Abstract
We consider the quantum mechanical many-body problem of electrons and fixed nuclei interacting via Coulomb forces, but with a relativistic form for the kinetic energy, namely p 2 /2m is replaced by (p 2 c 2 + m 2 c 4 ) 1/2 — mc 2 . The electrons are allowed to have q spin states (q = 2 in nature). For one electron and one nucleus instability occurs if Zα>2/π, where z is the nuclear charge and a is the fine structure constant. We prove that stability occurs in the many-body case if z α ≦ 2/π and α l/(47q). For small z, a better bound on a is also given. In the other direction we show that there is a critical αc (no greater than 128/15π) such that if α>αc then instability always occurs for all positive z (not necessarily integral) when the number of nuclei is large enough. Several other results of a technical nature are also given such as localization estimates and bounds for the relativistic kinetic energy.
Work partially supported by U.S. National Science Foundation grant PHY-85–15288-A02
The author thanks the Institute for Advanced Study for its hospitality and the U.S. National Science Foundation for support under grant DMS-8601978
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Lieb, E.H., Yau, HT. (2001). The Stability and Instability of Relativistic Matter. In: Thirring, W. (eds) The Stability of Matter: From Atoms to Stars. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-04360-8_34
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DOI: https://doi.org/10.1007/978-3-662-04360-8_34
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