Self-energies for the particle-hole propagator from Feynman-Dyson equations

Correlation-relaxation corrections to electronic transition energies are obtained through the self-energy fields for the particle-hole propagator. These objects are generated from Feynman-Dyson like equations within the scenario of the superoperator algebra. A Hartree-Fock reference state and a part...

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Autor principal: Bochicchio, Roberto Carlos
Otros Autores: Ferraro, Marta Beatriz, Grinberg, H., Cavasotto, C.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 1995
Acceso en línea:Registro en Scopus
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100 1 |a Bochicchio, Roberto Carlos 
245 1 0 |a Self-energies for the particle-hole propagator from Feynman-Dyson equations 
260 |c 1995 
270 1 0 |m Grinberg, H.; Departamento de Fisica, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Ciudad Universitaria, 1428 Buenos Aires, Argentina 
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506 |2 openaire  |e Política editorial 
520 3 |a Correlation-relaxation corrections to electronic transition energies are obtained through the self-energy fields for the particle-hole propagator. These objects are generated from Feynman-Dyson like equations within the scenario of the superoperator algebra. A Hartree-Fock reference state and a partition of the operator space along with a particle conserving manifold are used to recast the lower order perturbative expressions for the self-energies. Correlated states are used to make explicit the appearance of higher order correction terms to the self-energy. It is explicitly shown that the present scheme leads to a proper classification of the order of the contribution from both the intrinsic interaction operator and the improved reference state. © 1995.  |l eng 
536 |a Detalles de la financiación: EX-093, 3538/93a 
536 |a Detalles de la financiación: Fundación Antorchas 
536 |a Detalles de la financiación: This work has been madep ossibleb y research grantsi n aid from the University of BuenosA ires (ProjectN o. EX-093, Res. No. 3538/93a) nd Con-sejo National de InvestigacionesC ientificas y Tecnicas, Republica Argentina (Res. No. 1047-48/93). The authors are grateful to the Department of Physics, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, for facilitiesp rovidedd uring the courseo f this work. Financial support ‘from Antorchas Foundation (Res. A-12830/1-00007i0s) g reatlya cknowledged. 
593 |a Departamento de Fisica, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Ciudad Universitaria, 1428 Buenos Aires, Argentina 
700 1 |a Ferraro, Marta Beatriz 
700 1 |a Grinberg, H. 
700 1 |a Cavasotto, C. 
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