Nucleon gravitational form factors

A symmetry-preserving analysis of strong interaction quantum field equations is used to complete a unified treatment of pion, kaon, and nucleon electromagnetic and gravitational form factors. Findings include a demostration that the pion near-core pressure is roughly twice that in the proton, so bot...

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Detalles Bibliográficos
Autores: Yao, Zhao-Quian, Xu, Yinzhen, Binosi, Daniele, Cui, Zhu-Fang, Ding, Minghui, Raya, Khépani, Roberts, Craig D., Rodríguez Quintero, José, Schmidt, S. M.
Tipo de recurso: artículo
Fecha de publicación:2025
País:España
Institución:Universidad de Huelva (UHU)
Repositorio:Arias Montano. Repositorio Institucional de la Universidad de Huelva
Idioma:inglés
OAI Identifier:oai:ariasmontano.uhu.es:10272/27999
Acceso en línea:https://hdl.handle.net/10272/27999
Access Level:acceso abierto
Palabra clave:2212 Física Teórica
Descripción
Sumario:A symmetry-preserving analysis of strong interaction quantum field equations is used to complete a unified treatment of pion, kaon, and nucleon electromagnetic and gravitational form factors. Findings include a demostration that the pion near-core pressure is roughly twice that in the proton, so both are significantly greater than that of a neutron star; parton species separations of the nucleon’s three gravitational form factors, in which, inter alia, the glue-to-quark ratio for each form factor is seen to take the same constant value, independent of momentum transfer; and a determination of proton radii orderings, with the mechanical (normal force) radius being less than the mass-energy radius, which is less than the proton charge radius. This body of predictions should prove useful in an era of experiments that will enable them to be tested.