615 research outputs found

    Radiative μ\mu and τ\tau leptonic decays at NLO

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    We present the differential rates and branching ratios of the radiative decays τlνˉνγ\tau \to l \bar{\nu} \nu \gamma, with l=el=e or μ\mu, and μeνˉνγ\mu \to e \bar{\nu} \nu \gamma in the Standard Model at next-to-leading order. Radiative corrections are computed taking into account the full depencence on the mass mlm_l of the final charged leptons, which is necessary for the correct determination of the branching ratios. Only partial agreement is found with previous calculations performed in the ml0m_l \to 0 limit. Our results agree with the measurements of the branching ratios B(μeνˉνγ)\mathcal{B} (\mu \to e \bar{\nu} \nu \gamma) and B(τμνˉνγ)\mathcal{B} (\tau \to \mu \bar{\nu} \nu \gamma) for a minimum photon energy of 10 MeV in the μ\mu and τ\tau rest frames, respectively. Babar's recent precise measurement of the branching ratio B(τeνˉνγ)\mathcal{B} (\tau \to e \bar{\nu} \nu \gamma), for the same photon energy threshold, differs from our prediction by 3.5 standard deviations.Comment: 13 pages, 1 figure, results included as ancillary file

    W-propagator corrections to muon and tau leptonic decays

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    We derive the corrections induced by the W-boson propagator to the differential rates of the leptonic decay of a polarized muon and tau lepton. Results are presented both for decays inclusive of inner bremsstrahlung as well as for radiative ones, when a photon emitted in the decay process is measured. The numerical effect of these corrections is discussed. The definition of the Fermi constant is briefly reviewed.Comment: 5 pages, no figures, accepted for publicatio

    L'expansion coloniale de la fourmi d'Argentine

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    La fourmi Linepithema humile fait preuve d'une exceptionnelle aptitude à coloniser de très larges territoires. Cette expansion est favorisée par une organisation sociale bien différente de celle qu'elle adopte dans son pays d'origine. Quelle est la clé de ce changement

    Evolution of miniaturisation in inquiline parasitic ants: Timing of male elimination in Plagiolepis pygmaea, the host of Plagiolepis xene

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    Inquiline ant species are workerless social parasites whose queens rely completely on the host worker force to raise their brood. A remarkable feature of inquiline ants is the small size of sexuals, which are of the same size as or smaller than host workers. It has been suggested that miniaturisation evolved by parasites to prevent host workers from discriminating between their own worker brood and the inquiline sexuals, so that male and female inquilines can develop under conditions where the host species does not produce its own sexuals. In line with the miniaturisation hypothesis, workers of the ant P. pygmaea cull all the male brood of their own species, whereas at the same time males of their inquiline parasite P. xene are reared to adulthood. Here, we tested whether P. pygmaea workers recognize and eliminate males of their own species when they reach the size of the larger workers. Contrary to the assumption that size is indeed the primary cue used by workers to discriminate male from worker brood, we found that males of P. pygmaea are culled between the small and medium larval stages, that is much before reaching the critical size of the largest worker larvae. Based on this finding, we propose an extension of the miniaturisation hypothesis with a first step whereby the parasitic P. xene males escape the caste and sex recognition system of the host during early development. The most likely mechanism is chemical mimicry of host worker larvae. Miniaturisation would have evolved later to prevent the host workers to secondarily use size as a recognition cue to eliminate P. xene males

    Precise mass-dependent QED contributions to leptonic g-2 at order alpha^2 and alpha^3

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    Improved values for the two- and three-loop mass-dependent QED contributions to the anomalous magnetic moments of the electron, muon, and tau lepton are presented. The Standard Model prediction for the electron (g-2) is compared with its most precise recent measurement, providing a value of the fine-structure constant in agreement with a recently published determination. For the tau lepton, differences with previously published results are found and discussed. An updated value of the fine-structure constant is presented in "Note added after publication."Comment: 6 pages, 1 figure. v2: New determination of alpha presented (based on the recent electron g-2 measurement). v3: New formulae added in Sec.IIB. v4: Updated value of alpha presente

    SUSY-GUTs, SUSY-Seesaw and the Neutralino Dark Matter

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    We will consider a SUSY-SU(5) with one right-handed neutrino with a large top like Yukawa coupling. Assuming universal soft masses at high scale we compute the low-energy spectrum and subsequently the neutralino LSP relic density taking also into consideration SU(5) as well as the see-saw running effects above the gauge coupling unification scale. We found that there exists no viable region in parameter space for \tan\beta \ler ~35. The τ~\tilde{\tau} coannihilation process starts becoming efficient for \tan\beta \ger 35-40. However, this process is significantly constrained by the limited range in which the stau is lighter than the neutralino. In fact, for a given tanβ\tan\beta we find that there exists an upper bound on the lightest neutralino mass (Mχ10M_{\chi_1^0}) in this region. The A-pole funnel region appears at very large tanβ4550\tan\beta \simeq 45-50, while the focus-point region does not make an appearance till large (m0,M1/2m_0,M_{1/2}), namely a few TeV. Large A0A_0 terms at high scale can lead to extended regions consistent with WMAP constraints and remove the upper bounds in the stau coannihilation regions.Comment: 18 pages, 7 figures; references added, figure added, improved discussions in text, to appear in JHE

    Some model-independent phenomenological consequences of flexible brane worlds

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    In this work we will review the main properties of brane-world models with low tension. Starting from very general principles, it is possible to obtain an effective action for the relevant degrees of freedom at low energies (branons). Using the cross sections for high-energy processes involving branons, we set bounds on the different parameters appearing in these models. We also show that branons provide a WIMP candidate for dark matter in a natural way. We consider cosmological constraints on its thermal and non-thermal relic abundances. We derive direct detection limits and compare those limits with the preferred parameter region in the case in which the EGRET excess in the diffuse galactic gamma rays is due to dark matter annihilation. Finally we will discuss the constraints coming from the precision tests of the Standard Model and the muon anomalous magnetic moment.Comment: 10 pages, 6 figures. Contribution to the Proceedings of the Second International Conference on Quantum Theories and Renormalization Group in Gravity and Cosmology, IRGAC 2006, Barcelona, 11-15 July, 200
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