Background:The variational Hartree-Fock-Bogoliubov (HFB) mean-field theory is the starting point of various (ab initio) many-body methods dedicated to superfluid systems. In this context, pairing correlations may be driven towards zero either on purpose via HFB calculations constrained on, e.g., the particle-number variance or simply because inter-nucleon interactions cannot sustain pairing correlations in the first place in, e.g., closed-shell systems. While taking this limit constitutes a text-book problem when the system is of closed-(sub)shell character, it is typically, although wrongly, thought to be ill-defined whenever the naive filling of single-particle levels corresponds to an open-shell system.
Purpose:The present work demonstrates that the zero-pairing limit of an HFB state is well-defined independently of the average particle number A it is constrained to. Still, the nature of the limit state is shown to depend of the regime, i.e., on whether the nucleus characterizes as a closed-(sub)shell or an open-shell system when taking the limit. Finally, the consequences of the zero-pairing limit on Bogoliubov many-body perturbation theory (BMBPT) calculations performed on top of the HFB reference state are illustrated.Methods: The zero-pairing limit of a HFB state constrained to carry an arbitrary (integer) number of particles A on average is worked out analytically and realized numerically using a two-nucleon interaction derived within the frame of chiral effective field theory.Results: The zero-pairing limit of the HFB state is mathematically well-defined, independently of the closedor open-shell character of the system in the limit. Still, the nature of the limit state strongly depends on the underlying shell structure and on the associated naive filling reached in the zero-pairing limit for the particle number A of interest. First, the text-book situation is recovered for closed-(sub)shell systems, i.e., the limit state is reached for a finite value of the inter-nucleon interaction (the well-known BCS collapse) and takes the form of a single Slater determinant displaying (i) zero pairing energy, (ii) non-degenerate elementary excitations and (iii) zero particle-number variance. Contrarily, a non-standard situation is obtained for open-shell systems, i.e., the limit state is only reached for a zero value of the pairing interaction (no BCS collapse) and takes the form of a specific finite linear combination of Slater determinants displaying (a) a non-zero pairing energy, (b) degenerate elementary excitations and (c) a non-zero particle-number variance for which an analytical formula is derived. This non-zero particle-number variance acts as a lower bound that depends in a specific way on the number of valence nucleons and on the degeneracy of the valence shell. The fact that a given nucleus does belong to one category or the other, i.e., closed-(sub)shell or open shell, in the pairing limit may depend on the self-consistent spatial symmetry assumed in the calculation. All these findings are confirmed and ...