Abstract
The axion is a motivated cold dark matter candidate, which it would be
interesting to distinguish from weakly interacting massive particles. Sikivie
has suggested that axions could behave differently during non-linear galaxy
evolution, if they form a bose einstein condensate. Using classical equations
of motion during linear structure formation, we explore whether "gravitational
thermalisation" can drive axions to a bose einstein condensate. At linear order
in G_N, we interpret that the principle activities of gravity are to expand the
Universe and grow density fluctuations. From the anisotropic stress, we
estimate a short dissipation scale for axions which does not confirm previous
estimates of their gravitational thermalisation rate.
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