Effects of Finite Temperature and Pairing Correlations in Multi- Hypernuclei
arXiv:2403.09737 · doi:10.1103/PhysRevC.110.014329
Abstract
The influence of finite temperatures and pairing correlations on the ground state properties of multi - Ca, Sn and Pb hypernuclei is explored using finite temperature Hartree Fock Bogoliubov approach and contact pairing interaction. A critical temperature is predicted and is in agreement with the Bardeen Cooper Schrieffer relationship , beyond which pairing correlations drop to zero. Particle densities, single particle energies, and nuclear radii are weakly impacted by pairing as well as by finite temperatures. However, other nuclear properties which are more sensitive to pairing correlations, such as pairing gaps, condensation energies, and abnormal densities are also more impacted by finite temperature, especially around the critical temperature. Furthermore, calculations show the occurrence of the pairing re-entrance effect in the Pb hyperon drip line hypernucleus. Our study provides insight into the thermal evolution of pairing, i.e. the emergence and vanishing of pairing correlations in multi hypernuclei as a function of temperature.
arXiv comment10 pages, 8 figures
References in corpus (31)
- Neutrino Emission from Neutron Stars
- Strangeness in nuclear physics
- Perspectives on Core-Collapse Supernova Theory
- The equation of state for dense nucleonic matter from a metamodeling. I. Foundational aspects
- Effects of Strong and Electromagnetic Correlations on Neutrino Interactions in Dense Matter
- The explosion mechanism of core-collapse supernovae: progress in supernova theory and experiments
- Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy
- Thermal luminosities of cooling neutron stars
- Thermal Evolution of Compact Stars
- S-wave Pairing of Hyperons in Dense Matter
- Strangeness in Compact Stars
- Occurrence of Hyperon Superfluidity in Neutron Star Cores
- Observation of a Be double-Lambda hypernucleus in the J-PARC E07 experiment
- Nuclear Superfluidity and Specific Heat in the Inner Crust of Neutron Stars
- Superfluidity of hyperons in neutron stars
- A study of Lambda hypernuclei within the Skyrme-Hartree-Fock Model
- Implications of Hyperon Pairing for Cooling of Neutron Stars
- Hadron Physics at J-PARC
- Strength of pairing interaction for hyperons in multistrangeness hypernuclei
- Suppression, persistence and reentrance of superfluidity in overflowing nuclear systems
- Lambda hyperonic effect on the normal driplines
- Beyond-mean-field study of the hyperon impurity effect in hypernuclei with shape coexistence
- Density Functional approach for multi-strange hypernuclei: competition between and hyperons
- In-medium chiral SU(3) dynamics and hypernuclear structure
- Fast cooling and internal heating in hyperon stars
- pairing in multi-strange hypernuclei
- Possibility of ΛΛpairing and its dependence on background density in relativistic Hartree-Bogoliubov model
- Generalised mass formula for non-strange, strange and multiply-strange nuclear systems
- Finite temperature pairing re-entrance in drip-line Ni nucleus
- Superfluidity of hyperons in warm strange hadronic star matter
- The phase transition in hot hypernuclei within relativistic Thomas-Fermi approximation