Bose-Einstein condensation in helium white dwarf stars. I

Physics

Scientific paper

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Scientific paper

The formation of a Bose-Einstein condensate in the interior of
helium white dwarfs stars is discussed. Following the proposal made by
Gabadadze and Rosen, we have explored the consequences of such a
mechanism by calculating the cooling time of the stars. We have found
that it is shorter than the value predicted by the standard model.

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