Published March 1995 | Version v1
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Nodal trajectories and kaon photoproduction

  • 1. CEA Centre d'Etudes de Saclay, 91 - Gif-sur-Yvette (France). Dept. d'Astrophysique, de la Physique des Particules, de la Physique Nucleaire et de l'Instrumentation Associee
  • 2. Pittsburgh Univ., PA (United States). Dept. of Physics and Astronomy

Description

Using helicity amplitudes, the general structure of the full set of 15 single and double polarization spin observables for the reaction γp → K+Λ has been discussed earlier. Through this model independent approach, general rules on the angular structure of the observables have been derived. The observables in each class have similar 'nodal structure' possibilities, e.g. their values at 0 deg and 180 deg and their possible intervening nodes are of related nature. One of those rules is confronted with three recent dynamical models for the L1a class observables. (K.A.). 5 refs., 1 fig

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Additional details

Publishing Information

Imprint Pagination
4 p.
Report number
CEA-DAPNIA-SPhN--95-12

Conference

Title
15. European conference on few-body problems in physics.
Dates
5-9 Jun 1995.
Place
Peniscola (Spain).