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On the Cosmology of Massive Vector Fields with SO(3) Global Symmetry
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On the Cosmology of Massive Vector Fields with SO(3) Global Symmetry
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Forward citations
Cited by 4 Pith papers
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Misalignment production of isotropized vector dark matter?
Kinetic-coupling misalignment of an isotropized multi-vector condensate cannot produce dark matter: non-Gaussianity and isocurvature constraints exclude the viable parameter space in both weak- and strong-mixing regimes.
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Misalignment production of isotropized vector dark matter?
Isotropized multi-vector misalignment dark matter from kinetic coupling is excluded because non-Gaussianity and isocurvature bounds require incompatible mixing strengths.
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Inflation with vector fields revisited: non-Gaussianities
In kinetically coupled vector inflation, the bispectrum in the large-h regime exhibits competing local and flattened non-Gaussian signals with distinct h scalings that distinguish vector-supported dynamics.
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Cosmological implications of Bumblebee theory on an FLRW background
Bumblebee theory on an FLRW background yields a cosmological model whose single free parameter is fitted to supernovae observations, producing deceleration and dark energy behaviors that are compared to Lambda-CDM.
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