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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...
Autores principales: | , , |
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Lenguaje: | eng |
Publicado: |
1972
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/0550-3213(72)90131-9 http://cds.cern.ch/record/875666 |
_version_ | 1780907863889149952 |
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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). |
id | cern-875666 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1972 |
record_format | invenio |
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 AT geerk onthenatureofabsorption AT halzenf onthenatureofabsorption |