25 research outputs found

    Local Void vs Dark Energy: Confrontation with WMAP and Type Ia Supernovae

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    It is now a known fact that if we happen to be living in the middle of a large underdense region, then we will observe an "apparent acceleration", even when any form of dark energy is absent. In this paper, we present a "Minimal Void" scenario, i.e. a "void" with minimal underdensity contrast (of about -0.4) and radius (~ 200-250 Mpc/h) that can, not only explain the supernovae data, but also be consistent with the 3-yr WMAP data. We also discuss consistency of our model with various other measurements such as Big Bang Nucleosynthesis, Baryon Acoustic Oscillations and local measurements of the Hubble parameter, and also point out possible observable signatures.Comment: Minor numerical errors and typos corrected, references adde

    Response to "Comments on factors that impact the implementation of a systems development methodology"

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    Back-up report diffusive tube method for benzene (MDHS 50)

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    SIGLEAvailable from British Library Lending Division - LD:4274.84718(IR/L/AO--85/12) / BLDSC - British Library Document Supply CentreGBUnited Kingdo
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