English

N-body problem with contact interactions

Mathematical Physics 2017-12-19 v2 math.MP

Abstract

We introduce \emph{contact interactions hamiltonians} (self-adjointoperators defined by boundary conditions) between NN massive particles in R3R^3, N3N \geq 3. We prove that they are limits (in strong resolvent sense) when ϵ0 \epsilon \to 0 of interaction through a two-body potential which scales according to Vϵ(x)=ϵ3V(xϵ) V_\epsilon (|x|) =\epsilon ^{-3} V ( \frac {|x|}{ \epsilon} ) where V(x) V(|x|) is an integrable function. The advantage of the formalism of contact interactions is that the results do not depend on the shape of the approximating potentials. Depending on the masses and symmetries there may be three body bound states with wave function localized near the barycenter and less localized four-body bound states. For some range of masses there is an infinity of bound states with energies which accumulate geometrically to zero (Efimov effect). For contact interactions these are all the bound states which can be present in the NN-body system. We study of zero range hamiltonians by first compactly embedding the physical space L2(R3(N1)) L^2(R^{3 (N-1)}) in a larger Hilbert space of more singular functions (Krein space) Estimates are done in the auxiliary space, where strong resolvent convergence when ϵ0 \epsilon \to 0 and spectral properties are easily established. If the hamiltonian \emph{in Krein space} is positive, coming back to L2(R3N)L^2 (R^{3N}) is done using the compactness of the Krein map and the fact that for positive forms weak convergence implies strong convergence. If it is not positive we use a somewhat more sophisticated operation, Γ \Gamma-convergence [Dal]. In both cases the limit operator is unique.

Keywords

Cite

@article{arxiv.1711.10200,
  title  = {N-body problem with contact interactions},
  author = {Gianfausto Dell'Antonio},
  journal= {arXiv preprint arXiv:1711.10200},
  year   = {2017}
}

Comments

typo errors correcten

R2 v1 2026-06-22T22:59:10.909Z