Inflationary Gravitational Waves and the Evolution of the Early Universe
arXiv:1307.3010 · doi:10.1088/1475-7516/2014/01/040
Abstract
We study the effects of various phenomena which may have happened in the early universe on the spectrum of inflationary gravitational waves. The phenomena include phase transitions, entropy productions from non-relativistic matter, the production of dark radiation, and decoupling of dark matter/radiation from thermal bath. These events can create several characteristic signatures in the inflationary gravitational wave spectrum, which may be direct probes of the history of the early universe and the nature of high-energy physics.
48 pages, 18 figures; minor corrections
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- Semianalytic Calculation of Gravitational Wave Spectrum Nonlinearly Induced from Primordial Curvature Perturbations
- Primordial gravitational waves, precisely: The role of thermodynamics in the Standard Model
- Probing the Scale of New Physics by Advanced LIGO/VIRGO
- Thermal History of the Early Universe and Primordial Gravitational Waves from Induced Scalar Perturbations
- Fingerprinting models of first-order phase transitions by the synergy between collider and gravitational-wave experiments
- Imprint of a scalar era on the primordial spectrum of gravitational waves
- Primordial gravity wave background anisotropies
- Impact of high-scale Seesaw and Leptogenesis on inflationary tensor perturbations as detectable gravitational waves
- Axion Models with High Scale Inflation
- Studying Inflation with Future Space-Based Gravitational Wave Detectors
- Freeze-in Production of Dark Matter Prior to Early Matter Domination
- Cosmological and Astrophysical Probes of Vacuum Energy
- Probing flavor violation and baryogenesis via primordial gravitational waves
- Probing PeV scale SUSY-breaking with Satellite Galaxies and Primordial Gravitational Waves
- Measuring the primordial curvature perturbations from the scalar induced gravitational waves
- Axion Dark Matter Archaeology with Primordial Gravitational Waves
- Measuring the speed of scalar induced gravitational waves from observations