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    Entropy Production in Relativistic Binary Mixtures

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    In this paper we calculate the entropy production of a relativistic binary mixture of inert dilute gases using kinetic theory. For this purpose we use the covariant form of Boltzmann's equation which, when suitably transformed, yields a formal expression for such quantity. Its physical meaning is extracted when the distribution function is expanded in the gradients using the well-known Chapman-Enskog method. Retaining the terms to first order, consistently with Linear Irreversible Thermodynamics we show that indeed, the entropy production can be expressed as a bilinear form of products between the fluxes and their corresponding forces. The implications of this result are thoroughly discussed

    SU(6)\supsetSU(3)xSU(2) and SU(8)\supsetSU(4)xSU(2) Clebsch-Gordan coefficients

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    Tables of scalar factors are presented for 63x63 and 120x63 in SU(8)\supsetSU(4)xSU(2), and for 35x35 and 56x35 in SU(6)\supsetSU(3)xSU(2). Related tables for SU(4)\supsetSU(3)xU(1) and SU(3)\supsetSU(2)xU(1) are also provided so that the Clebsch-Gordan coefficients can be completely reconstructed. These are suitable to study meson-meson and baryon-meson within a spin-flavor symmetric scheme.Comment: 30 pages, mostly table
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