Colección SciELO Chile

Departamento Gestión de Conocimiento, Monitoreo y Prospección
Consultas o comentarios: productividad@anid.cl
Búsqueda Publicación
Búsqueda por Tema Título, Abstract y Keywords



Coherent and incoherent vector meson electroproduction in the future electron - ion colliders: The hot - spot predictions
Indexado
WoS WOS:000478705300013
Scopus SCOPUS_ID:85067456314
DOI 10.1016/J.NUCLPHYSA.2019.06.009
Año 2019
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



One of the more promising observables to probe the high energy regime of the QCD dynamics in the future Electron - Ion Colliders (EIC) is the exclusive vector meson production cross section in coherent and incoherent interactions. Such processes measure the average spatial distribution of gluons in the target as well the fluctuations and correlations in the gluon density. In this paper we present a comprehensive analysis of the energy, photon virtuality, atomic number and momentum transfer dependencies of the coherent and incoherent cross sections considering two different models for the nuclear profile function. In particular, we present the predictions of the hot - spot model, which assumes the presence of subnucleonic degrees of freedom and an energy-dependent profile. Our results indicate that the analysis of the ratio between the incoherent and coherent cross sections and the momentum transfer distributions in the future EIC can be useful to constrain the description of the hadronic structure at high energies. (C) 2019 Elsevier B.V. All rights reserved.

Revista



Revista ISSN
Nuclear Physics A 0375-9474

Métricas Externas



PlumX Altmetric Dimensions

Muestra métricas de impacto externas asociadas a la publicación. Para mayor detalle:

Disciplinas de Investigación



WOS
Physics, Nuclear
Scopus
Nuclear And High Energy Physics
SciELO
Sin Disciplinas

Muestra la distribución de disciplinas para esta publicación.

Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



Muestra la distribución de colaboración, tanto nacional como extranjera, generada en esta publicación.


Autores - Afiliación



Ord. Autor Género Institución - País
1 Krelina, M. Hombre Universidad Técnica Federico Santa María - Chile
Czech Tech Univ - República Checa
Ceské vysoké ucení technické v Praze - República Checa
Czech Technical University in Prague - República Checa
2 Goncalves, Victor P. Hombre Univ Fed Pelotas - Brasil
Universidade Federal de Pelotas - Brasil
3 Cepila, J. - Czech Tech Univ - República Checa
Ceské vysoké ucení technické v Praze - República Checa
Czech Technical University in Prague - República Checa

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Financiamiento



Fuente
CONICYT FONDECYT
CNPq
Fundação de Amparo à Pesquisa do Estado do Rio Grande do Sul
Conselho Nacional de Desenvolvimento Científico e Tecnológico
Ministry of Education, Youth and Sports of the Czech Republic
Grantová Agentura Ceské Republiky
FAPERGS
Consejo Nacional de Innovacion, Ciencia y Tecnologia
Czech Science Foundation (GACR)
17-04505S of the Czech Science Foundation
Ministerstvo Školství, Mládeže a Tělovýchovy
CONICYT Fondecyt (Chile)
Conselho Nacional de Desenvolvimento Científico e Tecnológico
INCT-FNA
programme CESNET of the Czech Republic
Instituto Nacional de Ciência e Tecnologia: Física Nuclear e Aplicações
Ministerio de Educación, Cultura y Deporte
Grantová Agentura České Republiky
Fundação de Amparo à Pesquisa do Estado do Rio Grande do Sul
Instituto Nacional de Ciência e Tecnologia: Física Nuclear e Aplicações

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
The authors are deeply grateful to the very useful discussions with J. G. Contreras and J. D. Tapia Takaki. VPG is grateful to the members of the Department of Physics and Astronomy of the University of Kansas by the warm hospitality during the initial phase of this study. JC has been supported by the grant 17-04505S of the Czech Science Foundation (GACR). VPG was partially financed by the Brazilian funding agencies CNPq, FAPERGS and INCT-FNA (process number 464898/2014-5). MK was supported by the CONICYT Fondecyt grant Postdoctorado N. 3180085 (Chile) and by the grant LTC17038 of the Ministry of Education, Youth and Sports of the Czech Republic. Access to computing and storage facilities of the National Grid Infrastructure MetaCentrum provided under the programme CESNET LM2015042 of the Czech Republic is greatly appreciated.
The authors are deeply grateful to the very useful discussions with J. G. Contreras and J. D. Tapia Takaki. VPG is grateful to the members of the Department of Physics and Astronomy of the University of Kansas by the warm hospitality during the initial phase of this study. JC has been supported by the grant 17-04505S of the Czech Science Foundation (GACR). VPG was partially financed by the Brazilian funding agencies CNPq, FAPERGS and INCT-FNA (process number 464898/2014-5). MK was supported by the CONICYT Fondecyt grant Postdoctorado N. 3180085 (Chile) and by the grant LTC17038 of the Ministry of Education, Youth and Sports of the Czech Republic. Access to computing and storage facilities of the National Grid Infrastructure MetaCentrum provided under the programme CESNET LM2015042 of the Czech Republic is greatly appreciated.

Muestra la fuente de financiamiento declarada en la publicación.