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    Effects of density-dependent quark mass on phase diagram of three-flavor quark matter

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    Considering the density dependence of quark mass, we investigate the phase transition between the (unpaired) strange quark matter and the color-flavor-locked matter, which are supposed to be two candidates for the ground state of strongly interacting matter. We find that if the current mass of strange quark msm_s is small, the strange quark matter remains stable unless the baryon density is very high. If msm_s is large, the phase transition from the strange quark matter to the color-flavor-locked matter in particular to its gapless phase is found to be different from the results predicted by previous works. A complicated phase diagram of three-flavor quark matter is presented, in which the color-flavor-locked phase region is suppressed for moderate densities.Comment: 4 figure

    Instability of the solitary waves for the generalized Boussinesq equations

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    In this work, we consider the following generalized Boussinesq equation \begin{align*} \partial_{t}^2u-\partial_{x}^2u+\partial_{x}^2(\partial_{x}^2u+|u|^{p}u)=0,\qquad (t,x)\in\mathbb R\times \mathbb R, \end{align*} with 0<p<0<p<\infty. This equation has the traveling wave solutions ϕω(xωt)\phi_\omega(x-\omega t), with the frequency ω(1,1)\omega\in (-1,1) and ϕω\phi_\omega satisfying \begin{align*} -\partial_{xx}{\phi}_{\omega}+(1-{\omega^2}){\phi}_{\omega}-{\phi}_{\omega}^{p+1}=0. \end{align*} Bona and Sachs (1988) proved that the traveling wave ϕω(xωt)\phi_\omega(x-\omega t) is orbitally stable when 0<p<4,0<p<4, p4<ω2<1\frac p4<\omega^2<1. Liu (1993) proved the orbital instability under the conditions 0<p<4,0<p<4, ω2<p4\omega^2<\frac p4 or p4,p\ge 4, ω2<1\omega^2<1. In this paper, we prove the orbital instability in the degenerate case 0<p<4,ω2=p40<p<4,\omega^2=\frac p4 .Comment: 29 page
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