1992
DOI: 10.1103/physrevd.45.1233
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Spinless Salpeter equation as a simple matrix eigenvalue problem

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Cited by 22 publications
(24 citation statements)
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“…[8]. These approaches include, among others, the development of elaborate numerical approximation methods [9,10,11] as well as the construction of effective Hamiltonians which, in spite of their apparently nonrelativistic form, incorporate relativistic effects by sophisticated momentum dependence of the involved parameters [12]. A lot of information on the solutions of the spinless Salpeter equation may even be gained by application of a relativistic virial theorem [13], most easily derived from a rather general "master virial theorem" [14].…”
Section: Introduction: the Spinless Salpeter Equationmentioning
confidence: 99%
“…[8]. These approaches include, among others, the development of elaborate numerical approximation methods [9,10,11] as well as the construction of effective Hamiltonians which, in spite of their apparently nonrelativistic form, incorporate relativistic effects by sophisticated momentum dependence of the involved parameters [12]. A lot of information on the solutions of the spinless Salpeter equation may even be gained by application of a relativistic virial theorem [13], most easily derived from a rather general "master virial theorem" [14].…”
Section: Introduction: the Spinless Salpeter Equationmentioning
confidence: 99%
“…Neglecting, furthermore, any reference to the spin degrees of freedom and restricting to positive energy solutions, one arrives at the SS equation, which is the correct tool to deal with the boundstate spectrum of qq, QQ and Qq or qQ (where q = u, d, s and Q = c, b, t) interacting via some effective potential with no spin dependence, i.e., spin-averaged data (SAD). This equation was solved analytically and then numerically for its bound-state energies using different techniques by many authors [3][4][5][6][7][8][9][10].…”
Section: Introductionmentioning
confidence: 99%
“…3 The prescription and the wave equation used are responsible for the deterioration of the fit parameters. The calculation and parameters are also model dependent as remarked in our earlier papers [10,31].…”
mentioning
confidence: 99%
“…. , d−1, which allows us to localize eigenvalues by upper bounds of increasing tightness [13,14] for rising d. We find and have always found [15][16][17][18][19][20][21][22][23][24] it advantageous to span these finite-dimensional variational trial subspaces by a basis the representations of which are known analytically in both configuration and momentum space (related, of course, by Fourier transformation): in this case, the expectation values of H may be analytically given by evaluating those of T (p) in momentum space and those of V (x) in configuration space. By spherical symmetry, each basis vector factorizes into the product of a radial part and a spherical harmonic Y ℓm (Ω) for angular momentum ℓ and projection m depending on the solid angle Ω.…”
Section: Relativistic Kinematics: Variational Upper Limits By Rayleigmentioning
confidence: 73%