On the relic, cosmic abundance of stable, weakly interacting massive particles

Physics

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Particle-Theory And Field-Theory Models Of The Early Universe, Background Radiations

Scientific paper

In the context of the expanding Universe, we solve the Boltzmann equation to obtain the relic abundance of a stable, weakly interacting massive particle species with arbitrary mass and interaction strength. We provide approximate analytic formulas for the evolution of the abundance and the final abundance. Our formulas are typically accurate to better than 5%.

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