Cosmic String Production Towards the End of Brane Inflation
arXiv:hep-th/0204074 · doi:10.1016/S0370-2693(02)01824-5
Abstract
Towards the end of the brane inflationary epoch in the brane world, cosmic strings (but not texture, domain walls or monopoles) are copiously produced during brane collision. These cosmic strings are D-branes with dimensions compactified. We elaborate on this prediction of the superstring theory description of the brane world. Using the data on the temperature anisotropy in the cosmic microwave background, we estimate the cosmic string tension to be around . This in turn implies that the anisotropy in the cosmic microwave background comes mostly from inflation, but with a component (of order 10%) from cosmic strings. This cosmic string effect should also be observable in gravitational wave detectors and maybe even pulsar timing measurements. Keywords : Inflation, Brane World, Superstring Theory, Cosmic String, Cosmology
12 pages, 2 figures
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- The constraints on the stochastic gravitational wave background from cosmic strings by an electromagnetic resonance system
- CMB ISW-lensing bispectrum from cosmic strings
- Imprints of cosmic strings on the cosmological gravitational wave background
- Electromagnetic back-reaction from currents on a straight string
- Super Jackstraws and Super Waterwheels
- Relativistic Dynamics of Multi-BPS D-vortices and Straight BPS D-strings
- Search for a Gravitational-Wave Background from Sound Speed Resonance from Advanced LIGO and Advanced Virgo's First Three Observing Runs
- Tackling tangledness of cosmic strings by knot polynomial topological invariants
- Non-Relativistic Strings in Expanding Spacetime
- Cosmic Strings-induced CMB anisotropies in light of Weighted Morphology
- Cosmological Perturbations in Inflationary Models with Anisotropic Space-Time Scaling in Lifshitz Background
- Modelling Cosmic Springs with Finsler and Generalised Finsler Geometries
- Modeling the Beam of Gravitational Radiation from a Cosmic String Loop
- Effects of Nontrivial Topology on Neutron Star Rotation and its Potential Observational Implications
- Iso-curvature fluctuations through axion trapping by cosmic string wakes
- p-q-superstrings in Anti-de-Sitter space-time
- Bogomol'nyi equations for Dirac-Born-Infeld cosmic string
- Percolating Cosmic String loops from evaporating primordial black holes
- Cosmological stretching of perturbations on a cosmic string
- Constraints on typical relic gravitational waves based on data of LIGO
- Sir Thomas Walter Bannerman Kibble CBE
- Magnetic field in vacuum of quantum spinor matter induced by a cosmic string in three-dimensional space
- Constraining the gravitational-wave emission of core-collapse supernovae with ground-based detectors
- Vacuum polarization by topological defects in de Sitter spacetime
- Applicability of multi-component study on Bayesian searches for targeted anisotropic stochastic gravitational-wave background