Zero-Energy Bound States of Neutron–Neutron or Neutron–Muon Systems

Author:

Oks Eugene1

Affiliation:

1. Physics Department, 380 Duncan Drive, Auburn University, Auburn, AL 36849, USA

Abstract

There exists the following paradigm: for interaction potentials U(r) that are negative and go to zero as r goes to infinity, bound states may exist only for the negative total energy E. For E > 0 and for E = 0, bound states are considered to be impossible, both in classical and quantum mechanics. In the present paper we break this paradigm. Namely, we demonstrate the existence of bound states of E = 0 in neutron–neutron systems and in neutron–muon systems, specifically when the magnetic moments of the two particles in the pair are parallel to each other. As particular examples, we calculate the root-mean-square size of the bound states of these systems for the values of the lowest admissible values of the angular momentum, and show that it exceeds the neutron radius by an order of magnitude. We also estimate the average kinetic energy and demonstrate that it is nonrelativistic. The corresponding bound states of E = 0 may be called “neutronium” (for the neutron–neutron systems) and “neutron–muonic atoms” (for the neutron–muon systems). We also point out that this physical system possesses higher-than-geometric (i.e., algebraic) symmetry, leading to the approximate conservation of the square of the angular momentum, despite the geometric symmetry being axial. We use this fact for facilitating analytical and numerical calculations.

Publisher

MDPI AG

Reference10 articles.

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2. Landau, L.D., and Lifshitz, E.M. (1962). The Classical Theory of Fields, Pergamon.

3. Beletsky, V.V. (2001). Essays on the Motion of Celestial Bodies, Birkhäuser/Springer.

4. Analytical Solution for the Three-Dimensional Motion of a Circumbinary Planet Around a Binary Star;Oks;New Astron.,2020

5. Circular Binary Star and an Interstellar Interloper: The Analytical Solution;Oks;New Astron.,2021

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