Abstract
The use of the structure functions formalism to describe the electromagnetic radiative corrections in e+e- colliders is described. Examples are given of specific applications to physical quantities. The total cross section with both initial and final state radiative corrections is derived, pt dependent structure functions are introduced and applied to the radiative neutrino counting problem. Expressions are derived for the forward-backward asymmetry A FB. The problem of the next-to-leading factorization and of the use of structure functions to construct a Monte Carlo type algorithm is also briefly sketched
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
