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• W2016885246 abstract "Using the O(3,2)-symmetric de Sitter solution of Einstein's equation describing a stongly interacting tensor field we show that hadronic bags confining quarks can be represented as de Sitter microuniverses with radii given by $frac{1}{{R}^{2}}=frac{ensuremath{lambda}{ensuremath{kappa}}^{2}}{6}$. Here ${ensuremath{kappa}}^{2}$ and $ensuremath{lambda}$ are the strong-coupling and the cosmological constants which appear in the Einstein equation used. Surprisingly the energy spectrum for the two-body hadronic states is essentially the same as that for a harmonic-oscillator potential, though the wave functions are completely different. The Einstein equation can be extended to include color for the tensor fields." @default.
• W2016885246 created "2016-06-24" @default.
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• W2016885246 date "1978-12-15" @default.
• W2016885246 modified "2023-10-18" @default.
• W2016885246 title "Confinement through tensor gauge fields" @default.
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• W2016885246 doi "https://doi.org/10.1103/physrevd.18.4596" @default.
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