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New Families of Isospectral Hydrogen-like potentials  [PDF]
J. Oscar Rosas-Ortiz
Physics , 1998, DOI: 10.1088/0305-4470/31/27/003
Abstract: By applying algebraic techniques, we construct a two-parametric family of strictly isospectral Hydrogen-like potentials as well as some of its one-parametric limits. An additional one-parametric almost isospectral family of Hydrogen-like potentials is also investigated. It is argued that the construction of a SUSY partner Hamiltonian using a factorization energy $\delta$ less than the ground state energy of the departure Hamiltonian is unnecessarily restrictive.
Exactly Solvable Hydrogen-like Potentials and Factorization Method  [PDF]
J. Oscar Rosas-Ortiz
Mathematics , 1998, DOI: 10.1088/0305-4470/31/50/012
Abstract: A set of factorization energies is introduced, giving rise to a generalization of the Schr\"{o}dinger (or Infeld and Hull) factorization for the radial hydrogen-like Hamiltonian. An algebraic intertwining technique involving such factorization energies leads to derive $n$-parametric families of potentials in general almost-isospectral to the hydrogen-like radial Hamiltonians. The construction of SUSY partner Hamiltonians with ground state energies greater than the corresponding ground state energy of the initial Hamiltonian is also explicitly performed.
A new analytical solving for electric polarizabilities of hydrogen-like atoms  [PDF]
V. F. Kharchenko
Physics , 2014,
Abstract: The direct transition-matrix approach to the description of the electric polarization of the quantum bound system of particles is used to determine the electric multipole polarizabilities of the hydrogen-like atoms. It is shown that in the case of the bound system formed by the Coulomb interaction the corresponding inhomogeneous integral equation determining an off-shell scattering function, which consistently describes virtual multiple scattering, can be solved exactly analytically for all electric multipole polarizabilities. Our method allows to reproduce the known Dalgarno-Lewis formula for electric multipole polarizabilities of the hydrogen atom in the ground state and can also be applied to determine the polarizability of the atom in excited bound states.
Electromagnetic Radiation Reaction and Stability of the Hydrogen-Like Atoms  [PDF]
Mohsen Dehghani
Journal of Modern Physics (JMP) , 2011, DOI: 10.4236/jmp.2011.211174
Abstract: Based on a suitable linear combination of the physical and un-physical electromagnetic potentials, the radiation reaction potentials have been calculated. Through the near zone expansion of the potentials, it has been shown that in either of the relativistic and non-relativistic cases the outgoing (radiated) energy of the electrons orbiting the nucleus is substituted by incoming (electromagnetic radiation reaction) energy. This means that energy is conserved and the classical hydrogen-like atoms are stable.
On the new translational shape invariant potentials  [PDF]
Arturo Ramos
Physics , 2011, DOI: 10.1088/1751-8113/44/34/342001
Abstract: Recently, several authors have found new translational shape invariant potentials not present in classic classifications like that of Infeld and Hull. For example, Quesne on the one hand and Bougie, Gangopadhyaya and Mallow on the other have provided examples of them, consisting on deformations of the classical ones. We analyze the basic properties of the new examples and observe a compatibility equation which has to be satisfied by them. We study particular cases of such equation and give more examples of new translational shape invariant potentials.
The g Factor of a Bound Electron in a Hydrogen-Like Atom  [PDF]
Savely G. Karshenboim
Physics , 2000,
Abstract: Recently, a precise measurement on the bound electron g factor in hydrogen-like carbon was performed [1]. We consider the present status of the theory of the g factor of an electron bound in a hydrogen-like atom and discuss new opportunities and possible applications of the recent experiment.
Lattice Boltzmann modeling of water-like fluids  [PDF]
Sauro Succi,Nasrollah Moradi,Andreas Greiner,Simone Melchionna
Frontiers in Physics , 2014, DOI: 10.3389/fphy.2014.00022
Abstract: We review recent advances on the mesoscopic modeling of water-like fluids, based on the lattice Boltzmann (LB) methodology. The main idea is to enrich the basic LB (hydro)-dynamics with angular degrees of freedom responding to suitable directional potentials between water-like molecules. The model is shown to reproduce some microscopic features of liquid water, such as an average number of hydrogen bonds per molecules (HBs) between 3 and 4, as well as a qualitatively correct statistics of the hydrogen bond angle as a function of the temperature. Future developments, based on the coupling the present water-like LB model with the dynamics of suspended bodies, such as biopolymers, may open new angles of attack to the simulation of complex biofluidic problems, such as protein folding and aggregation, and the motion of large biomolecules in complex cellular environments.
On Solvable Potentials, Supersymmetry, and the One-Dimensional Hydrogen Atom  [PDF]
R. P. Martínez-y-Romero, H. N. Núnez-Yépez, A. L. Salas-Brito
Communications and Network (CN) , 2010, DOI: 10.4236/cn.2010.21009
Abstract: The ways for improving on techniques for finding new solvable potentials based on supersymmetry and shape invariance has been discussed by Morales et al. [1] In doing so they address the peculiar system known as the one-dimensional hydrogen atom. In this paper we show that their remarks on such problem are mistaken. We do this by explicitly constructing both the one-dimensional Coulomb potential and the superpotential associated with the problem, objects whose existence are denied in the mentioned paper.
Potentials and distribution functions to be used for dynamical modeling with GAIA-like data  [PDF]
B. Famaey,H. Dejonghe
Physics , 2001, DOI: 10.1051/eas:2002038
Abstract: We present new tools to establish axisymmetric equilibrium models of the Milky Way. The models we wish to establish are pairs (V,F) where V is the gravitational potential generated by the whole mass distribution including the dark matter, and F is the distribution function in phase space for late-type tracer stars. We present a set of Stackel potentials that fit some fundamental parameters of the Milky Way (mass density in the solar neighbourhood and Oort constants). Then we define new component distribution functions that can be combined with these potentials in order to reproduce kinematical data like those that will be provided by GAIA.
Non-Hermitian SUSY Hydrogen-like Hamiltonians with real spectra  [PDF]
Oscar Rosas-Ortiz,Rodrigo Munoz
Physics , 2003, DOI: 10.1088/0305-4470/36/31/311
Abstract: It is shown that the radial part of the Hydrogen Hamiltonian factorizes as the product of two not mutually adjoint first order differential operators plus a complex constant epsilon. The 1-susy approach is used to construct non-hermitian Hamiltonians with hydrogen spectra. Other non-hermitian Hamiltonians are shown to admit an extra `complex energy' at epsilon. New self-adjoint hydrogen-like Hamiltonians are also derived by using a 2-susy transformation with complex conjugate pairs epsilon, (c.c) epsilon.
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