On essential self-adjointness for magnetic Schroedinger and Pauli operators on the unit disc in R^2

Details On essential self-adjointness for magnetic Schroedinger and Pauli operators on the unit disc in R^2 On essential self-adjointness for magnetic Schroedinger and Pauli operators on the unit disc in R^2

2010-03-16

arxiv.org/abs/1003.3099v2

Physics

Mathematical Physics

18 pages; the main theorem has been expanded and generalized

Scientific paper

We study the question of magnetic confinement of quantum particles on the unit disk $\ID$ in $\IR^2$, i.e. we wish to achieve confinement solely by means of the growth of the magnetic field $B(\vec x)$ near the boundary of the disk. In the spinless case we show that $B(\vec x)\ge \frac{\sqrt 3}{2}\cdot\frac{1}{(1-r)^2}-\frac{1}{\sqrt 3}\frac{1}{(1-r)^2\ln \frac{1}{1-r}}$, for $|\vec x|$ close to 1, insures the confinement provided we assume that the non-radially symmetric part of the magnetic field is not very singular near the boundary. Both constants $\frac{\sqrt 3}{2}$ and $-\frac{1}{\sqrt 3}$ are optimal. This answers, in this context, an open question from Y. Colin de Verdi\`ere and F. Truc. We also derive growth conditions for radially symmetric magnetic fields which lead to confinement of spin 1/2 particles.

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