A Pairwise Surrogate for Gravitational-Wave Spectra from Highly Relativistic Vacuum Bubble Collisions
gr-qc, astro-ph.CO, hep-ph
Submitted: 2026-10-08
Updated: 2026-10-08
Code: https://github.com/MSABuschmann/PhaseTransitionBuilder
Terminology
Sources
- Global String Radiation
- Evolution of Axionic Strings and Spectrum of Axions Radiated from Them
- Axion dark matter: strings and their cores
- Axions from Strings: the Attractive Solution
- Dark Matter from Axion Strings with Adaptive Mesh Refinement
- Cosmological phase transitions: from perturbative particle physics to gravitational waves
- On bubble collisions in strongly supercooled phase transitions
- Gravitational wave spectra from strongly supercooled phase transitions
- Updated predictions for gravitational waves produced in a strongly supercooled phase transition
- Friction pressure on relativistic bubble walls
- The Supercooling Window at Weak and Strong Coupling
- Gravitational waves from vacuum first-order phase transitions: from the envelope to the lattice
- Sledgehamr: Simulating Scalar Fields with Adaptive Mesh Refinement
- Gravitational Radiation from Colliding Vacuum Bubbles: Envelope Approximation to Many-Bubble Collisions
- Gravitational Wave Production by Collisions: More Bubbles
- Revisiting the envelope approximation: gravitational waves from bubble collisions
- Gravitational waves from bubble collisions: analytic derivation
- Model-independent features of gravitational waves from bubble collisions
- Gravitational radiation from a bulk flow model
- Gravitational waves from bubble dynamics: Beyond the Envelope
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