Energy bounds for the spinless Salpeter equation

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Energy Bounds for the Spinless Salpeter Equation

We study the spectrum of the Salpeter Hamiltonian H = β √ m2 + p2 +V (r), where V (r) is an attractive central potential in three dimensions. If V (r) is a convex transformation of the Coulomb potential −1/r and a concave transformation of the harmonic-oscillator potential r, then upper and lower bounds on the discrete eigenvalues of H can be constructed, which may all be expressed in the form ...

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Energy Bounds for the Spinless Salpeter Equation: Harmonic Oscillator

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Lower Bounds for the Spinless Salpeter Equation

We obtain lower bounds on the ground state energy, in one and three dimensions, for the spinless Salpeter equation (Schrödinger equation with a relativistic kinetic energy operator) applicable to potentials for which the attractive parts are in L(R) for some p > n (n = 1 or 3). An extension to confining potentials, which are not in L(R), is also presented.

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The spinless Salpeter equation may be considered either as a standard approximation to the Bethe–Salpeter formalism, designed for the description of bound states within a relativistic quantum field theory, or as the most simple, to a certain extent relativistic generalization of the costumary nonrelativistic Schrödinger formalism. Because of the presence of the rather difficult-to-handle square...

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ژورنال

عنوان ژورنال: Journal of Mathematical Physics

سال: 2001

ISSN: 0022-2488,1089-7658

DOI: 10.1063/1.1405848