2015
DOI: 10.1140/epjc/s10052-015-3305-0
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Spontaneous Lorentz violation: the case of infrared QED

Abstract: It is by now clear that infrared sector of QED has an intriguingly complex structure. Based on earlier pioneering works on this subject, two of us recently proposed a simple modification of QED by constructing a generalization of the U (1) charge group of QED to the "Sky" group incorporating the known spontaneous Lorentz violation due to infrared photons, but still compatible in particular with locality [1]. There it was shown that the "Sky" group is generated by the algebra of angle dependent charges and a st… Show more

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Cited by 23 publications
(34 citation statements)
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References 33 publications
(48 reference statements)
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“…In general there can be a lot of parameters in a quantum field theory with Lorentz violation [57,58]. Here we consider only the following Lagrangian:…”
Section: Constraint On Lorentz Violation Parametermentioning
confidence: 99%
“…In general there can be a lot of parameters in a quantum field theory with Lorentz violation [57,58]. Here we consider only the following Lagrangian:…”
Section: Constraint On Lorentz Violation Parametermentioning
confidence: 99%
“…This can also be compared with the formulation of Bagan et al [17]. As pointed out in the Introduction this analysis with exact massless QED is beset with problems like Lorentz symmetry violation [10,18]. The analysis of limit of massive QED to massless is better understood when we use lightcone quantisation.…”
Section: Discussionmentioning
confidence: 96%
“…Following there are several interesting questions that have been posed in understanding BMS symmetries in gravity [9], effective action in QFT's and gauge theories including non abelian gauge theories. Balachandran et al [10] have pointed out the exact massless photon QED may violate Lorentz symmetry. Similar analysis also leads to color symmetry being broken [11].…”
Section: Introductionmentioning
confidence: 99%
“…We can generate such elements of G 0 by letting µ(x) approach an angle dependent limit µ ∞ (n), as indicated by (2.11). Then on exponentiation, and restrictingn to a Cauchy slice, we get the Sky group of [10,11] isomorphic to the maps from the celestial sphere S 2 ∞ at infinity to U(1). As µ runs over its possibilities, we get a collection of Sky charges µ ∞ (n) wheren now fixes the representation of G 0 /G ∞ 0 .…”
Section: Jhep07(2018)083mentioning
confidence: 99%
“…It is important that the redundant degrees of freedom implicit in the Lagrangian do not appear at the level of local observables [2,10,11]. They must by definition commute with G(Λ), but because of the locality, they then commute also with Q(µ).…”
Section: On Gauge Redundancies In Qedmentioning
confidence: 99%