A new gravitational wave background from the Big Bang
Juan Garcia-Bellido, Daniel G. Figueroa

TL;DR
This paper models the generation of a stochastic gravitational wave background during the universe's reheating phase after hybrid inflation, highlighting potential detectability and implications for early universe physics.
Contribution
It introduces a detailed mechanism for gravitational wave production during reheating, including bubble collisions and turbulence, and assesses their detectability across different inflation scales.
Findings
Significant gravitational wave energy density possible at GUT scales
Low-scale models may produce detectable signals for BBO or DECIGO
Similar results obtained for chaotic inflation models
Abstract
The reheating of the universe after hybrid inflation proceeds through the nucleation and subsequent collision of large concentrations of energy density in the form of bubble-like structures moving at relativistic speeds. This generates a significant fraction of energy in the form of a stochastic background of gravitational waves, whose time evolution is determined by the successive stages of reheating: First, tachyonic preheating makes the amplitude of gravity waves grow exponentially fast. Second, bubble collisions add a new burst of gravitational radiation. Third, turbulent motions finally sets the end of gravitational waves production. From then on, these waves propagate unimpeded to us. We find that the fraction of energy density today in these primordial gravitational waves could be significant for GUT scale models of inflation, although well beyond the frequency range sensitivity…
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Taxonomy
TopicsCosmology and Gravitation Theories · Pulsars and Gravitational Waves Research · Geophysics and Gravity Measurements
