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Supernova bounds on Weinberg’s Goldstone bosons
journal contribution
posted on 2016-01-20, 00:00 authored by W-Y. Keung, K-W. Ng, H. Tu, T-C. YuanRecently, Weinberg proposed a scenario where Goldstone bosons may be masquerading as fractional
cosmic neutrinos. We calculate the energy loss rates through the emission of these Goldstone bosons in a
postcollapse supernova core. Invoking the well-established emissivity bound from the Supernova 1987A
observations and simulations, we find that nuclear bremsstrahlung processes can notably impose a bound
on the Goldstone boson coupling to the Standard Model Higgs, g, dependent on the mass of the associated
radial field, mr. We apply the supernova emissivity bound at typical core conditions: a density of
ρ ¼ 3 × 1014 g=cm3 and a temperature T ¼ 30 MeV. Even in the conservative limit where mr is large
enough compared with the Goldstone boson energies attainable at this temperature, our bound
jgj ≲ 0.011ðmr=500 MeVÞ2 is very competitive to those derived from current and projected sensitivities
of collider experiments.
Funding
This work was supported in part by the National Science Council, Taiwan, ROC, under the NSC Grants No. 101- 2112-M-001-010-MY3 (K. W. N., H. T.), No. 101-2112- M-001-005-MY3 (T. C. Y.), and in part by the U.S. Department of Energy under Grant No. DE-FG02- 12ER41811 (W. Y. K.).
History
Publisher Statement
This is the copy of an article published in the Physical Review D © 2014 American Physical Society Publications.Publisher
American Physical Societyissn
1550-7998Issue date
2014-10-16Usage metrics
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