2003
DOI: 10.1103/physrevc.68.015801
|View full text |Cite
|
Sign up to set email alerts
|

Possibility ofΛΛpairing and its dependence on background density in a relativistic Hartree-Bogoliubov model

Abstract: We calculate a ΛΛ pairing gap in binary mixed matter of nucleons and Λ hyperons within the relativistic Hartree-Bogoliubov model. Lambda hyperons to be paired up are immersed in background nucleons in a normal state. The gap is calculated with a one-boson-exchange interaction obtained from a relativistic Lagrangian. It is found that at background density ρN = 2.5ρ0 the ΛΛ pairing gap is very small, and that denser background makes it rapidly suppressed. This result suggests a mechanism, specific to mixed matte… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

1
20
0

Year Published

2006
2006
2020
2020

Publication Types

Select...
8

Relationship

0
8

Authors

Journals

citations
Cited by 17 publications
(21 citation statements)
references
References 34 publications
1
20
0
Order By: Relevance
“…However, the superfluid hyperon gap is strongly dependent on the hyperon properties in neutron star matter and on the YY interaction (Wang & Shen 2010). In particular, it has been shown the small value of B obtained from 6 He (Takahashi et al 2001) leads to a very small gap in dense neutron matter (Tanigawa, Matsuzaki, & Chiba 2003) and in dense neutron star matter (Wang & Shen 2010) or even suppresses completely the superfluidity. Following Wang & Shen (2010), superfluidity exists in massive neutron stars only for strong interactions.…”
Section: Summary Of Constraintsmentioning
confidence: 99%
“…However, the superfluid hyperon gap is strongly dependent on the hyperon properties in neutron star matter and on the YY interaction (Wang & Shen 2010). In particular, it has been shown the small value of B obtained from 6 He (Takahashi et al 2001) leads to a very small gap in dense neutron matter (Tanigawa, Matsuzaki, & Chiba 2003) and in dense neutron star matter (Wang & Shen 2010) or even suppresses completely the superfluidity. Following Wang & Shen (2010), superfluidity exists in massive neutron stars only for strong interactions.…”
Section: Summary Of Constraintsmentioning
confidence: 99%
“…In the following, we will therefore calibrate our ΛΛ pairing interaction on hypernuclear matter pre-dictions of Ref. [23], which represents an average prediction for the maximum possible Λ pairing gap.…”
Section: B Mean Field + Pairing Approximationmentioning
confidence: 99%
“…Fermi momenta corresponding to these densities are calculated as k FΛ = ( 3π 2 2 ρ Λ ) 1/3 . The density profile of hypernuclear matter calculations [23] which has corresponding Fermi momentum and density fraction allows to extract ΛΛ pairing gap for each hypernuclei for each force sets. For finding adequate Λ pairing strength (V Λpair in Eq.…”
Section: λλ Pairing and Binding Energiesmentioning
confidence: 99%
“…15)-18) It has also been used to examine the properties of strange hadronic matter. 5), 19)- 21) The purpose of this paper is to present a self-consistent calculation of double-Λ hypernuclei in a wide range of mass number A within the framework of relativistic mean-field theory (RMF), and also to examine possible contributions of the two strange mesons σ * and φ to the ΛΛ binding energy. In principle, exact few-body calculations are more appropriate for light hypernuclei, but they are not available for heavy systems.…”
Section: §1 Introductionmentioning
confidence: 99%