Semi-relativistic stability and critical mass of a system of spinless bosons in gravitational interaction
From MaRDI portal
Publication:257992
DOI10.1016/0370-2693(89)91331-2zbMath1332.82009OpenAlexW2064096369MaRDI QIDQ257992
F. Blanchet-Sadri, M. Dambrine
Publication date: 17 March 2016
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: http://cds.cern.ch/record/201298
Related Items (17)
SEMIRELATIVISTIC TREATMENT OF BOUND STATES ⋮ DISCRETE SPECTRA OF SEMIRELATIVISTIC HAMILTONIANS FROM ENVELOPE THEORY ⋮ Convexity and potential sums for Salpeter-type Hamiltonians ⋮ Relativistic N-boson systems bound by pair potentials V(rij)=g(rij2) ⋮ The spinless relativistic kink-like problem ⋮ Lower Bounds for the Spinless Salpeter Equation ⋮ Upper limit on the number of bound states of the spinless Salpeter equation ⋮ The one-dimensional spinless Salpeter Coulomb problem with minimal length ⋮ The zero-mass spinless Salpeter equation with a regularized inverse square potential ⋮ The spinless relativistic Hellmann problem ⋮ The one-dimensional spinless relativistic Coulomb problem ⋮ Upper limit on the critical strength of central potentials in relativistic quantum mechanics ⋮ The spinless relativistic Hulthén problem ⋮ Energy bounds for the spinless Salpeter equation ⋮ The rest-frame Darwin potential from the Lienard-Wiechert solution in the radiation gauge ⋮ DISCRETE SPECTRA OF SEMIRELATIVISTIC HAMILTONIANS ⋮ Relativistic harmonic oscillator
Cites Work
This page was built for publication: Semi-relativistic stability and critical mass of a system of spinless bosons in gravitational interaction
