$\Lambda^{\ast}(1405)$-matter: stable or unstable?
Jaroslava Hrt\'ankov\'a, Nir Barnea, Eliahu Friedman, Avraham Gal,, Ji\v{r}\'i Mare\v{s}, Martin Sch\"afer

TL;DR
This study investigates whether $\Lambda^{ ext{ast}}(1405)$-matter could be stable by using RMF calculations, finding it to be highly unstable and inconsistent with experimental absorption data.
Contribution
It provides the first comprehensive RMF analysis of $\Lambda^{ ext{ast}}(1405)$-matter stability across various interaction strengths.
Findings
Binding energy per $\Lambda^{ ext{ast}}$ saturates below 100 MeV for large A.
$\Lambda^{ ext{ast}}$ matter is unstable against decay to hyperon aggregates.
Strong $ar K N$ potentials fail to match experimental absorption fractions.
Abstract
A recent suggestion [PLB 774 (2017) 522] that purely- nuclei provide the absolute minimum energy in charge-neutral baryon matter for baryon-number , is tested within RMF calculations. A broad range of interaction strengths, commensurate with binding energy assumed to be of order 100 MeV, is scanned. It is found that the binding energy per , , saturates for with values of considerably below 100 MeV, implying that matter is highly unstable against strong decay to and hyperon aggregates. The central density of matter is found to saturate as well, at roughly twice nuclear matter density. Moreover, it is shown that the underlying very strong potentials, fitted for isospin to the mass and width…
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