Theoretical and observational aspects of cosmological inflation
arXiv:1506.00989
Abstract
This thesis piles up the results of five works in the field of cosmological inflation, inflationary cosmological perturbations, cosmic microwave background(CMB) and weak gravitational lensing of cosmic microwave background.
PHD thesis defended on 20/11/2014 at Jadavpur University, 124 Pages and 22 Figures. arXiv admin note: text overlap with arXiv:0906.0664, arXiv:hep-ph/0210162 by other authors
References in corpus (14)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Monodromy in the CMB: Gravity Waves and String Inflation
- Primordial fluctuations and non-Gaussianities in multi-field DBI inflation
- Non-gaussianity from the second-order cosmological perturbation
- Phenomenology of D-Brane Inflation with General Speed of Sound
- Inflationary Perturbations: the Cosmological Schwinger Effect
- A non inflationary model with scale invariant cosmological perturbations
- Analogue of cosmological particle creation in an ion trap
- Generating the Curvature Perturbation at the End of Inflation in String Theory
- A classical bounce: constraints and consequences
- Efficient Cosmological Parameter Estimation with Hamiltonian Monte Carlo
- A combined analysis of 3D Weak Lensing, Lyman-alpha forest and WMAP year three data
- Natural Inflation: the status after WMAP 3-year data
- Natural inflation at the GUT scale