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arxiv: hep-th/0406180 · v3 · submitted 2004-06-21 · ✦ hep-th · astro-ph· gr-qc· hep-ph

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Vector Perturbations in a Contracting Universe

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classification ✦ hep-th astro-phgr-qchep-ph
keywords contractingperturbationsuniversevectoraddressedartifactbangbouncing
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In this note we show that vector perturbations exhibit growing mode solutions in a contracting Universe, such as the contracting phase of the Pre Big Bang or the Cyclic/Ekpyrotic models of the Universe. This is not a gauge artifact and will in general lead to the breakdown of perturbation theory -- a severe problem that has to be addressed in any bouncing model. We also comment on the possibility of explaining, by means of primordial vector perturbations, the existence of the observed large scale magnetic fields. This is possible since they can be seeded by vorticity.

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  1. The Status of Gravitational Vector Perturbations with Recent CMB Data

    astro-ph.CO 2026-05 unverdicted novelty 4.0

    Recent CMB datasets tighten 95% CL upper bounds on vector-mode amplitude r_v to 1.3e-4 (neutrino isocurvature), 6.8 (octupole), and 4.2 (sourced) at k=0.05 Mpc^-1, with no significant detection.