English

CLASSICAL PHOTOABSORPTION SUM RULES

High Energy Physics - Phenomenology 2016-09-01 v1

Abstract

We use a quantum loop expansion to derive sum rule constraints on polarized photoabsorption cross sections in the Standard Model, generalizing earlier results obtained by Altarelli, Cabibbo, and Maiani. We show that the logarithmic integral of the spin-dependent photoabsorption cross section νthdννΔσBorn(ν)\int^\infty_{\nu_{th}} {d\nu\over \nu} \Delta \sigma_{\rm Born}(\nu) vanishes for any 222 \to 2 Standard Model or supersymmetric process γabc\gamma a \to b c in the classical, tree-graph approximation. Here ν=pq/M\nu = {p \cdot q}/M and Δσ(ν)=σP(ν)σA(ν)\Delta \sigma(\nu) = \sigma_P(\nu)- \sigma_A(\nu) is the difference between the photoabsorption cross section for parallel and antiparallel photon and target helicities. Tests of the sum rule for the reactions γeWν\gamma e \to W \nu and γγW+W\gamma \gamma \to W^+ W^- can provide new tests of the canonical magnetic and quadrupole couplings of the Standard Model. We also extend the sum rule to certain virtual photon processes.

Keywords

Cite

@article{arxiv.hep-ph/9502416,
  title  = {CLASSICAL PHOTOABSORPTION SUM RULES},
  author = {Stanley J. Brodsky and Ivan Schmidt},
  journal= {arXiv preprint arXiv:hep-ph/9502416},
  year   = {2016}
}

Comments

11 pages, 1 figure. For hard copy, e-mail request for SLAC-PUB-95-6761 to [email protected]