BPS brane cosmology in N=2 supergravity
arXiv:1509.01651 · doi:10.1088/0264-9381/32/18/185014
Abstract
We study the embedding of flat BPS 3-branes in five dimensional N=2 supergravity theory. We derive the branes' dynamical equations as well as general expressions for the hypermultiplet fields then focus on a single brane and study its time evolution. It is shown that the brane's Hubble parameter correlates with the moduli of the underlying manifold's complex structure. For certain particular solutions, the moduli seem to exhibit an instability; being large valued at early times then rapidly decaying to either zero or some convergent constant value. The possibility of extending these results to the cosmology of our universe is implied and briefly discussed. Our results are in line with the production and decay of heavy moduli in the early universe, as is currently believed in the literature.
17 pages, 1 figure
References in corpus (12)
- General inflaton potentials in supergravity
- Moduli Decays and Gravitinos
- The cosmological constant and dark energy in braneworlds
- Moduli decay in the hot early Universe
- Brane inflation: A field theory approach in background supergravity
- Issues in Complex Structure Moduli Inflation
- Simple inflationary models in Gauss-Bonnet brane-world cosmology
- Symplectic covariance of the N=2 hypermultiplets
- Simple brane-world inflationary models in light of BICEP2
- Brane Cosmology for Vacuum and Cosmological Constant Bulk
- The Cosmological Constant Problem from the Point of View of String Theory
- On two string axions as inflaton