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Nucleosynthesis constraints on the faint vector portal

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arxiv 1501.00459 v1 pith:6PAK4IEY submitted 2015-01-02 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords vectorconstraintskappalesssimmixingnucleosynthesisportalabelian
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

New Abelian U(1)' gauge bosons $V_{\mu}$ can couple to the Standard Model through mixing of the associated field strength tensor $V_{\mu\nu}$ with the one from hypercharge, $F_{\mu\nu}^Y$. Here we consider early Universe sensitivity to this vector portal and show that the effective mixing parameter with the photon, $\kappa$, is being probed for vector masses in the GeV ballpark down to values $10^{-10} \lesssim \kappa \lesssim 10^{-14}$ where no terrestrial probes exist. The ensuing constraints are based on a detailed calculation of the vector relic abundance and an in-depth analysis of relevant nucleosynthesis processes.

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