Relativistic N-boson systems bound by pair potentials V(r_{ij}) = g(r_{ij}^2)
arXiv:math-ph/0405025 · doi:10.1063/1.1767298
Abstract
We study the lowest energy E of a relativistic system of N identical bosons bound by pair potentials of the form V(r_{ij}) = g(r_{ij}^2) in three spatial dimensions. In natural units hbar = c = 1 the system has the semirelativistic `spinless-Salpeter' Hamiltonian H = \sum_{i=1}^N \sqrt{m^2 + p_i^2} + \sum_{j>i=1}^N g(|r_i - r_j|^2), where g is monotone increasing and has convexity g'' >= 0. We use `envelope theory' to derive formulas for general lower energy bounds and we use a variational method to find complementary upper bounds valid for all N >= 2. In particular, we determine the energy of the N-body oscillator g(r^2) = c r^2 with error less than 0.15% for all m >= 0, N >= 2, and c > 0.
15 pages, 4 figures
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- Numerical tests of the envelope theory for few-boson systems
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- Klein-Gordon lower bound to the semirelativistic ground-state energy
- Some equivalences between the auxiliary field method and the envelope theory
- The auxiliary field method in quantum mechanics
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- Tests of the Envelope Theory in One Dimension
- Binding energies of semirelativistic N-boson systems
- Gravitating semirelativistic N-boson systems
- Approximate solutions for N-body Hamiltonians with identical particles in D dimensions
- Quasi Kepler's third law for quantum many-body systems
- Bound cyclic systems with the envelope theory
- Exact solutions for semirelativistic problems with non-local potentials
- Envelope Theory for Systems with Different Particles
- Improvement of the Envelope Theory for Systems with Different Particles
- Tests of the envelope theory for three-body forces
- Compact equations for the envelope theory
- Accuracy Tests of the Envelope Theory
- Upper bounds for critical coupling constants for binding some quantum many-body systems