Abstract

We study the degenerates into the candidates for da rk matter and dark energy from ur-Higgs bosons which has appeared as a mother for SM Higgs boson above. It is shown that only about a tenth of them (ur-Higgs) can be transformed to the Higgs boson with corrected mass by γ- irradiation from surroundings, which is in electrow eak interaction with particles. The remainder degenerate into the hybrid molecules of a glueball and pseudo-scalar mesons (candidate of dark matter); and into the quasi-crystals of fullerene c onsists of σ mesons and some ω mesons (candidate of dark energy) which will raise repulsi ve strong force as soon as the (free) fullerenes approach very near each other. Where we regard the developed fullerene as a finite nucleus of the limit of N(p, n) → 0, namely, m(p, n) → 0 in Dirac equation of mean-field theory. And large amount of condensing (latent) heat from (tt_bar)* g as to the liquid (Higgs boson) might be considered as at last transformed to dark energy, b y which the quasi-crystal above would be annealed (or sublimated) to more developed fulleren e. Then the content ratio between matter (atom), dark matter and dark energy is consistent w ith the latest result of WMAP (9 Years). It is interesting that if we choose reciprocal of the fin e structure constant (1/α) as a mass contributing factor (number) of gluon in QGP for matter, the con tent ratio is completely in accordance with WMAP. Also our mass of dark matter (considered at a round 120.611 GeV/c 2 ) seems relevant to the result of Fermi-LAT.

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