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Note on the relativistic reaction rate coefficient

Author

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  • Kremer, G.M.

Abstract

The first approximation to the reaction rate coefficient is determined by considering the equilibrium Maxwell–Jüttner distribution function and relativistic reactive differential cross-sections which take into account the activation energy of the chemical reaction. It is shown how the reaction rate coefficient behaves as a function of the activation energy when the mixture evolves with respect to the ratio of the rest energy and the thermal energy of the relativistic mixture.

Suggested Citation

  • Kremer, G.M., 2007. "Note on the relativistic reaction rate coefficient," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 380(C), pages 61-65.
    • Handle: RePEc:eee:phsmap:v:380:y:2007:i:c:p:61-65
    DOI: 10.1016/j.physa.2007.03.006
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    References listed on IDEAS

    as
    1. Shizgal, Bernie D. & Chikhaoui, Aziz, 2006. "On the use temperature parameterized rate coefficients in the estimation of non-equilibrium reaction rates," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 365(2), pages 317-332.
    2. Anderson, J.L., 1976. "Variational principles for calculation of transport coefficients of relativistic multi-component systems," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 85(2), pages 287-309.
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    Cited by:

    1. Kremer, Gilberto M. & Moratto, Valdemar, 2017. "Transport coefficients for relativistic gas mixtures of hard-sphere particles," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 471(C), pages 44-58.

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