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Now showing items 145 - 160 of 22467

  • On being a\r g\r ood\r Bayesian

    Buck, Caitlin E.   Meson, Bo  

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  • G ROUP I DENTITY AND L EADING - BY -E XAMPLE

    Michalis Drouvelis   Daniele Nosenzo  

    We study the interplay between leading-by-example and group identity in a public goods game experiment. A common identity between the leader and her followers is beneficial for cooperation: average contributions are more than 30% higher than in a treatment where no identity was induced. In two further treatments we study the effects of heterogeneous identities. We find no effect on cooperation when only part of the followers share the leader's identity, or when followers share a common identity that differs from that of the leader. We conclude that group identity is an effective but fragile instrument to promote cooperation.
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  • DOUBLE-STRANDED POLYC:POLY(G/I) RNA FOR IMMUNOSTIMULATION AND CANCER TREATMENT

    The present invention relates to polyC:poly(G/l) dsRNAs for triggering innate immunity, in particular through toll-like receptor 3 (TLR-3) and, optionally, RIG-I or RIG-I— like receptors (RLRs), as well as compositions and medicaments containing such dsRNAs, methods for their production and their use in medicine, especially immunostimulation and prevention and/or therapy of infections and tumor diseases.
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  • M/G/1 Queue with Exponential Working Vacation and Gated Service

    Zsolt Saffer   Miklós Telek  

    In this paper we consider the analysis of an M/G/1 queue with working vacation. In contrast to the previous literature where the working vacation starts when all customers are served (exhaustive discipline) we consider the case where the vacation period starts when the customers present at the system at beginning of the service period are served (gated discipline). The analysis of the model with gated discipline requires a different approach than the one with exhaustive discipline.
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  • Double-stranded polyC:poly(G/I) RNA for immunostimulation and cancer treatment

    The present invention relates to polyC:poly(G/I) dsRNAs for triggering innate immunity, in particular through toll-like receptor 3 (TLR-3) and, optionally, RIG-I or RIG-I-like receptors (RLRs), as well as compositions and medicaments containing such dsRNAs, methods for their production and their use in medicine, especially immunostimulation and prevention and/or therapy of infections and tumor diseases.
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  • Morse theory for the space of Higgs G–bundles

    Indranil Biswas and Graeme Wilkin  

    Fix a C ∞ principal G–bundle E0G{E^0_G} on a compact connected Riemann surface X, where G is a connected complex reductive linear algebraic group. We consider the gradient flow of the Yang–Mills–Higgs functional on the cotangent bundle of the space of all smooth connections on E0G{E^0_G}. We prove that this flow preserves the subset of Higgs G–bundles, and, furthermore, the flow emanating from any point of this subset has a limit. Given a Higgs G–bundle, we identify the limit point of the integral curve passing through it. These generalize the results of the second named author on Higgs vector bundles.
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  • Interacting New Agegraphic Viscous Dark Energy with Varying G

    A. Sheykhi and M. R. Setare  

    We consider the new agegraphic model of dark energy with a varying gravitational constant, G, in a non-flat universe. We obtain the equation of state and the deceleration parameters for both interacting and noninteracting new agegraphic dark energy. We also present the equation of motion determining the evolution behavior of the dark energy density with a time variable gravitational constant. Finally, we generalize our study to the case of viscous new agegraphic dark energy in the presence of an interaction term between both dark components.
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  • [Nr 105] Atlas genomu raka (TCGA) w nowotworach g?owy i szyi

    Szybiak, Bartosz   Golusiński, Pawe?   Wiznerowicz, Maciej   Suchorska, Wiktoria   Golusiński, Wojciech  

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  • Stochastic Motion of Test Particle Implies That G Varies with Time

    Davood Momeni  

    The aim of this letter is to propose a new description to the time varying gravitational constant problem, which naturally implements the Dirac’s large numbers hypothesis in a new proposed holographic scenario for the origin of gravity as an entropic force. We survey the effect of the Stochastic motion of the test particle in Verlinde’s scenario for gravity (Verlinde in arXiv:1001.0785, 2010). Firstly we show that we must get the equipartition values for t→∞ which leads to the usual Newtonian gravitational constant. Secondly, the stochastic (Brownian) essence of the motion of the test particle, modifies the Newton’s 2nd law. The direct result is that the Newtonian constant has been time dependence in resemblance as Setare and Momeni (arXiv:1004.0589, 2010).
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  • Compatibility with Derived G-Invariance

    36. Compatibility with Derived G-Invariance
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  • Nordiskt I?karem?te i G?teborg

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  • G?z ??i Lensi Yüzeyinde Fakik Paternde Ps?doeksfoliyasyon Materyal Birikimi

    Güler, Emre   Tenlik, Aylin   Kara Akyüz, Tuba   Erdurmu?, Mesut   Hep?en, ?brahim Feyzi  

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  • Variable G Corrections to Statefinder Parameters of Dark Energy

    Mubasher Jamil  

    Motivated by several observational and theoretical developments concerning the variability of Newton’s gravitational constant with time G(t), we calculate the varying G correction to the statefinder parameters for four models of dark energy namely interacting dark energy holographic dark energy, new-agegraphic dark energy and generalized Chaplygin gas.
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  • Cusp form motives and admissible\r G\r -covers

    Petersen   Dan  

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  • Do?an G??men,\r The Adam Smith Problem

    Cockshott   Paul  

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  • Bulk viscous LRS Bianchi-I Universe with variable G and decaying I >

    Yadav, Anil Kumar   Pradhan, Anirudh   Singh, Ajay Kumar  

    The present study deals with spatially homogeneous and totally anisotropic locally rotationally symmetric (LRS) Bianchi type I cosmological model with variable G and I > in presence of imperfect fluid. To get the deterministic model of Universe, we assume that the expansion (theta) in the model is proportional to shear (sigma). This condition leads to A=a""B (n) , where A, B are metric potential. The cosmological constant I > is found to be decreasing function of time and it approaches a small positive value at late time which is supported by recent Supernovae Ia (SN Ia) observations. Also it is evident that the distance modulus curve of derived model matches with observations perfectly.
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