kodama
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mfb said:See post #26.
The BaBar publication is here. The actual fit to the electron spectrum starts at 15 MeV. You need some sidebands for the region where your main analysis starts. That means they do not set proper upper limits in the range of 15 to 20 MeV, but a peak there would have been noted.
Oh well, the usual approach. "Our model is excluded!" "Quick, tune the couplings down so experiments need more data to exclude it!"
still it does give quantitative predictions, and specific numbers.
btw any thoughts on this, would barbar or ep colliders produce this?
A light particle solution to the cosmic lithium problem
Andreas Goudelis, Maxim Pospelov, Josef Pradler
(Submitted on 29 Oct 2015 (v1), last revised 24 May 2016 (this version, v2))
We point out that the cosmological abundance of 7Li can be reduced down to observed values if during its formation Big Bang Nucleosynthesis is modified by the presence of light electrically neutral particles X that have substantial interactions with nucleons. We find that the lithium problem can be solved without affecting the precisely measured abundances of deuterium and helium if the following conditions are satisfied: the mass and lifetimes of such particles are bounded by 1.6MeV≤mX≤20MeV and few100s≲τX≲104s, and the abundance times the absorption cross section by either deuterium or 7Be are comparable to the Hubble rate, nXσabsv∼H, at the time of 7Be formation. We include X-initiated reactions into the primordial nucleosynthesis framework, observe that it leads to a substantial reduction of the freeze-out abundances of 7Li+7Be, and find specific model realizations of this scenario. Concentrating on the axion-like-particle case, X=a, we show that all these conditions can be satisifed if the coupling to d-quarks is in the range of f−1d∼TeV−1, which can be probed at intensity frontier experiments.
Comments: 5 pages, 4 figures; v2: minor improvements, matches published version
Subjects: High Energy Physics - Phenomenology (hep-ph); Cosmology and Nongalactic Astrophysics (astro-ph.CO); Nuclear Theory (nucl-th)
Journal reference: Phys. Rev. Lett. 116, 211303 (2016)
DOI: http://arxiv.org/ct?url=http%3A%2F%2Fdx.doi.org%2F10%252E1103%2FPhysRevLett%252E116%252E211303&v=08290ee6
Cite as: arXiv:1510.08858 [hep-ph]
(or arXiv:1510.08858v2 [hep-ph] for this version)
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