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On the nature of absorption

The imaginary helicity non-flip omega exchange amplitudes in KN and NN scattering are determined versus t and s from data on elastic differential cross section differences. The omega -universality prediction Im omega /sub N/(t)= 3 Im omega /sub K/(t), is found to be satisfied for 0<or= mod t mod...

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Detalles Bibliográficos
Autores principales: Barger, V, Geer, K, Halzen, F
Lenguaje:eng
Publicado: 1972
Materias:
Acceso en línea:https://dx.doi.org/10.1016/0550-3213(72)90131-9
http://cds.cern.ch/record/875666
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author Barger, V
Geer, K
Halzen, F
author_facet Barger, V
Geer, K
Halzen, F
author_sort Barger, V
collection CERN
description The imaginary helicity non-flip omega exchange amplitudes in KN and NN scattering are determined versus t and s from data on elastic differential cross section differences. The omega -universality prediction Im omega /sub N/(t)= 3 Im omega /sub K/(t), is found to be satisfied for 0<or= mod t mod <or=0.5, indicating that the absorptive cuts as small t preserve universality. The impact parameter distributions of the omega amplitudes show: (i) a peripheral peak centred around b approximately=1 fm, with Delta b approximately =+or-0.5 fm in KN and Delta b approximately=+or-0.75 fm in NN; (ii) a sizeable negative contribution at small b, more negative in NN than in KN, (iii) a smaller tail of negative contributions around b approximately=2 fm. Strong absorption of the omega -pole imaginary amplitude with lambda values around two is needed to reproduced this structure. A new version of the absorption model suggested by pi N amplitude analysis, is confirmed by the results. (20 refs).
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1972
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spelling cern-8756662019-09-30T06:29:59Zdoi:10.1016/0550-3213(72)90131-9http://cds.cern.ch/record/875666engBarger, VGeer, KHalzen, FOn the nature of absorptionParticle Physics - PhenomenologyThe imaginary helicity non-flip omega exchange amplitudes in KN and NN scattering are determined versus t and s from data on elastic differential cross section differences. The omega -universality prediction Im omega /sub N/(t)= 3 Im omega /sub K/(t), is found to be satisfied for 0<or= mod t mod <or=0.5, indicating that the absorptive cuts as small t preserve universality. The impact parameter distributions of the omega amplitudes show: (i) a peripheral peak centred around b approximately=1 fm, with Delta b approximately =+or-0.5 fm in KN and Delta b approximately=+or-0.75 fm in NN; (ii) a sizeable negative contribution at small b, more negative in NN than in KN, (iii) a smaller tail of negative contributions around b approximately=2 fm. Strong absorption of the omega -pole imaginary amplitude with lambda values around two is needed to reproduced this structure. A new version of the absorption model suggested by pi N amplitude analysis, is confirmed by the results. (20 refs).CERN-TH-1471oai:cds.cern.ch:8756661972
spellingShingle Particle Physics - Phenomenology
Barger, V
Geer, K
Halzen, F
On the nature of absorption
title On the nature of absorption
title_full On the nature of absorption
title_fullStr On the nature of absorption
title_full_unstemmed On the nature of absorption
title_short On the nature of absorption
title_sort on the nature of absorption
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/0550-3213(72)90131-9
http://cds.cern.ch/record/875666
work_keys_str_mv AT bargerv onthenatureofabsorption
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AT halzenf onthenatureofabsorption