Precise calculation of neutralino relic density in the minimal supergravity model

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We study precise calculation of neutralino relic density in the minimal supergravity model. We compare the exact formula for the thermal average of the neutralino annihilation cross section times relative velocity with the expansion formula in terms of the temperature, including all the contributions to neutralino annihilation cross section analytically. We confirm that the expansion formula fails badly near s-channel poles. We show that the expansion method causes 5-10 % error even far away from the poles.
10 pages, 4 figures, LaTeX. Talk given at 4th International Workshop on Particle Physics and the Early Universe (COSMO-2000), Cheju Island, Korea, September 4-8, 2000. Typos corrected

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