Some specific solutions to the translation-invariant N-body harmonic oscillator Hamiltonian (original) (raw)

The quantum n-body problem in dimension d ⩾ n – 1: ground state

Journal of Physics A: Mathematical and Theoretical

We employ generalized Euler coordinates for the n body system in d ≥ n − 1 dimensional space, which consists of the centre-of-mass vector, relative (mutual), mass-independent distances r ij and angles as remaining coordinates. We prove that the kinetic energy of the quantum n-body problem for d ≥ n − 1 can be written as the sum 2-dimensional quantum particle in curved space. This was verified for n = 2, 3, 4. After de-quantization the similaritytransformed ∆ rad becomes the Hamiltonian of the classical top with variable tensor of inertia in an external potential. This approach allows a reduction of the dn-dimensional spectral problem to a n(n−1) 2-dimensional spectral problem if the eigenfunctions depend only on relative distances. We prove that the ground state function of the n body problem depends on relative distances alone.

The quantum N-body problem

Journal of Mathematical Physics, 2000

This selective review is written as an introduction to the mathematical theory of the Schro ¤ d inger ¥ equation for N ¦ particles. § Characteristic for these systems are the cluster properties of the potential in configuration space, which are expressed in a simple © geometric language. The methods developed over the last 40 years to deal with this primary aspect are described by giving full proofs of a number of basic and by now classical results. The central theme is the interplay between the spectral theorÿ of N ¦-body Hamiltonians and the space-time and phase-space analysis of bound states and scattering states.

Approximate solutions for N-body Hamiltonians with identical particles in D dimensions

Results in Physics, 2013

A method based on the envelope theory is presented to compute approximate solutions for N-body Hamiltonians with identical particles in D dimensions (D P 2). In some favorable cases, the approximate eigenvalues can be analytically determined and can be lower or upper bounds. The accuracy of the method is tested with several examples, and an application to a N-body system with a minimal length is studied. Finally, a semiclassical interpretation is given for the generic formula of the eigenvalues.

Quantum three body problems using harmonic oscillator bases with different sizes

2000

We propose a new treatment for the quantum three-body problem. It is based on an expansion of the wave function on harmonic oscillator functions with different sizes in the Jacobi coordinates. The matrix elements of the Hamiltonian can be calculated without any approximation and the precision is restricted only by the dimension of the basis. This method can be applied whatever the system under consideration. In some cases, the convergence property is greatly improved in this new scheme as compared to the old traditional method. Some numerical tricks to reduce computer time are also presented.

The Relativistic Many Body Problem in Quantum Mechanics

Symmetries in Science XI, 2005

We discusse a relativistic Hamiltonian for an n-body problem in which all the masses are equal and all spins take value 1/2. In the frame of reference in which the total momentum P = 0, the Foldy-Wouthuysen transformation is applies and the positive energy part of the Hamiltonian is separated. The Hamiltonian with unharmonic oscillator potential is applied to describe mass differences for charmonium and bottonium states. * Member of El Colegio Nacional and Sistema Nacional de Investigadores

Four-body problem in d-dimensional space: Ground state, (quasi)-exact-solvability. IV

Journal of Mathematical Physics, 2019

As a generalization and extension of our previous paper J. Phys. A: Math. Theor. 53 055302 [1], in this work we study a quantum 4-body system in R d (d ≥ 3) with quadratic and sextic pairwise potentials in the relative distances, r ij ≡ |r i − r j |, between particles. Our study is restricted to solutions in the space of relative motion with zero total angular momentum (S-states). In variables ρ ij ≡ r 2 ij , the corresponding reduced Hamiltonian of the system possesses a hidden sl(7; R) Lie algebra structure. In the ρ-representation it is shown that the 4-body harmonic oscillator with arbitrary masses and unequal spring constants is exactly-solvable (ES). We pay special attention to the case of four equal masses and to atomic-like (where one mass is infinite, three others are equal), molecular two-center (two masses are infinite, two others are equal) and molecular threecenter (three infinite masses) cases. In particular, exact results in the molecular case are compared with those obtained within the Born-Oppenheimer approximation. The first and second order symmetries of non-interacting system are searched. Also, the reduction to the lower dimensional cases d = 1, 2 is discussed. It is shown that for four body harmonic oscillator case there exists an infinite family of eigenfunctions which depend on the single variable which is the moment-of-inertia of the system.

N -body gravity and the Schrödinger equation

Classical and Quantum Gravity, 2007

We consider the problem of the motion of N bodies in a self-gravitating system in two spacetime dimensions. We point out that this system can be mapped onto the quantum-mechanical problem of an N-body generalization of the problem of the H + 2 molecular ion in one dimension. The canonical gravitational N-body formalism can be extended to include electromagnetic charges. We derive a general algorithm for solving this problem, and show how it reduces to known results for the 2-body and 3-body systems.

Spectral Analysis of N-Body Schrodinger Operators

The Annals of Mathematics, 1981

For a large class of two body potentials, we solve two of the main problems in the spectral analysis of multiparticle quantum Hamiltonians: explicitly, we prove that the point spectrum lies in a closed countable set (and describe that set in terms of the eigenvalues of Hamiltonians of subsystems) and that there is no singular continuous spectrum. We accomplish this by extending Mourre's work on three body problems to N-body problems.

Four-body problem in d-dimensional space: Ground state, (quasi)-exact-solvability. IV

Journal of Mathematical Physics

Due to its great importance for applications, we generalize and extend the approach of our previous papers to study aspects of the quantum and classical dynamics of a 4-body system with equal masses in d-dimensional space with interaction depending only on mutual (relative) distances. The study is restricted to solutions in the space of relative motion which are functions of mutual (relative) distances only. The ground state (and some other states) in the quantum case and some trajectories in the classical case are of this type. We construct the quantum Hamiltonian for which these states are eigenstates. For d ≥ 3, this describes a six-dimensional quantum particle moving in a curved space with special d-independent metric in a certain d-dependent singular potential, while for d = 1 it corresponds to a three-dimensional particle and coincides with the A 3 (4-body) rational Calogero model; the case d = 2 is exceptional and is discussed separately. The kinetic energy of the system has a hidden sl(7, R) Lie (Poisson) algebra structure, but for the special case d = 1 it becomes degenerate with hidden algebra sl(4, R). We find an exactlysolvable four-body S 4-permutationally invariant, generalized harmonic oscillator-type potential as well as a quasi-exactly-solvable four-body sextic polynomial type potential with singular terms. Naturally, the tetrahedron whose vertices correspond to the positions of the particles provides pure geometrical variables, volume variables, that lead to exactly solvable models. Their generalization to the n-body system as well as the case of non-equal masses is briefly discussed.