6,466 research outputs found

    Unified TeV Scale Picture of Baryogenesis and Dark Matter

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    We present a simple extension of MSSM which provides a unified picture of cosmological baryon asymmetry and dark matter. Our model introduces a gauge singlet field NN and a color triplet field XX which couple to the right--handed quark fields. The out--of equilibrium decay of the Majorana fermion NN mediated by the exchange of the scalar field XX generates adequate baryon asymmetry for MN∼100M_N \sim 100 GeV and MX∼M_X \sim TeV. The scalar partner of NN (denoted N~1\tilde{N}_1) is naturally the lightest SUSY particle as it has no gauge interactions and plays the role of dark matter. N~1\tilde{N}_1 annihilates into quarks efficiently in the early universe via the exchange of the fermionic X~\tilde{X} field. The model is experimentally testable in (i) neutron--antineutron oscillations with a transition time estimated to be around 101010^{10} sec, (ii) discovery of colored particles XX at LHC with mass of order TeV, and (iii) direct dark matter detection with a predicted cross section in the observable range.Comment: 10 pages, one reference updated. Version to appear in Phys. Rev. Let

    A Theory of R(D∗,D)R(D^*,D) Anomaly With Right-Handed Currents

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    We present an ultraviolet complete theory for the R(D∗)R(D^*) and R(D)R(D) anomaly in terms of a low mass WR±W_R^\pm gauge boson of a class of left-right symmetric models. These models, which are based on the gauge symmetry SU(3)c×SU(2)L×SU(2)R×U(1)B−LSU(3)_c \times SU(2)_L \times SU(2)_R \times U(1)_{B-L}, utilize vector-like fermions to generate quark and lepton masses via a universal seesaw mechanism. A parity symmetric version as well as an asymmetric version are studied. A light sterile neutrino emerges naturally in this setup, which allows for new decay modes of BB-meson via right-handed currents. We show that these models can explain R(D∗)R(D^*) and R(D)R(D) anomaly while being consistent with LHC and LEP data as well as low energy flavor constraints arising from KL−KS,Bd,s−Bˉd,sK_L-K_S, B_{d,s}-\bar{B}_{d,s}, D−DˉD-\bar{D} mixing, etc., but only for a limited range of the WRW_R mass: 1.2 (1.8) TeV≤MWR≤3 TeV1.2\, (1.8)~{\rm TeV} \leq M_{W_R}\leq 3~ {\rm TeV} for parity asymmetric (symmetric) Yukawa sectors. The light sterile neutrinos predicted by the model may be relevant for explaining the MiniBoone and LSND neutrino oscillation results. The parity symmetric version of the model provides a simple solution to the strong CP problem without relying on the axion. It also predicts an isospin singlet top partner with a mass MT=(1.5−2.5)M_T = (1.5-2.5) TeV.Comment: 43 pages, 7 figures, references added, model slightly modifie
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