Scalar radius of the pion and γγ → ππ

We make an improvement of the dispersion relation calculation of the quadratic scalar radius of the pion, 〈r2〉s pπ, and the reaction γγ → π0 π0. We solve a previous discrepancy between the the solution of the Muskhelishvili-Omnès equations for the non-strange null isospin (I) pion scalar form factor...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Roca, L., Oller, J.A., Schat, C.
Formato: CONF
Materias:
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_18248039_v_n_p_Roca
Aporte de:
id todo:paper_18248039_v_n_p_Roca
record_format dspace
spelling todo:paper_18248039_v_n_p_Roca2023-10-03T16:33:10Z Scalar radius of the pion and γγ → ππ Roca, L. Oller, J.A. Schat, C. Dispersion relations Form factors Isospin Lower energies Approximation theory Dispersions Shear waves Stress intensity factors Hadrons We make an improvement of the dispersion relation calculation of the quadratic scalar radius of the pion, 〈r2〉s pπ, and the reaction γγ → π0 π0. We solve a previous discrepancy between the the solution of the Muskhelishvili-Omnès equations for the non-strange null isospin (I) pion scalar form factor and the Indurain's calculation using an Omnès representation of this form factor. We show that Ynduráin's method is indeed compatible with the determinations from the Muskhelishvili-Omnès equations once a possible zero in the scalar form factor is considered. Once this is accounted for, the resulting value is 〈r2〉 s pπ = 0.63 ±0.05 fm2. Regarding the reaction γγ → π0 π0 we emphasize how the f0(980) signal emerges in γγ → ππ within the dispersive approach and how this fixes to a large extent the phase of the isoscalar S-wave γγ → ππ amplitude above the KK̄ threshold. This allows us to make sharper predictions for the cross section at lower energies and our results could then be used to distinguish between different ππ isoscalar S-wave parameterizations with the advent of new precise data on γγ → π0π0. We also pay special attention to the role played by the σ resonance in γγ → ππ and calculate its coupling and width to γγ, for which we obtain Λ(σ → γγ) = ( 1.68 ± 0.15) KeV. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_18248039_v_n_p_Roca
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Dispersion relations
Form factors
Isospin
Lower energies
Approximation theory
Dispersions
Shear waves
Stress intensity factors
Hadrons
spellingShingle Dispersion relations
Form factors
Isospin
Lower energies
Approximation theory
Dispersions
Shear waves
Stress intensity factors
Hadrons
Roca, L.
Oller, J.A.
Schat, C.
Scalar radius of the pion and γγ → ππ
topic_facet Dispersion relations
Form factors
Isospin
Lower energies
Approximation theory
Dispersions
Shear waves
Stress intensity factors
Hadrons
description We make an improvement of the dispersion relation calculation of the quadratic scalar radius of the pion, 〈r2〉s pπ, and the reaction γγ → π0 π0. We solve a previous discrepancy between the the solution of the Muskhelishvili-Omnès equations for the non-strange null isospin (I) pion scalar form factor and the Indurain's calculation using an Omnès representation of this form factor. We show that Ynduráin's method is indeed compatible with the determinations from the Muskhelishvili-Omnès equations once a possible zero in the scalar form factor is considered. Once this is accounted for, the resulting value is 〈r2〉 s pπ = 0.63 ±0.05 fm2. Regarding the reaction γγ → π0 π0 we emphasize how the f0(980) signal emerges in γγ → ππ within the dispersive approach and how this fixes to a large extent the phase of the isoscalar S-wave γγ → ππ amplitude above the KK̄ threshold. This allows us to make sharper predictions for the cross section at lower energies and our results could then be used to distinguish between different ππ isoscalar S-wave parameterizations with the advent of new precise data on γγ → π0π0. We also pay special attention to the role played by the σ resonance in γγ → ππ and calculate its coupling and width to γγ, for which we obtain Λ(σ → γγ) = ( 1.68 ± 0.15) KeV. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.
format CONF
author Roca, L.
Oller, J.A.
Schat, C.
author_facet Roca, L.
Oller, J.A.
Schat, C.
author_sort Roca, L.
title Scalar radius of the pion and γγ → ππ
title_short Scalar radius of the pion and γγ → ππ
title_full Scalar radius of the pion and γγ → ππ
title_fullStr Scalar radius of the pion and γγ → ππ
title_full_unstemmed Scalar radius of the pion and γγ → ππ
title_sort scalar radius of the pion and γγ → ππ
url http://hdl.handle.net/20.500.12110/paper_18248039_v_n_p_Roca
work_keys_str_mv AT rocal scalarradiusofthepionandngpp
AT ollerja scalarradiusofthepionandngpp
AT schatc scalarradiusofthepionandngpp
_version_ 1807319810483159040