54 research outputs found

    Mass Measurements and the Bound--Electron g Factor

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    The accurate determination of atomic masses and the high-precision measurement of the bound-electron g factor are prerequisites for the determination of the electron mass, which is one of the fundamental constants of nature. In the 2002 CODATA adjustment [P. J. Mohr and B. N. Taylor, Rev. Mod. Phys. 77, 1 (2005)], the values of the electron mass and the electron-proton mass ratio are mainly based on g factor measurements in combination with atomic mass measurements. In this paper, we briefly discuss the prospects for obtaining other fundamental information from bound-electron g factor measurements, we present some details of a recent investigation of two-loop binding corrections to the g factor, and we also investigate the radiative corrections in the limit of highly excited Rydberg S states with a long lifetime, where the g factor might be explored using a double resonance experiment.Comment: 13 pages, LaTeX; dedicated to Prof. H.-J. Kluge on the occasion of his 65th birthday, to appear in Int. J. Mass. Spectrometr

    Radio Wavelength Transients: Current and Emerging Prospects

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    Known classes of radio wavelength transients range from the nearby--stellar flares and radio pulsars--to the distant Universe--\gamma-ray burst afterglows. Hypothesized classes of radio transients include analogs of known objects, e.g., extrasolar planets emitting Jovian-like radio bursts and giant-pulse emitting pulsars in other galaxies, to the exotic, prompt emission from \gamma-ray bursts, evaporating black holes, and transmitters from other civilizations. A number of instruments and facilities are either under construction or in early observational stages and are slated to become available in the next few years. With a combination of wide fields of view and wavelength agility, the detection and study of radio transients will improve immensely.Comment: to appear in proceedings of Hot-wiring the Transient Universe, 2008 March issue of Astronomische Nachrichte

    Techniques in Analytic Lamb Shift Calculations

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    Quantum electrodynamics has been the first theory to emerge from the ideas of regularization and renormalization, and the coupling of the fermions to the virtual excitations of the electromagnetic field. Today, bound-state quantum electrodynamics provides us with accurate theoretical predictions for the transition energies relevant to simple atomic systems, and steady theoretical progress relies on advances in calculational techniques, as well as numerical algorithms. In this brief review, we discuss one particular aspect connected with the recent progress: the evaluation of relativistic corrections to the one-loop bound-state self-energy in a hydrogenlike ion of low nuclear charge number, for excited non-S states, up to the order of alpha (Zalpha)^6 in units of the electron mass. A few details of calculations formerly reported in the literature are discussed, and results for 6F, 7F, 6G and 7G states are given.Comment: 16 pages, LaTe

    Multi-wavelength analysis of high energy electrons in solar flares: a case study of August 20, 2002 flare

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    A multi-wavelength spatial and temporal analysis of solar high energy electrons is conducted using the August 20, 2002 flare of an unusually flat (gamma=1.8) hard X-ray spectrum. The flare is studied using RHESSI, Halpha, radio, TRACE, and MDI observations with advanced methods and techniques never previously applied in the solar flare context. A new method to account for X-ray Compton backscattering in the photosphere (photospheric albedo) has been used to deduce the primary X-ray flare spectra. The mean electron flux distribution has been analysed using both forward fitting and model independent inversion methods of spectral analysis. We show that the contribution of the photospheric albedo to the photon spectrum modifies the calculated mean electron flux distribution, mainly at energies below 100 keV. The positions of the Halpha emission and hard X-ray sources with respect to the current-free extrapolation of the MDI photospheric magnetic field and the characteristics of the radio emission provide evidence of the closed geometry of the magnetic field structure and the flare process in low altitude magnetic loops. In agreement with the predictions of some solar flare models, the hard X-ray sources are located on the external edges of the Halpha emission and show chromospheric plasma heated by the non-thermal electrons. The fast changes of Halpha intensities are located not only inside the hard X-ray sources, as expected if they are the signatures of the chromospheric response to the electron bombardment, but also away from them.Comment: 26 pages, 9 figures, accepted to Solar Physic

    Étude stéréoscopique et spectrographique des sursauts radio solaires de type III

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    Study made using stereo space experiments 1 and 5, which allowed to compare the intensities and the propagation times between 2 different directions (earth and interplanetary probe) and by means of the radio spectrograph of Nançay. The shape of the apparent radiation pattern is obtained for the first time. Study of the dynamic spectrum of groups of type 4 and discovered types N, highlighting the possibility of reflection of the beams on magnetic mirrors. The results are shown to contain important information on the coronal density structure, and a number of extensions are suggested for a more complete understanding of the types III as a heliospheric phenomenon.Étude faites au moyen des expériences spatiales stéréo 1 et 5, qui ont permis de comparer les intensités et les temps de propagation entre 2 directions différentes (terre et sonde interplanétaire) et au moyen du radio spectrographe de Nançay. On obtient pour la première fois la forme du diagramme de rayonnement apparent. Étude du spectre dynamique des groupes de type 4 et découvertes des types N, mettant en évidence la possibilité de réflexion des faisceaux sur miroirs magnétique. On montre que les résultats contiennent une information importante sur la structure de la densité coronale, et on suggère un certain nombre de prolongements en vue d'une appréhension plus complète des types III en tant que phénomène héliosphèrique

    Type III Radio Burst Productivity of Solar Flares

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    We study the statistical relationship between optical flares and type III radio bursts, using modern and extensive computer files. Results emerge along two main lines, concerning the physical mechanism of ejection of energetic particles, and the magnetic field geometry respectively.First, we find that type III probability of occurrence increases strongly with the brightness of a flare and its proximity to a sunspot, and with accompanying prominence activity. This suggests that Bornmann's class I and III events correspond to distinct physical phenomena, particle acceleration and magnetic expansion respectively, both working simultaneously in class II events, which are the most favorable to the ejection of energetic particles out of flaring sites.</jats:p

    Cristal trapézoïdal en spectroscopie X d'implosion par laser

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    Elastically bent, trapezoidal crystals for Bragg diffraction of X-rays allow designing broadband spectrometers with flat field, normal incidence and high resolution. This is applied to study microballoon implosions driven by six laser beams.En courbant élastiquement un cristal trapézoïdal pour la diffraction de Bragg des rayons X, on réalise un spectrographe à champ plan, large bande et haute résolution, sous incidence normale. Grâce à lui, on étudie des implosions de microballons par un laser à six faisceaux

    Whole genome sequencing for mutation discovery in rare neurodevelopmental disorders

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    Recent developments in next generation sequencing (NGS) technologies and their accompanying bioinformatic tools have set the stage for an era of unprecedented progress in research on rare genetic disorders. Here, we develop a whole genome sequencing workflow for the analysis of NGS data and apply it to search for pathogenic mutations in four individuals affected by rare neurodevelopmental disorders. A list of high confidence pathogenic variants was finalized for all individuals. Our developed workflow and findings pave the way for further functional analyses of the brain developmental pathogenesis of the novel mutation(s).Les développements récents dans le séquençage nouvelle génération (NGS) du génome ainsi que les outils de bioinformatique qui les accompagnent font que nous entrons une ère de progrès rapide en recherche sur les désordres génétiques rares. Ici, nous développons un workflow pour l'analyse des données NGS et l'appliquons pour chercher les mutations pathogènes dans quatre individus atteints d'une maladie neurodéveloppementale rare. Une liste de variantes probables pathogènes a été développée pour tout individu. Notre workflow et trouvailles permettent d'avancer notre recherche en analyse fonctionnelle des mécanismes pathogénétiques de la mutation
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