Abstract
We study a mechanism for the energy loss in the core of a star via the Compton-like process γe → φ r ∗ e with the virtual Higgs boson φ r ∗ turning into a pair of Goldstone bosons JJ that carry away the thermonuclear energy. An astrophysical constaints upon the coupling is derived. The bound is loose enough that the decay mode H → JJ can well be the dominating channel in the hidden Higgs models.
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