Use este identificador para citar ou linkar para este item: http://repositorio.ufc.br/handle/riufc/46427
Registro completo de metadados
Campo DCValorIdioma
dc.contributor.authorSILVA, Euclimar Passos da-
dc.date.accessioned2019-10-02T19:32:07Z-
dc.date.available2019-10-02T19:32:07Z-
dc.date.issued2001-04-13-
dc.identifier.citationDA SILVA, E. P.pt_BR
dc.identifier.urihttp://www.repositorio.ufc.br/handle/riufc/46427-
dc.descriptionSILVA, E. P. Annihilation probability density in positron scattering by He. 2001.Artigo. Phys. Rev., 13 April 2001.pt_BR
dc.description.abstractWe have calculated annihilation probability densities in positron collisions against the He atom. Our scattering wave functions were obtained with the Schwinger multichannel method [J. S. E. Germano and M. A. P. Lima, Phys. Rev. A 47 , 3976 (1993)]. It has been found that direct annihilation, in which electronic cloud deformation shields the nuclear repulsive potential effectively attracting the positron to a binary encounter, dominates the annihilation process at low impact energies. Closer to the real positronium formation threshold, the signature of virtual positronium has been noticed. At room temperature, significant annihilation probability has been observed over a somewhat extended region.pt_BR
dc.language.isoenpt_BR
dc.publisherThe American Physical Societypt_BR
dc.rightsAcesso Abertopt_BR
dc.subjectannihilation probabilitypt_BR
dc.titleAnnihilation probability density in positron scattering by Hept_BR
dc.typeArtigo de Periódicopt_BR
dc.title.enAnnihilation probability density in positron scattering by Hept_BR
Aparece nas coleções:CSOBRAL - Artigos publicados em revistas científicas

Arquivos associados a este item:
Arquivo Descrição TamanhoFormato 
2001_art_epsilva.pdfSILVA, E. P. Annihilation probability density in positron scattering by He. 2001.Artigo. Phys. Rev., 13 April 2001.73,71 kBAdobe PDFVisualizar/Abrir


Os itens no repositório estão protegidos por copyright, com todos os direitos reservados, salvo quando é indicado o contrário.