Theory of a density-wave instability in symmetric nuclear matter

2001 ◽  
Vol 64 (1) ◽  
Author(s):  
A. E. Pozamantir ◽  
A. W. Overhauser
2009 ◽  
Vol 87 (3) ◽  
pp. 271-277 ◽  
Author(s):  
Moshe Rozali ◽  
Lionel Brits

We review the Sakai–Sugimoto model of holographic QCD at zero temperature and finite chemical potential, comparing the results to those expected at large-Nc QCD, and those in a closely related holographic model. We find that as the baryon chemical potential is increased above a critical value, there is a phase transition to a nuclear matter phase, the details of which depend on the model. We argue that the nuclear matter phase is necessarily inhomogeneous to arbitrarily high density, which suggests an explanation of the “chiral density wave” instability of the quark Fermi surface in large-Nc QCD. Some details of the instanton distribution in the holographic dual are reminiscent of a Fermi surface. This short manuscript summarizes a talk given by M.R. at Theory CANADA 4 conference and is based largely (but not entirely) on the results of (Rozali et al. JHEP. 53, 01 (2008)).


2021 ◽  
Vol 321 ◽  
pp. 04004
Author(s):  
Santosh Kumar Rai ◽  
Neha Ahlawat ◽  
Pardeep Kumar ◽  
Vinay Panwar

In present paper, a mathematical model based on the one dimensional nonlinear mass, momentum and energy conservation equations has been developed to study the density wave instability (DWI) in horizontal heater and horizontal cooler supercritical water natural circulation loop (HHHC-SCWNCL). The one dimensional nonlinear mass, momentum and energy conservation equations are discretized by using finite difference method (FDM). The numerical model is validated with the benchmark results (NOLSTA model). Numerical simulations are performed to find the threshold stability zone (TSZ) and draw the stability map for natural circulation loop. Further, effect of change in diameter and riser height on the density wave instability of SCWNCL has been investigated.


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.


1981 ◽  
Vol 301 (2) ◽  
pp. 125-132 ◽  
Author(s):  
H. Ui ◽  
Y. Kawazoe
Keyword(s):  

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