pith. sign in

arxiv: 2002.09223 · v1 · pith:YVVSAPCEnew · submitted 2020-02-21 · ⚛️ nucl-ex · hep-ex· hep-ph· nucl-th

Strangeness in Nuclei and Neutron Stars

classification ⚛️ nucl-ex hep-exhep-phnucl-th
keywords matterstrangenessdenseneutronnuclearstarsanalysiscollisions
0
0 comments X
read the original abstract

We review the present status of the experimental and theoretical developments in the field of strangeness in nuclei and neutron stars. We start by discussing the $\bar K N$ interaction, that is governed by the presence of the $\Lambda(1405)$. We continue by showing the two-pole nature of the $\Lambda(1405)$, and the production mechanisms in photon-, pion-, kaon-induced reactions as well as proton-proton collisions, while discussing the formation of $\bar K NN$ bound states. We then move to the theoretical and experimental analysis of the properties of kaons and antikaons in dense nuclear matter, paying a special attention to kaonic atoms and the analysis of strangeness creation and propagation in nuclear collisions. Next, we examine the $\phi$ meson and the advances in photoproduction, proton-induced and pion-induced reactions, so as to understand its properties in dense matter. Finally, we address the dynamics of hyperons with nucleons and nuclear matter, and the connection to the phases of dense matter with strangeness in the interior of neutron stars.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 9 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Cooling of Hybrid Stars with a 2SC+$<dd>$ Phase

    nucl-th 2026-06 unverdicted novelty 7.0

    Hybrid stars containing the 2SC+<dd> phase cool more slowly than those with the 2SC phase because inherited 3P2 superfluidity suppresses quark beta decay, producing cooling curves close to the CFL case.

  2. Symmetry Energy Expansion with Strange Dense Matter

    nucl-th 2025-04 unverdicted novelty 7.0

    A redefinition of the symmetry energy expansion that incorporates finite strangeness consistent with SU(3) flavor symmetry and remains valid beyond typical neutron-star central densities.

  3. $\Lambda$ hyperons in core-collapse supernovae: Equilibration and neutrino opacities

    hep-ph 2026-07 unverdicted novelty 6.0

    Lambda hyperons equilibrate rapidly in post-collapse proto-neutron stars through nonleptonic NN to N Lambda processes and enhance low-energy muon neutrino opacities beyond nucleonic contributions.

  4. Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis

    nucl-th 2026-06 unverdicted novelty 6.0

    Bayesian analysis of astrophysical and laboratory data favors the two-families scenario of coexisting hadronic and strange quark stars over the one-family scenario.

  5. Collision Energy Dependence of Hypertriton Production in Au+Au Collisions at RHIC

    nucl-ex 2026-04 unverdicted novelty 6.0

    Hypertriton yields and Lambda ratios increase at lower collision energies but remain a factor of two below thermal models, while the double ratio to triton production stays constant at 0.4, pointing to intrinsically l...

  6. Wave-Function Femtometry: Hypertriton - The Ultimate Halo Nucleus

    nucl-ex 2026-04 unverdicted novelty 5.0

    Hypertriton production yield in LHC pp collisions, described by nuclear coalescence, confirms its halo structure with a Lambda separation of 9.54 fm from the deuteron core.

  7. A quarkyonic matter model

    hep-ph 2026-05 unverdicted novelty 4.0

    The IdylliQ model uses quark saturation to generate stiff equations of state and effective baryon repulsions that mitigate hyperon softening in neutron star matter.

  8. Impact of hyperon mixing on neutron star structure based on Skyrme-type equations of state: Systematic analysis of $\Lambda NN$ and $\Lambda\Lambda N$ three-body forces with Bayesisan inference

    nucl-th 2026-05 unverdicted novelty 4.0

    Systematic scan of ΛNN and ΛΛN three-body force parameters in Skyrme EDF for beta-equilibrated hyperonic matter, TOV branch classification, and Bayesian analysis with XGBoost-SHAP on NS mass-radius constraints.

  9. Cooling of Isolated Neutron Stars with Hyperon-mixed Kaon-Condensation Matter

    astro-ph.HE 2026-05 unverdicted novelty 4.0

    Strong proton superconductivity at high densities shuts down nucleon and hyperon direct Urca cooling, making kaon-induced Urca processes dominant and explaining cold massive neutron stars.