39 research outputs found

    Effects of initial axion production and photon--axion oscillation on type Ia supernova dimming

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    Recently, Csaki, Kaloper and Terning (CKT) suggested that axion-photon oscillation in the intergalactic medium can explain the observed dimming of distant type Ia supernovae. This mechanism works only if the initial axion flux is much smaller than the initial photon flux. We study several mechanisms for such initial axion production. The direct axion production in the supernovae, the photon-axion oscillation in the magnetic field of supernovae and in the magnetic field of their host galaxies are addressed. We find it likely that the initial axion flux is very small and therefore does not pose a problem to the CKT mechanism.Comment: 11 pages, Revtex4. Minor modifications in the tex

    KLπ0ννˉK_L \to \pi^0 \nu \bar \nu Beyond the Standard Model

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    We analyze the decay KLπ0ννˉK_L \to \pi^0 \nu \bar \nu in a model independent way. If lepton flavor is conserved the final state is (to a good approximation) purely CP even. In that case this decay mode goes mainly through CP violating interference between mixing and decay. Consequently, a theoretically clean relation between the measured rate and electroweak parameters holds in any given model. Specifically, Γ(KLπ0ννˉ)/Γ(K+π+ννˉ)=sin2θ\Gamma(K_L \to \pi^0 \nu \bar \nu)/\Gamma(K^+ \to \pi^+ \nu \bar \nu)= \sin^2\theta (up to known isospin corrections), where θ\theta is the relative CP violating phase between the KKˉK-\bar K mixing amplitude and the sdννˉs\to d\nu\bar\nu decay amplitude. The experimental bound on BR(K+π+ννˉ)BR(K^+ \to \pi^+ \nu \bar \nu) provides a model independent upper bound: BR(KLπ0ννˉ)<1.1×108BR(K_L \to \pi^0 \nu \bar \nu) < 1.1 \times 10^{-8}. In models with lepton flavor violation, the final state is not necessarily a CP eigenstate. Then CP conserving contributions can dominate the decay rate.Comment: 12 pages, revtex, no figure
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