2018
DOI: 10.3390/universe4030047
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Asymptotic Charges at Null Infinity in Any Dimension

Abstract: We analyse the conservation laws associated with large gauge transformations of massless fields in Minkowski space. Our aim is to highlight the interplay between boundary conditions and finiteness of the asymptotically conserved charges in any space-time dimension, both even and odd, greater than or equal to three. After discussing nonlinear Yang-Mills theory and revisiting linearised gravity, our investigation extends to cover the infrared behaviour of bosonic massless quanta of any spin.

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Cited by 32 publications
(50 citation statements)
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References 116 publications
(284 reference statements)
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“…For higher d, it was presumed to hold by some authors [3]. However, gauge conditions exist for the Bondi-gauge null-infinity behavior of asymptotically flat spacetimes that render bms(d + 2) finite-dimensional [21], and with this choice ccarr2(d + 1) = bms(d + 2). This does not exclude that less restrictive gauge fixing might be considered leading to other, possibly infinite-dimensional bms(d + 2) algebras for d ≥ 3.…”
Section: Conformal Carrollian Isometriesmentioning
confidence: 99%
“…For higher d, it was presumed to hold by some authors [3]. However, gauge conditions exist for the Bondi-gauge null-infinity behavior of asymptotically flat spacetimes that render bms(d + 2) finite-dimensional [21], and with this choice ccarr2(d + 1) = bms(d + 2). This does not exclude that less restrictive gauge fixing might be considered leading to other, possibly infinite-dimensional bms(d + 2) algebras for d ≥ 3.…”
Section: Conformal Carrollian Isometriesmentioning
confidence: 99%
“…Einstein's equations determine D.D.C (n) , 0 < n < m − 3, recursively in terms of D.D.C (−1) and determine D.D.C (n) , m − 1 < n < 2m − 3, recursively in terms of D.D.C (m−2) (see [29])…”
Section: Conditions For Finiteness Of the Chargementioning
confidence: 99%
“…Extension of the asymptotic analysis to higher dimensions raises interesting issues, which have led to a somewhat unclear situation at null infinity where some studies yield infinitedimensional asymptotic symmetries as in four spacetime dimensions, while some others do not [37][38][39][40][41][42][43][44][45][46]. The question is further complicated in odd spacetime dimensions because half-integer fractional powers of r −1 mix with integer powers, leading to problems with the conformal definition of null infinity [47][48][49], and the frequent necessity to split the analysis according to whether the spacetime dimension is odd or even since only in the latter case does one avoid non-analytic functions at null infinity.…”
Section: Introductionmentioning
confidence: 99%