Microscopic evaluation of the hypernuclear chart with ΛΛ-hyperons

preprint2015arXivOpen access

Abstract

A large number of hypernuclei, where a considerable fraction of nucleons is replaced by strange baryons, and even pure hyperonic species are expected to be bound. Though, the hypernuclear landscape remains largely unknown because of scarce constraints on the NYNY and YYYY interactions. We want to estimate the number of potentially bound hypernuclei. In order to evaluate realistic error bars within the theoretical uncertainties associated to the spherical mean-field approach, and the present information from already synthetized hypernuclei on the N−YN-Y and Y−YY-Y channels, we limit ourselves to purely ΛΛ-hypernuclei, to magic numbers of ΛΛ's (for Z ≤\leq 120 and Λ≤Λ\leq70), and to even-even-even systems. We consider a density functional approach adjusted to microscopic Bruckner-Hartree-Fock calculations, where the ΛΛΛΛ term is corrected in a phenomenological way, to reproduce present experimental constraints. The number of bound even-even-even ΛΛ-hypernuclei is estimated to 491680 ±\pm 34400. This relatively low uncertainty is due to the fact that the well constrained low density and highly unconstrained high density behavior of the energy functional turn out to be largely decoupled. Results in ΛΛ-hypernuclei appear to be almost independent of the choice for the high-density part of the ΛΛΛΛ interaction. The location of the ΛΛ-hyperdriplines is also evaluated. Significant deviations from Iron-Nickel elements can be found for ΛΛ-hypernuclei with the largest binding energy per baryon. Proton, neutron and ΛΛ-hyperon magicity evolution and triple magic ΛΛ-hypernuclei are studied. Possible bubbles and haloes effect in ΛΛ-hypernuclei are also discussed.

Explore this paper’s authors, topics and related work.

Building this map preview

BZPEER is loading the nearby papers, people, topics and institutions for this page.

Reviews 0

Write a reviewWrite

No reviews yet.

Discussion 0

Add a commentWrite

No comments yet.