17,343 research outputs found

    Complete Reducibility in Good Characteristic

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    Let GG be a simple algebraic group of exceptional type, over an algebraically closed field of characteristic p≥0p \ge 0. A closed subgroup HH of GG is called GG-completely reducible (GG-cr) if whenever HH is contained in a parabolic subgroup PP of GG, it is contained in a Levi subgroup of PP. In this paper we determine the GG-conjugacy classes of non-GG-cr simple connected subgroups of GG when pp is good for GG. For each such subgroup XX, we determine the action of XX on the adjoint module L(G)L(G) and the connected centraliser of XX in GG. As a consequence we classify all non-GG-cr connected reductive subgroups of GG, and determine their connected centralisers. We also classify the subgroups of GG which are maximal among connected reductive subgroups, but not maximal among all connected subgroups.Comment: 66 pages. To appear in Trans. Amer. Math. So

    Finite subgroups of simple algebraic groups with irreducible centralizers

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    We determine all finite subgroups of simple algebraic groups that have irreducible centralizers - that is, centralizers whose connected component does not lie in a parabolic subgroup.Comment: 24 page

    On the involution fixity of exceptional groups of Lie type

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    The involution fixity ifix(G){\rm ifix}(G) of a permutation group GG of degree nn is the maximum number of fixed points of an involution. In this paper we study the involution fixity of primitive almost simple exceptional groups of Lie type. We show that if TT is the socle of such a group, then either ifix(T)>n1/3{\rm ifix}(T) > n^{1/3}, or ifix(T)=1{\rm ifix}(T) = 1 and T=2B2(q)T = {}^2B_2(q) is a Suzuki group in its natural 22-transitive action of degree n=q2+1n=q^2+1. This bound is best possible and we present more detailed results for each family of exceptional groups, which allows us to determine the groups with ifix(T)â©˝n4/9{\rm ifix}(T) \leqslant n^{4/9}. This extends recent work of Liebeck and Shalev, who established the bound ifix(T)>n1/6{\rm ifix}(T) > n^{1/6} for every almost simple primitive group of degree nn with socle TT (with a prescribed list of exceptions). Finally, by combining our results with the Lang-Weil estimates from algebraic geometry, we determine bounds on a natural analogue of involution fixity for primitive actions of exceptional algebraic groups over algebraically closed fields.Comment: 45 pages; to appear in Int. J. Algebra Compu

    Simulations of Strong Gravitational Lensing with Substructure

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    Galactic sized gravitational lenses are simulated by combining a cosmological N-body simulation and models for the baryonic component of the galaxy. The lens caustics, critical curves, image locations and magnification ratios are calculated by ray-shooting on an adaptive grid. When the source is near a cusp in a smooth lens' caustic the sum of the magnifications of the three closest images should be close to zero. It is found that in the observed cases this sum is generally too large to be consistent with the simulations implying that there is not enough substructure in the simulations. This suggests that other factors play an important role. These may include limited numerical resolution, lensing by structure outside the halo, selection bias and the possibility that a randomly selected galaxy halo may be more irregular, for example due to recent mergers, than the isolated halo used in this study. It is also shown that, with the level of substructure computed from the N-body simulations, the image magnifications of the Einstein cross type lenses are very weak functions of source size up to \sim 1\kpc. This is also true for the magnification ratios of widely separated images in the fold and cusp caustic lenses. This means that selected magnification ratios for different the emission regions of a lensed quasar should agree with each other, barring microlensing by stars. The source size dependence of the magnification ratio between the closest pair of images is more sensitive to substructure.Comment: 28 pages, 2 tables and 14 figures. Accepted to MNRA

    Reversible tuning of the surface state in a psuedo-binary Bi2(Te-Se)3 topological insulator

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    We use angle-resolved photoemission spectroscopy to study non-trivial surface state in psuedobinary Bi2Se0.6Te2.3 topological insulator. We show that unlike previously studied binaries, this is an intrinsic topological insulator with conduction bulk band residing well above the chemical potential. Our data indicates that under good vacuum condition there are no significant aging effects for more then two weeks after cleaving. We also demonstrate that shift of the Kramers point at low temperature is caused by UV assisted absorption of molecular hydrogen. Our findings pave the way for applications of these materials in devices and present an easy scheme to tune their properties.Comment: 4 pages, 4 figure

    On extensions of the Jacobson-Morozov theorem to even characteristic

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    Let G be a simple algebraic group over an algebraically closed field k of characteristic 2. We consider analogues of the Jacobson-Morozov theorem in this setting. More precisely, we classify those nilpotent elements with a simple 3-dimensional Lie overalgebra in g:=Lie(G)\mathfrak{g} := \text{Lie}(G) and also those with overalgebras isomorphic to the algebras Lie(SL2)\text{Lie}(\text{SL}_2) and Lie(PGL2)\text{Lie}(\text{PGL}_2). This leads us to calculate the dimension of Lie automiser ng(kâ‹…e)/cg(e)\mathfrak{n}_\mathfrak{g}(k\cdot e)/\mathfrak{c}_\mathfrak{g}(e) for all nilpotent orbits; in even characteristic this quantity is very sensitive to isogeny.Comment: 22 page

    A note on extremely primitive affine groups

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    Let G be a nite primitive permutation group on a set with nontrivial point stabilizer G . We say that G is extremely primitive if G acts primitively on each of its orbits in n f g. In earlier work, Mann, Praeger and Seress have proved that every extremely primitive group is either almost simple or of a ne type and they have classi ed the a ne groups up to the possibility of at most nitely many exceptions. More recently, the almost simple extremely primitive groups have been completely determined. If one assumes Wall's conjecture on the number of maximal subgroups of almost simple groups, then the results of Mann et al. show that it just remains to eliminate an explicit list of a ne groups in order to complete the classi cation of the extremely primitive groups. Mann et al. have conjectured that none of these a ne candidates are extremely primitive and our main result con rms this conjecture
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