Determination of the strange quark content of the nucleon from a next-to-leading-order QCD analysis of neutrino charm production

We present the first next-to-leading-order QCD analysis of neutrino charm production, using a sample of 6090 ^– and -induced opposite-sign dimuon events observed in the CCFR detector at the Fermilab Tevatron. We find that the nucleon strange quark content is suppressed with respect to the non-strange sea quarks by a factor =0.477 _–0.053 ^+0.063 , where the error includes statistical, systematic and QCD scale uncertainties. In contrast to previous leading order analyses, we find that the strange seax-dependence is similar to that of the non-strange sea, and that the measured charm quark mass,m _c =1.70±0.19 GeV/c², is larger and consistent with that determined in other processes. Further analysis finds that the difference inx-distributions betweenxs(x) and is small. A measurement of the Cabibbo-Kobayashi-Maskawa matrix element |V _cd |=0.232 _–0.020 ^+0.018 is also presented.     

FLASH PHOTOLYSIS-ELECTRON SPIN RESONANCE STUDIES OF THE INTERACTION OF PHENAZINE METHOSULFATE WITH REACTION-CENTER PREPARATIONS FROM THE R-26 MUTANT OF RHODOPSEUDOMONAS SPHEROIDES*

Abstract— Using the technique of flash photolysis-electron spin resonance, we have shown, by means of a kinetic analysis, that phenazine methosulfate (PMS) interacts with reaction-center preparations from the blue-green mutant R26 of Rhodopseudomonas spheroides. At intermediate concentrations of PMS, biphasic decay kinetics of the P870⁺ ESR signal are observed demonstrating that the PMS radical interacts with reaction centers by a specific binding mechanism. With PMS bound to reaction centers, the P870⁺ ESR signal decays in ˜ 1 ms; whereas, in unbound reaction centers the decay is ˜ 120 ms. A model is proposed involving the interaction of PMS on the donor side of P870.     

Thermal physics in carbon nanotube growth kinetics

The growth of single wall carbon nanotubes (SWNTs) mediated by metal nanoparticles is considered within (i) the surface diffusion growth kinetics model coupled with (ii) a thermal model taking into account heat release of carbon adsorption-desorption on nanotube surface and carbon incorporation into the nanotube wall and (iii) carbon nanotube-inert gas collisional heat exchange. Numerical simulations performed together with analytical estimates reveal various temperature regimes occurring during SWNT growth. During the initial stage, which is characterized by SWNT lengths that are shorter than the surface diffusion length of carbon atoms adsorbed on the SWNT wall, the SWNT temperature remains constant and is significantly higher than that of the ambient gas. After this stage the SWNT temperature decreases towards that of gas and becomes nonuniformly distributed over the length of the SWNT. The rate of SWNT cooling depends on the SWNT-gas collisional energy transfer that, from molecular dynamics simulations, is seen to be efficient only in the SWNT radial direction. The decreasing SWNT temperature may lead to solidification of the catalytic metal nanoparticle terminating SWNT growth or triggering nucleation of a new carbon layer and growth of multiwall carbon nanotubes.