Can induced orbital paramagnetism be controlled by strong magnetic fields?
Magnetic hypersusceptibilities and hypershielding at the nuclei of BH, CH+,C4H4, and C8H8 molecules in the presence of an external spatially uniform, time-independent magnetic field have been investigated accounting for cubic response contributions via Rayleigh-Schrödinger perturbation theory. Numer...
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paper:paper_15499618_v5_n11_p3049_Pagola2023-06-08T16:21:28Z Can induced orbital paramagnetism be controlled by strong magnetic fields? Pagola, Gabriel Ignacio Ferraro, Marta Beatriz Magnetic hypersusceptibilities and hypershielding at the nuclei of BH, CH+,C4H4, and C8H8 molecules in the presence of an external spatially uniform, time-independent magnetic field have been investigated accounting for cubic response contributions via Rayleigh-Schrödinger perturbation theory. Numerical estimates have been obtained at the coupled Hartree-Fock and density-functional levels of theory within the conventional common-origin approach, using extended gaugeless basis sets. The fundamental role of electron correlation effects was assessed. Critical values of the applied magnetic field at which transition from paramagnetic to diamagnetic behavior would occur were estimated. It is shown that perturbative methods may successfully be employed to estimate the interaction energy for big cyclic molecules. © 2009 American Chemical Society. Fil:Pagola, G.I. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Ferraro, M.B. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2009 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15499618_v5_n11_p3049_Pagola http://hdl.handle.net/20.500.12110/paper_15499618_v5_n11_p3049_Pagola |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
description |
Magnetic hypersusceptibilities and hypershielding at the nuclei of BH, CH+,C4H4, and C8H8 molecules in the presence of an external spatially uniform, time-independent magnetic field have been investigated accounting for cubic response contributions via Rayleigh-Schrödinger perturbation theory. Numerical estimates have been obtained at the coupled Hartree-Fock and density-functional levels of theory within the conventional common-origin approach, using extended gaugeless basis sets. The fundamental role of electron correlation effects was assessed. Critical values of the applied magnetic field at which transition from paramagnetic to diamagnetic behavior would occur were estimated. It is shown that perturbative methods may successfully be employed to estimate the interaction energy for big cyclic molecules. © 2009 American Chemical Society. |
author |
Pagola, Gabriel Ignacio Ferraro, Marta Beatriz |
spellingShingle |
Pagola, Gabriel Ignacio Ferraro, Marta Beatriz Can induced orbital paramagnetism be controlled by strong magnetic fields? |
author_facet |
Pagola, Gabriel Ignacio Ferraro, Marta Beatriz |
author_sort |
Pagola, Gabriel Ignacio |
title |
Can induced orbital paramagnetism be controlled by strong magnetic fields? |
title_short |
Can induced orbital paramagnetism be controlled by strong magnetic fields? |
title_full |
Can induced orbital paramagnetism be controlled by strong magnetic fields? |
title_fullStr |
Can induced orbital paramagnetism be controlled by strong magnetic fields? |
title_full_unstemmed |
Can induced orbital paramagnetism be controlled by strong magnetic fields? |
title_sort |
can induced orbital paramagnetism be controlled by strong magnetic fields? |
publishDate |
2009 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15499618_v5_n11_p3049_Pagola http://hdl.handle.net/20.500.12110/paper_15499618_v5_n11_p3049_Pagola |
work_keys_str_mv |
AT pagolagabrielignacio caninducedorbitalparamagnetismbecontrolledbystrongmagneticfields AT ferraromartabeatriz caninducedorbitalparamagnetismbecontrolledbystrongmagneticfields |
_version_ |
1768546270276747264 |