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Gravitational interactions of integrable models
that integrability properties of symmetric space models still hold for the matter sector. Using similar arguments for the fermionic counterpart, namely Gross--Neveu-type models, we verify that such conclusions must also hold for them, as recently suggested.
Autores principales: | , |
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Lenguaje: | eng |
Publicado: |
1995
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/0370-2693(95)01301-6 http://cds.cern.ch/record/285624 |
_version_ | 1780888252404727808 |
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author | Abdalla, E. Abdalla, M.C.B. |
author_facet | Abdalla, E. Abdalla, M.C.B. |
author_sort | Abdalla, E. |
collection | CERN |
description | that integrability properties of symmetric space models still hold for the matter sector. Using similar arguments for the fermionic counterpart, namely Gross--Neveu-type models, we verify that such conclusions must also hold for them, as recently suggested. |
id | cern-285624 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1995 |
record_format | invenio |
spelling | cern-2856242023-03-14T16:35:08Zdoi:10.1016/0370-2693(95)01301-6http://cds.cern.ch/record/285624engAbdalla, E.Abdalla, M.C.B.Gravitational interactions of integrable modelsParticle Physics - Theorythat integrability properties of symmetric space models still hold for the matter sector. Using similar arguments for the fermionic counterpart, namely Gross--Neveu-type models, we verify that such conclusions must also hold for them, as recently suggested.We couple non-linear σ-models to Liouville gravity, showing that integrability properties of symmetric space models still hold for the matter sector. Using similar arguments for the fermionic counterpart, namely Gross-Neveu-type models, we verify that such conclusions must also hold for them, as recently suggested.We couple non-linear $\sigma$-models to Liouville gravity, showing that integrability properties of symmetric space models still hold for the matter sector. Using similar arguments for the fermionic counterpart, namely Gross--Neveu-type models, we verify that such conclusions must also hold for them, as recently suggested.hep-th/9507171CERN-TH-95-209IC-95-201CERN-TH-95-209IC-95-201oai:cds.cern.ch:2856241995-07-31 |
spellingShingle | Particle Physics - Theory Abdalla, E. Abdalla, M.C.B. Gravitational interactions of integrable models |
title | Gravitational interactions of integrable models |
title_full | Gravitational interactions of integrable models |
title_fullStr | Gravitational interactions of integrable models |
title_full_unstemmed | Gravitational interactions of integrable models |
title_short | Gravitational interactions of integrable models |
title_sort | gravitational interactions of integrable models |
topic | Particle Physics - Theory |
url | https://dx.doi.org/10.1016/0370-2693(95)01301-6 http://cds.cern.ch/record/285624 |
work_keys_str_mv | AT abdallae gravitationalinteractionsofintegrablemodels AT abdallamcb gravitationalinteractionsofintegrablemodels |