2015
DOI: 10.1103/physrevd.92.125006
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Photon self-interaction on deformed spacetime

Abstract: A novel nonlocal four-photon interaction on the deformed spacetime is derived and studied in the three selected models (I, II, III). The first two models (I, II) are obtained via two distinct second-order θ-exact Seiberg-Witten maps of the noncommutative U(1) gauge field strength on Moyal space. The third one (III), inspired by the manifestly gauge invariant structures emerging in the first two, due to the model generality has been constructed with a different set of freedom parameters. The physical relevancy … Show more

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Cited by 16 publications
(34 citation statements)
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“…It turns out that this kink implies the presence of a point charge at the origin via the gravitational junction conditions of f (T ) gravity [54], as the quantities demanded to be continuous in [54] are not all continuous at r = 0 when V (0) = 0. Mathematically this charge is manifest in (21), and figures 4 -8 where the graph insets indicate that r 2 V | r→∞ does not go to zero, and hence an electric charge is present according to (21). One other issue to note is that the effective mass of these solutions, as defined by the integral of ρ, the energy density of the Yang-Mills field, does not converge as strongly as in the purely magnetic counter-parts.…”
Section: Iiiii the Solutionsmentioning
confidence: 97%
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“…It turns out that this kink implies the presence of a point charge at the origin via the gravitational junction conditions of f (T ) gravity [54], as the quantities demanded to be continuous in [54] are not all continuous at r = 0 when V (0) = 0. Mathematically this charge is manifest in (21), and figures 4 -8 where the graph insets indicate that r 2 V | r→∞ does not go to zero, and hence an electric charge is present according to (21). One other issue to note is that the effective mass of these solutions, as defined by the integral of ρ, the energy density of the Yang-Mills field, does not converge as strongly as in the purely magnetic counter-parts.…”
Section: Iiiii the Solutionsmentioning
confidence: 97%
“…However, we find that the successful magnetic solutions having this gravitational vanishing criterion at infinity turn out to indeed meet the condition of no global magnetic charge, as defined by (22). Electric solutions are studied separately below, and will turn out to possess a global electric charge dictated by (21). Utilizing the restrictions discussed above, the following set of mutually compatible conditions are chosen in order to proceed with the asymptotically vanishing evolutions in the next section:…”
Section: Iiii Initial Conditions and Asymptoticsmentioning
confidence: 99%
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“…In the Θ-exact SW map approach, the UV/IR mixing is related to phase factor of distinctive star product between commutative fields. The phenomenological implications of the Θ-exact SW map and properties of UV/IR mixing pursued extensively in ref [20,21]. There are enormous amount of work has been done considering Moyal-Weyl (MW) approach [15,[32][33][34][35][36][37] as well as Seiberg-Witten Map approach [38][39][40][41][42][43][44][45][46][47] in order to remove the UV/IR mixing.…”
Section: Introductionmentioning
confidence: 99%
“…However, there is a case of socalled lightlike unitarity condition, Θ 0i ¼ −Θ 1i , ∀ i ¼ 1, 2, 3 [14], which is regarded as being acceptable with respect to the general unitarity condition of quantum field theories (QFTs) on noncommutative spaces. For Moyal geometry, recently it was proven that there exists a θ-exact formulation of noncommutative gauge field theory based on the Seiberg-Witten map [15][16][17][18][19][20] that preserves unitarity [14], and has improved UV/IR behavior at the quantum level in its supersymmetric version [21][22][23]. Noncommutativity may also have implications on cosmology, as for example through the determination of the maximal decoupling/ coupling temperatures of the right-handed neutrino species in the early universe [24,25].…”
Section: Introductionmentioning
confidence: 99%