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Dirac spinors in an inhomogeneous cosmological model

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Abstract

Solutions of the Dirac equation in the Senovilla inhomogeneous cosmological model, which is free of a big-bang singularity, are presented. It is found that the energy density of the spinors is initially zero, but attains a maximum at some time and then decreases.

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Srivastava, S.K., Sinha, K.P. Dirac spinors in an inhomogeneous cosmological model. Int J Theor Phys 32, 1005–1011 (1993). https://doi.org/10.1007/BF01215306

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  • DOI: https://doi.org/10.1007/BF01215306

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