYSICS$$b15 / 66 = 0.227$$c2017$$dQ1$$eT1 000069757 591__ $$aPHYSICS, PARTICLES & FIELDS$$b7 / 29 = 0.241$$c2017$$dQ1$$eT1 000069757 592__ $$a1.801$$b2017 000069757 593__ $$aPhysics and Astronomy (miscellaneous)$$c2017$$dQ1 000069757 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/publishedVersion 000069757 700__ $$aBalachandran, A.P. 000069757 700__ $$aMarmo, G. 000069757 700__ $$aDe Queiroz, A.R. 000069757 7102_ $$12004$$2405$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Física Teórica 000069757 773__ $$g96, 10 (2017), 105001 [5 pp]$$pPhys. rev. D$$tPHYSICAL REVIEW D$$x2470-0010 000069757 8564_ $$s116631$$uhttps://zaguan.unizar.es/record/69757/files/texto_completo.pdf$$yVersión publicada 000069757 8564_ $$s106031$$uhttps://zaguan.unizar.es/record/69757/files/texto_completo.jpg?subformat=icon$$xicon$$yVersión publicada 000069757 909CO $$ooai:zaguan.unizar.es:69757$$particulos$$pdriver 000069757 951__ $$a2019-07-09-12:26:30 000069757 980__ $$aARTICLE