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The Structure and the Density of a Bare Quark Star in a Cold Genesis Theory of Particles

DOI: 10.4236/jhepgc.2024.104108, PP. 1933-1980

Keywords: Quark Star, Cold Genesis, Current Quark Density, Preons Model, Preon Star, Black Hole

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Abstract:

Based on the preonic structure of quarks obtained in a Cold genesis theory of particles (CGT), it was obtained a semi-empiric relation for the current mass of quarks specific to CGT but with the constants obtained with the aid of the Gell-Mann-Oakes-Renner formula, giving values close to those obtained by the Standard Model, the current quark’s volume at ordinary nuclear temperature being obtained as sum of theoretic apparent volumes of preonic kerneloids. The maximal densities of the current quarks: strange (s), charm (c), bottom (b), and top (t) resulted in the range (0.8 - 4.2) × 1018 kg/m3, as values which could be specific to possible quark stars, in concordance with previous results. By the preonic quark model of CGT, the possible structure of a quark star resulted from the intermediary transforming: N e ( 2d+u )→ s ？ ˉ + λ ？ and the forming of composite quarks with the structure: C？(λ？- s ？ ˉ -λ？) and C+( s ？ ˉ -λ？- s ？ ˉ ), and of Sq-layers: C+C？C+ and C？C+C？ which can form composite quarks: H q ±

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