Stochastic Bubble Completion in de Sitter Space: Power Spectrum, Bispectrum, and Infrared Moment Hierarchies
astro-ph.CO, gr-qc, hep-ph, hep-th
Submitted: 2026-10-06
Updated: 2026-10-06
Terminology
Sources
- Detecting gravitational waves from cosmological phase transitions with LISA: an update
- Cosmological phase transitions: from perturbative particle physics to gravitational waves
- Constraining first-order phase transitions with curvature perturbations
- Finite Bubble Statistics Constrain Late Cosmological Phase Transitions
- Cosmological and Astrophysical Constraints on Late First-Order Phase Transitions
- Bubble nucleation and inflationary perturbations
- Dark Radiation Isocurvature from Cosmological Phase Transitions
- The curvature perturbations and induced gravitational waves induced by the first-order phase transition during reheating
- Phase transition during inflation and the gravitational wave signal at pulsar timing arrays
- Simulating first-order phase transition during inflation
- Gravitational waves from first-order phase transitions: Towards model separation by bubble nucleation rate
- Black holes and gravitational waves from phase transitions in realistic models
- Bubble Correlation in First-Order Phase Transitions
- Bubble Clustering in Cosmological First Order Phase Transitions
- Curvature Perturbations from First-Order Phase Transitions: Implications to Black Holes and Gravitational Waves
- How large are curvature perturbations from slow first-order phase transitions? A gauge-invariant analysis
- Cosmology with a TeV mass GUT Higgs
- Thermal Inflation and the Moduli Problem
- Thermal Inflation and the Gravitational Wave Background
- Phase Transitions and Gravitational Wave Production at the End of Thermal Inflation
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