Comparing the Cosmological Critical Density of Neutralinos and Cold Dark Matter

Mathematics – Logic

Scientific paper

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Scientific paper

Cosmological surveys conducted in the last decade have placed substantial constraints upon the cold dark matter (CDM) component of the universe. These surveys include NASA’s Wilkinson Microwave Anisotropy Probe and the Sloan Digital Sky Survey, which is exhaustively mapping the positions of clusters of galaxies out to >4 billion light years. These results place the CDM cosmological density in the range of 0.087 < ΩCDM h2 < 0.138 at the 99% confidence level. An ideal candidate for the CDM is the lowest mass, weakly interacting, neutral, long lived, suspersymmetric particle known as the neutralino, χ. As long as the neutralino conserves R parity exactly it will be stable. Here we examine the sensitivity of the neutralino cross section in a range of minimal supersymmetric models using the DarkSUSY algorithm. We do this under the constraint that the cosmological WIMP CDM contribution to the mass-energy density scales as Ωχh2 ≈ 1/<σv>, where the cross section, σ, is a calculable parameter in the DarkSUSY code, v is the relative velocity of the neutralino and the cross section target and < > indicates thermal averaging. We compare these neutralino densities to the observed CDM density to constrain the model parameter space. We gratefully acknowledge the Kentucky Space Grant Consortium and NASA for supporting this research.

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