Skip to main content Accessibility help
×
Hostname: page-component-77c89778f8-swr86 Total loading time: 0 Render date: 2024-07-22T18:22:29.909Z Has data issue: false hasContentIssue false

14 - Factorization and evolution in high-energy scattering

Published online by Cambridge University Press:  05 August 2012

George Sterman
Affiliation:
State University of New York, Stony Brook
Get access

Summary

Most zero-mass and high-energy cross sections are not directly calculable in perturbation theory, because of the presence of large logarithms of energy over mass (see the comments at the end of Chapter 13). Nevertheless, events with large momentum transfer are the result of violent short-distance collisions, which one can isolate quantitatively. The separation of calculable short-distance from incalculable long-distance effects is known as factorization. Deeply inelastic scattering cross sections illustrate this property. They may be used, in turn, to compute a wide class of other inclusive and semi-inclusive cross sections with large momentum transfers. The evolution in momentum transfer of deeply inelastic and related cross sections may also be determined by methods related to both the renormalization group and the parton model. The operator product expansion gives an alternate interpretation, which generalizes factorization beyond leading power behavior, at least in deeply inelastic scattering.

The examples of this chapter, in which the above results are derived and discussed, are drawn primarily from QCD, but the techniques of factorization and the operator product expansion are generally applicable in field theory. They transcend low-order calculations, by systematically organizing contributions from arbitrary orders of the perturbative expansion.

Deeply inelastic scattering

As an introduction, and to facilitate calculation, we first discuss tensor analysis and kinematics for the leptoproduction amplitude (Roy r1975, Close r1979), in which a lepton scatters from a hadron of momentum pμ to produce an arbitrary hadronic state with momentum pn.

Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 1993

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×