240 research outputs found

    On generalized Melvin solution for the Lie algebra E6E_6

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    A multidimensional generalization of Melvin's solution for an arbitrary simple Lie algebra G\cal G is considered. The gravitational model in DD dimensions, D4D \geq 4, contains nn 2-forms and lnl \geq n scalar fields, where nn is the rank of G\cal G. The solution is governed by a set of nn functions Hs(z)H_s(z) obeying nn ordinary differential equations with certain boundary conditions imposed. It was conjectured earlier that these functions should be polynomials (the so-called fluxbrane polynomials). The polynomials Hs(z)H_s(z), s=1,,6s = 1,\dots,6, for the Lie algebra E6E_6 are obtained and a corresponding solution for l=n=6l = n = 6 is presented. The polynomials depend upon integration constants QsQ_s, s=1,,6s = 1,\dots,6. They obey symmetry and duality identities. The latter ones are used in deriving asymptotic relations for solutions at large distances. The power-law asymptotic relations for E6E_6-polynomials at large zz are governed by integer-valued matrix ν=A1(I+P)\nu = A^{-1} (I + P), where A1A^{-1} is the inverse Cartan matrix, II is the identity matrix and PP is permutation matrix, corresponding to a generator of the Z2Z_2-group of symmetry of the Dynkin diagram. The 2-form fluxes Φs\Phi^s, s=1,,6s = 1,\dots,6, are calculated.Comment: 16 pages, Latex, no figures, prepared for a talk at RUSGRAV-16 conference in Kaliningrad, 2017, 2nd. revised version, several typos are eliminate

    Classification of Dimension 5 Lorentz Violating Interactions in the Standard Model

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    We give a complete classification of mass dimension five Lorentz-non-invariant interactions composed from the Standard Model fields, using the effective field theory approach. We identify different classes of Lorentz violating operators, some of which are protected against transmutation to lower dimensions even at the loop level. Within each class of operators we determine a typical experimental sensitivity to the size of Lorentz violation.Comment: 26 page

    On generalized Melvin solutions for Lie algebras of rank 3

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    Generalized Melvin solutions for rank-33 Lie algebras A3A_3, B3B_3 and C3C_3 are considered. Any solution contains metric, three Abelian 2-forms and three scalar fields. It is governed by three moduli functions H1(z),H2(z),H3(z)H_1(z),H_2(z),H_3(z) (z=ρ2z = \rho^2 and ρ\rho is a radial variable), obeying three differential equations with certain boundary conditions imposed. These functions are polynomials with powers (n1,n2,n3)=(3,4,3),(6,10,6),(5,8,9)(n_1,n_2, n_3) = (3,4,3), (6,10,6), (5,8,9) for Lie algebras A3A_3, B3B_3, C3C_3, respectively. The solutions depend upon integration constants q1,q2,q30q_1, q_2, q_3 \neq 0. The power-law asymptotic relations for polynomials at large zz are governed by integer-valued 3×33 \times 3 matrix ν\nu, which coincides with twice the inverse Cartan matrix 2A12 A^{-1} for Lie algebras B3B_3 and C3C_3, while in the A3A_3 case ν=A1(I+P)\nu = A^{-1} (I + P), where II is the identity matrix and PP is a permutation matrix, corresponding to a generator of the Z2\mathbb{Z}_2-group of symmetry of the Dynkin diagram. The duality identities for polynomials and asymptotic relations for solutions at large distances are obtained. 2-form flux integrals over a 22-dimensional disc of radius RR and corresponding Wilson loop factors over a circle of radius RR are presented.Comment: 10 pages, Latex, 1 figure; 5th version: the abstract in the Latex file is corrected. arXiv admin note: text overlap with arXiv:1706.0785
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