A bstract We calculate the ratios R τ / P ≡ Γ ( → Pν [ γ ]) /Γ μν μ = π , K ) at one loop following a large- N C expansion where Chiral Perturbation Theory is enlarged by including lightest resonances and respecting short-distance behavior dictated QCD. find δR (0 . 18 ± 0 57)% 97 58)%, uncertainties are induced fundamentally counterterms. test lepton universality, obtaining | g 9964 0038 9857 ...

http://dx.doi.org/10.1016/j.sse.2016.07.009 0038-1101/ 2016 Elsevier Ltd. All rights reserved. ⇑ Corresponding author at: Infineon Technologies Austria AG, Siemensstraße 2, A-9500 Villach, Austria. E-mail address: [email protected] (M. Capriotti). M. Capriotti a,⇑, E. Bahat Treidel , C. Fleury , O. Bethge , C. Ostermaier , M. Rigato , S.L.C. Lancaster , F. Brunner , H. Detz , O. Hil...

Using high-resolution optical spectroscopy we determine the chemical abundance of secondary star in binary millisecond pulsar PSR J1023+0038. We measure a metallicity [Fe/H] = 0.48 +/- 0.04 which is higher than Solar value and general find that element abundances are different compared to stars X-ray binaries solar neighbourhood similar Fe content. Our results suggest was formed supernova explo...

http://dx.doi.org/10.1016/j.sse.2014.06.035 0038-1101/ 2014 Elsevier Ltd. All rights reserved. ⇑ Corresponding author. Tel.: +43 15880136060. E-mail addresses: [email protected] (J. Ghosh), [email protected]. at (T. Windbacher), [email protected] (V. Sverdlov), [email protected]. ac.at (S. Selberherr). Joydeep Ghosh ⇑, Thomas Windbacher, Viktor Sverdlov, Siegfried Selber...

*College of Nursing, University of Cincinnati Academic Health Center, Cincinnati, Ohio, †Occupational Medicine Residency Director, College of Medicine, Department of Environmental Health, University of Cincinnati, Cincinnati, Ohio, and ‡Allbright Health Care Center, Cincinnati Health Department, Cincinnati, Ohio Reprint Address: Donna M. Gates, EDD, RN, FAAN, College of Nursing, 3110 Vine Stree...

http://dx.doi.org/10.1016/j.solener.2016.08.050 0038-092X/ 2016 The Authors. Published by Elsevier Ltd. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/). ⇑ Corresponding author. E-mail address: [email protected] (M.C. Paul). W. Li , M.C. Paul a,⇑, N. Sellami , T. Sweet , A. Montecucco , J. Siviter , H. Baig , M. Gao , T. Mal...

http://dx.doi.org/10.1016/j.sse.2016.07.010 0038-1101/ 2016 Elsevier Ltd. All rights reserved. ⇑ Corresponding author. E-mail address: [email protected] (B. Kaczer). 1 Also at KU Leuven, ESAT Department, Leuven, Belgium. B. Kaczer a,⇑, J. Franco , P. Weckx , Ph.J. Roussel , M. Simicic , V. Putcha , E. Bury , M. Cho , R. Degraeve , D. Linten , G. Groeseneken , P. Debacker , B. Parvais , P. Ragh...

http://dx.doi.org/10.1016/j.sse.2014.04.032 0038-1101/ 2014 Elsevier Ltd. All rights reserved. ⇑ Corresponding author at: STMicroelectronics, 850 rue Jean Monnet, F-38926 Crolles Cedex, France. E-mail address: [email protected] (Y. Solaro). Yohann Solaro a,b,c,⇑, Jing Wan , Pascal Fonteneau , Claire Fenouillet-Beranger , Cyrille Le Royer , Alexander Zaslavsky , Philippe Ferrari , Sorin Cris...

The transitional millisecond pulsar PSR J1023+0038 is the first discovered to emit UV and optical pulses. Here we present results of X-ray phase-resolved timing analysis observations performed with Hubble Space Telescope, XMM-Newton, NuSTAR satellites between 2014 2021. Ultraviolet pulsations are detected in high luminosity mode disappear during low flaring modes, similar what observed band. In...