Abstract
We discuss the cosmological implications of an antisymmetric tensor field when it experiences a kind of "Higgs mechanism," including nonlocal interaction terms, on D-branes. Even when a huge magnetic-condensation-inducing anisotropy is assumed in the early universe, the expansion of the universe leads to an Isotropic B-matter-dominated universe.
| Original language | English |
|---|---|
| Pages (from-to) | 779-786 |
| Number of pages | 8 |
| Journal | Journal of the Korean Physical Society |
| Volume | 49 |
| Issue number | 2 I |
| State | Published - Aug 2006 |
Keywords
- Antisymmteric tensor field
- Cosmology
- D-brane