| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8193979 | Physics Letters B | 2010 | 4 Pages |
Abstract
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.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
M.E. Mosquera, O. Civitarese, O.G. Benvenuto, M.A. De Vito,