Charge Asymmetry in the Brane World and Formation of Charged Black Holes
arXiv:hep-ph/0203010 · doi:10.1103/PhysRevD.67.087702
Abstract
In theories with an infinite extra dimension, free particles localized on the brane can leak out to the extra space. We argue that if there were color confinement in the bulk, electrons would be more able to escape than quarks and than protons (which are composed states). Thus, this process generates an electric charge asymmetry on brane matter densities. A primordial charge asymmetry during Big Bang Nucleosynthesis era is predicted. We use current bounds on this and on electron disappearance to constrain the parameter space of these models. Although the generated asymmetry is generically small, it could be particularly enhanced on large densities as in astrophysical objects, like massive stars. We suggest the possibility that such accumulation of charge may be linked, upon supernova collapse, to the formation of a charged Black Hole and the generation of Gamma-Ray Bursts.
Four pages, one figure. Minor changes, conclusions remain
References in corpus (2)
Cited by in corpus (18)
- Electrically charged compact stars and formation of charged black holes
- Nonadiabatic charged spherical gravitational collapse
- Gravitational lensing by Einstein-Born-Infeld black holes
- Relativistic Structure, Stability and Gravitational Collapse of Charged Neutron Stars
- Gravitational lensing and frame dragging of light in the Kerr-Newman and the Kerr-Newman-(anti) de Sitter black hole spacetimes
- Radiating Shear-Free Gravitational Collapse with Charge
- Constraints on the Electrical Charge Asymmetry of the Universe
- Gravitational redshift/blueshift of light emitted by geodesic test particles, frame-dragging and pericentre-shift effects, in the Kerr-Newman-de Sitter and Kerr-Newman black hole geometries
- Complementary Constraints on Brane Cosmology
- Probing spacetime noncommutative constant via charged astrophysical black hole lensing
- Spherically symmetric models for charged radiating stars and voids: Theoretical approach
- Numeric simulation of relativistic stellar core collapse and the formation of Reissner-Nordstrom space-times
- Nonadiabatic charged spherical evolution in the postquasistatic approximation
- Collapse of spherical charged anisotropic fluid spacetimes
- Photon emission of extremal Kerr-Newman black holes
- A class of charged-Taub-NUT-scalar metrics via Harison and Ehlers Transformations
- LHC signatures of vector boson emission from brane to bulk
- Cracking in charged relativistic spheres