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    Spin Polarized versus Chiral Condensate in Quark Matter at Finite Temperature and Density

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    It is shown that the spin polarized condensate appears in quark matter at high baryon density and low temperature due to the tensor-type four-point interaction in the Nambu-Jona-Lasinio-type model as a low energy effective theory of quantum chromodynamics. It is indicated within this low energy effective model that the chiral symmetry is broken again by the spin polarized condensate as increasing the quark number density, while the chiral symmetry restoration occurs in which the chiral condensate disappears at a certain density.Comment: 25 pages, 9 figure

    The X-ray CCD camera of the MAXI Experiment on the ISS/JEM

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    MAXI, Monitor of All-sky X-ray Image, is the X-ray observatory on the Japanese experimental module (JEM) Exposed Facility (EF) on the International Space Station (ISS). MAXI is a slit scanning camera which consists of two kinds of X-ray detectors: one is a one-dimensional position-sensitive proportional counter with a total area of ∼5000cm2\sim 5000 cm^2, the Gas Slit Camera (GSC), and the other is an X-ray CCD array with a total area ∼200cm2\sim 200 cm^2, the Solid-state Slit Camera (SSC). The GSC subtends a field of view with an angular dimension of 1∘×180∘^\circ\times 180^\circ while the SSC subtends a field of view with an angular dimension of 1∘^\circ times a little less than 180∘^\circ. In the course of one station orbit, MAXI can scan almost the entire sky with a precision of 1∘^\circ and with an X-ray energy range of 0.5-30 keV. We have developed the engineering model of CCD chips and the analogue electronics for the SSC. The energy resolution of EM CCD for Mn Kα\alpha has a full-width at half maximum of ≃\simeq 182 eV. Readout noise is ≃\simeq 11 e^- rms.Comment: 10 pages, 4 figures Accepted for Nuclear Instruments and Method in Physics Researc
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