Neutron-proton pairing in Nuclear Matter
arXiv:1907.10986 · doi:10.1103/PhysRevC.99.065804
Abstract
The self-energy effect on the neutron-proton (np) pairing gap is investigated up to the third order within the framework of the extend Bruecker-Hartree-Fock (BHF) approach combined with the BCS theory. The self-energy up to the second-order contribution turns out to reduce strongly the effective energy gap, while the \emph{renormalization} term enhances it significantly. In addition, the effect of the three-body force on the np pairing gap is shown to be negligible. To connect the present results with the np pairing in finite nuclei, an effective density-dependent zero-range pairing force is established with the parameters calibrated to the microscopically calculated energy gap.
References in corpus (24)
- Pairing in nuclear systems: from neutron stars to finite nuclei
- Asymmetric Nuclear Matter from Extended Brueckner-Hartree-Fock Approach
- Overview of Neutron-Proton Pairing
- Interplay of Three-Body Interactions in the EOS of Nuclear Matter
- Screening Effects in Superfluid Nuclear and Neutron Matter within Brueckner Theory
- Thermodynamics of - condensate in asymmetric nuclear matter
- Spin-triplet pairing in large nuclei
- Isovector spin-singlet (T=1, S=0) and isoscalar spin-triplet (T=0, S=1) pairing interactions and spin-isospin response
- Dispersive effects in neutron matter superfluidity
- 3PF2 pairing in high-density neutron matter
- Screening Effects on Pairing in Neutron Matter
- Self-energy Effects in the Superfluidity of Neutron Matter
- Isospin singlet (pn) pairing and quartetting contribution to the binding energy of nuclei
- Spatially inhomogeneous condensate in asymmetric nuclear matter
- Screening of nuclear pairing in nuclear and neutron matter
- Reduction of superfluid gap by scattering
- Minimal Relativity and - Pairing in Symmetric Nuclear Matter
- Superfluidity with dressed nucleons
- Angle-dependent Gap state in Asymmetric Nuclear Matter
- Three-body force effect on off-shell mass operator and spectral functions in nuclear matter
- Medium polarization in asymmetric nuclear matter
- Medium polarization effects in 3SD1 spin-triplet pairing
- Isoscalar neutron-proton pairing and SU(4)-symmetry breaking in Gamow-Teller transitions
- FFLO state with angle dependent Gap in Asymmetric Nuclear Matter
Cited by in corpus (4)
- Nucleon momentum distributions in asymmetric nuclear matter
- Role of nucleon-nucleon correlation in transport coefficients and gravitational-wave-driven -mode instability of neutron stars
- Pairing properties of semilocal coordinate&momentum-space regularized chiral interactions
- Phase diagrams of neutron-proton superfluid in asymmetric nuclear matter