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arxiv: 0712.1523 · v3 · submitted 2007-12-10 · ✦ hep-ph · astro-ph· hep-th

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Hypermagnetic Baryogenesis

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classification ✦ hep-ph astro-phhep-th
keywords hypermagneticbaryogenesisbaryonbaryonshelicityscalesphaleronamplitude
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We study a new scenario for baryogenesis due to the spontaneous breaking of the $CPT$ invariance through the interaction between a baryon current and a hypermagnetic helicity. The hypermagnetic helicity (Chern-Simons number) of $U(1)_Y$ provides a $CPT$ violation background for the generation of baryons via sphaleron processes, which protects these baryons from the sphaleron wash-out effect in thermal equilibrium. It is shown that if the present amplitude of the resultant magnetic fields are sufficiently large, for a wide range mass scale (from TeV to the Planck scale), the observational magnitude of the baryon asymmetry of the Universe can be realized.

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