2012
DOI: 10.1063/1.3682244
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Non-Born-Oppenheimer electronic and nuclear densities for a Hooke-Calogero three-particle model: Non-uniqueness of density-derived molecular structure

Abstract: We consider the calculation of non-Born-Oppenheimer, nBO, one-particle densities for both electrons and nuclei. We show that the nBO one-particle densities evaluated in terms of translationally invariant coordinates are independent of the wavefunction describing the motion of center of mass of the whole system. We show that they depend, however, on an arbitrary reference point from which the positions of the vectors labeling the particles are determined. We examine the effect that this arbitrary choice has on … Show more

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Cited by 15 publications
(16 citation statements)
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“…Note also that (27) and the zero overall momentum of the basis function in the LF Cartesian representation is guaranteed if c u = 0. The condition c u = 0 is equivalent to the requirement It is convenient to consider various coordinates for the calculations, for at least two reasons.…”
Section: Linear Transformation Of the Coordinates Channelsmentioning
confidence: 99%
“…Note also that (27) and the zero overall momentum of the basis function in the LF Cartesian representation is guaranteed if c u = 0. The condition c u = 0 is equivalent to the requirement It is convenient to consider various coordinates for the calculations, for at least two reasons.…”
Section: Linear Transformation Of the Coordinates Channelsmentioning
confidence: 99%
“…However, we can define some auxiliary tools which may be helpful in understanding the process of emerging the molecular shape from a shapeless, spherically-symmetric structure given by the square of the many-body wavefunction. One of these tools is the operator of the oneparticle density of mass 4,12 exemplified in Eqs. 10 and 58.…”
Section: Final Remarksmentioning
confidence: 99%
“…3. Very recently, in two very interesting works 4,5 Ludẽna et al have demonstrated that the one-particle density of mass distribution, for a state described by a given wavefunction, strongly depends on the choice of the reference point. In a way, this issue may be traced back to the very beginning of the modern science: the difference between the Ptolemean and the Copernican representations of the Solar System may also be reduced to a difference in the choice of the reference point.…”
Section: Introductionmentioning
confidence: 99%
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