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- W1994550610 abstract "In the present paper, a spinless primordial tachyon is considered in the background of Robertson–Walker (RW) cosmology. Various physical parameters, such as probability density, energy, and dissipation of energy are investigated in open, flat, and closed RW models. For this purpose, the Klein–Gordon equation, generalized to curved space-time and having a term proportional to the scalar curvature of the space-time, is solved for the spacelike scalar field ψ(t,r,θ,φ). It is speculated that if a primordial spinless tachyon survives up to the present epoch, its metamass would be less than 2.447×10−93 g." @default.
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- W1994550610 date "1984-03-01" @default.
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- W1994550610 title "On the survival of primordial tachyons up to the present epoch" @default.
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- W1994550610 doi "https://doi.org/10.1063/1.526177" @default.
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