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Poul Jo

Researcher at Aarhus University

Publications -  84
Citations -  9887

Poul Jo is an academic researcher from Aarhus University. The author has contributed to research in topics: Coupled cluster & Propagator. The author has an hindex of 45, co-authored 84 publications receiving 9419 citations.

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Linear response calculations for large scale multiconfiguration self‐consistent field wave functions

TL;DR: In this paper, it was shown that large scale MCSCF linear response (MCLR) calculations can be carried out efficiently using an iterative algorithm where the linear transformations are carried out directly, i.e., without explicitly constructing the MCLR matrices.
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Quadratic response functions for a multiconfigurational self‐consistent field wave function

TL;DR: In this paper, an efficient implementation of the quadratic response function for a multiconfiguration self-consistent field reference wave function is described. And sample calculations for the hyperpolarizability of Ne and for the two-photon transition matrix elements of H2 are presented.
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Hartree-Fock limit magnetizabilities from London orbitals

TL;DR: In this paper, the Hartree-Fock limit for a series of diamagnetic molecules was calculated using London atomic orbitals using London basis sets of moderate size, in contrast to calculations of molecular polarizabilities which require large basis sets to be reliable.
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Integral-direct coupled cluster calculations of frequency-dependent polarizabilities, transition probabilities and excited-state properties

TL;DR: In this article, an atomic integral-direct implementation of molecular linear response properties and excited-state one-electron properties is presented for the coupled cluster models CCS, CC2, and CCSD.
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Mo/ller–Plesset energy derivatives

TL;DR: In this paper, a variational Mo/ller-Plesset energy functional (Lagrangian) which is variational in all variables (the Lagrange multipliers, the orbital rotation parameters, and the orbital energies) is constructed, which ensures that the responses of the orbitals and orbital energies to n in geometrical perturbations determine the energy derivatives to order 2n+1.