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In the present simulations, thermal fluctuations with a wave-length longer than the box size cannot be incorporated. We should remark that these modes could be effective at destroying the long-range order of the phase with slablike nuclei.
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47
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3142768613
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note
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The phase diagram for x=0.5 in Fig. 18 is slightly modified several points from Fig.1 in G. Watanabe, K. Sato, K. Yasuoka, and T. Ebisuzaki, astro-ph/0310290, to appear in "Young Neutron Stars and Their Environments" IAU Symposium 218, ASP Conference Proceedings, edited by F. Camilo and B. M. Gaensler.
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