28,681 research outputs found

    A magnetically driven origin for the low luminosity GRB 170817A associated with GW170817

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    The gamma-ray burst GRB 170817A associated with GW170817 is subluminous and subenergetic compared with other typical short GRBs. It may be due to a relativistic jet viewed off-axis, or a structured jet, or cocoon emission. Giant flares from magnetars may possibly be ruled out. However, the luminosity and energetics of GRB 170817A is coincident with that of magnetar giant flares. After the coalescence of the binary neutron star, a hypermassive neutron star may be formed. The hypermassive neutron star may have magnetar-strength magnetic field. During the collapse of the hypermassive neutron star, the magnetic field energy will also be released. This giant-flare-like event may explain the the luminosity and energetics of GRB 170817A. Bursts with similar luminosity and energetics are expected in future neutron star-neutron star or neutron star-black hole mergers.Comment: 6 pages, 1 figure, accepted in Research in Astronomy and Astrophysic

    Cosmic age, Statefinder and OmOm diagnostics in the decaying vacuum cosmology

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    As an extension of Λ\LambdaCDM, the decaying vacuum model (DV) describes the dark energy as a varying vacuum whose energy density decays linearly with the Hubble parameter in the late-times, ρΛ(t)H(t)\rho_\Lambda(t) \propto H(t), and produces the matter component. We examine the high-zz cosmic age problem in the DV model, and compare it with Λ\LambdaCDM and the Yang-Mills condensate (YMC) dark energy model. Without employing a dynamical scalar field for dark energy, these three models share a similar behavior of late-time evolution. It is found that the DV model, like YMC, can accommodate the high-zz quasar APM 08279+5255, thus greatly alleviates the high-zz cosmic age problem. We also calculate the Statefinder (r,s)(r,s) and the {\it Om} diagnostics in the model. It is found that the evolutionary trajectories of r(z)r(z) and s(z)s(z) in the DV model are similar to those in the kinessence model, but are distinguished from those in Λ\LambdaCDM and YMC. The Om(z){\it Om}(z) in DV has a negative slope and its height depends on the matter fraction, while YMC has a rather flat Om(z){\it Om}(z), whose magnitude depends sensitively on the coupling.Comment: 12 pages, 4 figures, with some correction

    Primitive permutation groups and derangements of prime power order

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    Let GG be a transitive permutation group on a finite set of size at least 22. By a well known theorem of Fein, Kantor and Schacher, GG contains a derangement of prime power order. In this paper, we study the finite primitive permutation groups with the extremal property that the order of every derangement is an rr-power, for some fixed prime rr. First we show that these groups are either almost simple or affine, and we determine all the almost simple groups with this property. We also prove that an affine group GG has this property if and only if every two-point stabilizer is an rr-group. Here the structure of GG has been extensively studied in work of Guralnick and Wiegand on the multiplicative structure of Galois field extensions, and in later work of Fleischmann, Lempken and Tiep on rr'-semiregular pairs.Comment: 30 pages; to appear in Manuscripta Mat

    Derangements in primitive permutation groups, with an application to character theory

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    Let GG be a finite primitive permutation group and let κ(G)\kappa(G) be the number of conjugacy classes of derangements in GG. By a classical theorem of Jordan, κ(G)1\kappa(G) \geqslant 1. In this paper we classify the groups GG with κ(G)=1\kappa(G)=1, and we use this to obtain new results on the structure of finite groups with an irreducible complex character that vanishes on a unique conjugacy class. We also obtain detailed structural information on the groups with κ(G)=2\kappa(G)=2, including a complete classification for almost simple groups.Comment: 29 page

    Combined nutritional stress and a new systemic pesticide (flupyradifurone, Sivanto®) reduce bee survival, food consumption, flight success, and thermoregulation.

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    Flupyradifurone (FPF, Sivanto®) is a new butenolide insecticide that, like the neonicotinoids, is a systemic nicotinic acetylcholine receptor (nAChR) agonist. However, FPF is considered bee-safe (according to standard Risk Assessment tests), and is thus a potential solution to the adverse effects of other pesticides on beneficial insects. To date, no studies have examined the impact of nutritional stress (decreased food diversity and quality) and FPF exposure on bee health although both stressors can occur, especially around agricultural monocultures. We therefore tested the effects of a field-realistic FPF concentration (4 ppm, FPFdaily dose = 241 ± 4 ng/bee/day, 1/12 of LD50) and nutritional stress (nectar with low-sugar concentrations) on honey bee (Apis mellifera L.) mortality, food consumption, thermoregulation, flight success (unsuccessful vs. successful), and flight ability (duration, distance, velocity). Flight and thermoregulation are critical to colony health: bees fly to collect food and reproduce, and they thermoregulate to increase flight efficiency and to rear brood. We studied the effects across seasons because seasonality can influence bee sensitivity to environmental stress. We demonstrate that, depending upon season and nutritional stress, FPF can reduce bee survival (-14%), food consumption (-14%), thermoregulation (-4%, i.e. hypothermia), flight success (-19%), and increase flight velocity (+13%). Because pesticide exposure and nutritional stress can co-occur, we suggest that future studies and pesticide risk assessments consider both seasonality and nutritional stress when evaluating pesticide safety for bees

    Statistical tests for Lyapunov exponents of deterministic systems.

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    In order to develop statistical tests for the Lyapunov exponents of deterministic dynamical systems, we develop bootstrap tests based on empirical likelihood for percentiles and expectiles of strictly stationary processes. The percentiles and expectiles are estimated in terms of asymmetric least deviations and asymmetric least squares methods. Asymptotic distributional properties of the estimators are established.
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