Abstract: | Cross sections for e + p charged current deep inelastic scattering at a centre-of-mass energy of have been determined with an integrated luminosity of collected with the ZEUS detector at HERA. The differential cross sections , and for are presented. In addition, has been measured in the kinematic range and . The predictions of the Standard Model agree well with the measured cross sections. The mass of the W boson propagator is determined to be from a fit to . The chiral structure of the Standard Model is also investigated in terms of the (1-y)2 dependence of the double-differential cross section. The structure-function has been extracted by combining the measurements presented here with previous ZEUS results from e - p scattering, extending the measurement obtained in a neutrino-nucleus scattering experiment to a significantly higher Q 2 region.Received: 17 July 2003, Published online: 12 November 2003 a supported by the Natural Sciences and Engineering Research Council of Canada (NSERC) b supported by the German Federal Ministry for Education and Research (BMBF), under contract numbers HZ1GUA 2, HZ1GUB 0, HZ1PDA 5, HZ1VFA 5 c supported by the MINERVA Gesellschaft für Forschung GmbH, the Israel Science Foundation, the U.S.-Israel Binational Science Foundation and the Benozyio Center for High Energy Physics d supported by the German-Israeli Foundation and the Israel Science Foundation e supported by the Italian National Institute for Nuclear Physics (INFN) f supported by the Japanese Ministry of Education, Culture, Sports, Science and Technology (MEXT) and its grants for Scientific Research g supported by the Korean Ministry of Education and Korea Science and Engineering Foundation h supported by the Netherlands Foundation for Research on Matter (FOM) i supported by the Polish State Committee for Scientific Research, grant no. 620/E-77/SPUB-M/DESY/P-03/DZ 247/2000-2002 j partially supported by the German Federal Ministry for Education and Research (BMBF) k supported by the Fund for Fundamental Research of Russian Ministry for Science and Education and by the German Federal Ministry for Education and Research (BMBF) l supported by the Spanish Ministry of Education and Science through funds provided by CICYT m supported by the Particle Physics and Astronomy Research Council, UK n supported by the US Department of Energy o supported by the US National Science Foundation p supported by the Polish State Committee for Scientific Research, grant no. 112/E-356/SPUB-M/DESY/P-03/DZ 301/2000-2002, 2 P03B 13922 q supported by the Polish State Committee for Scientific Research, grant no. 115/E-343/SPUB-M/DESY/P-03/DZ 121/2001-2002, 2 P03B 07022 |