Neutron-proton pairing in symmetric nuclear matter

1990 ◽  
Vol 337 (3) ◽  
pp. 355-356 ◽  
Author(s):  
Th. Alm ◽  
G. R�pke ◽  
M. Schmidt
2019 ◽  
Vol 28 (05) ◽  
pp. 1950034
Author(s):  
Prafulla K. Panda ◽  
Constança Providência ◽  
Steven A. Moszkowski ◽  
Henrik Bohr ◽  
João da Providência

We generalize the Bogoliubov quark-meson coupling (QMC) model to also include hyperons. The hyperon-[Formula: see text]-meson couplings are fixed by the model and the hyperon-[Formula: see text]-meson couplings are fitted to the hyperon potentials in symmetric nuclear matter. The present model predicts neutron stars with masses above 2[Formula: see text] and the radius of a 1.4[Formula: see text] star [Formula: see text]14[Formula: see text]km. In the most massive stars, bags overlap at the core of the star, and this may be interpreted as a transition to deconfined quark matter.


1991 ◽  
Vol 17 (6) ◽  
pp. 887-900 ◽  
Author(s):  
T Shamsunnahar ◽  
S Saha ◽  
K Kabir ◽  
L M Nath

1980 ◽  
Vol 63 (5) ◽  
pp. 1665-1687 ◽  
Author(s):  
T. Matsui ◽  
T. Otofuji ◽  
K. Sakai ◽  
M. Yasuno

1996 ◽  
Vol 597 (1) ◽  
pp. 1-18 ◽  
Author(s):  
E.S. Hernández ◽  
J. Navarro ◽  
A. Polls ◽  
J. Ventura

2000 ◽  
Vol 15 (24) ◽  
pp. 1529-1537 ◽  
Author(s):  
J. C. T. DE OLIVEIRA ◽  
M. KYOTOKU ◽  
M. CHIAPPARINI ◽  
H. RODRIGUES ◽  
S. B. DUARTE

In the context of a relativistic mean field theory the delta-resonance matter formation in a highly compressed nuclear medium is investigated. For a given set of nucleon–meson coupling constants, the delta-resonance formation is studied by changing the delta-meson coupling constants. The effect on the equation of state and on the delta-resonance population with respect to changes in the delta-resonance coupling constants values is discussed for very asymmetric and quasi-symmetric nuclear matter, as an extension of works restricted to the symmetric nuclear matter treatment.5,6


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