Stability of Relativistic Matter With Magnetic Fields
Elliott H. Lieb, Heinz Siedentop, Jan Philip Solovej

TL;DR
This paper demonstrates that incorporating magnetic fields into relativistic quantum models of matter using the Dirac operator can ensure stability, resolving previous uncertainties about combined effects.
Contribution
It introduces a formulation using the Dirac operator with magnetic fields to establish stability of relativistic matter with Coulomb forces.
Findings
Using the Dirac operator with magnetic fields ensures stability.
The free Dirac operator leads to instability for any fine structure constant.
Properly defining the negative energy sea is crucial for stability.
Abstract
Stability of matter with Coulomb forces has been proved for non-relativistic dynamics, including arbitrarily large magnetic fields, and for relativistic dynamics without magnetic fields. In both cases stability requires that the fine structure constant alpha be not too large. It was unclear what would happen for both relativistic dynamics and magnetic fields, or even how to formulate the problem clearly. We show that the use of the Dirac operator allows both effects, provided the filled negative energy `sea' is defined properly. The use of the free Dirac operator to define the negative levels leads to catastrophe for any alpha, but the use of the Dirac operator with magnetic field leads to stability.
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