Domain Walls From Confining Bubbles: SU(N c) Yang Mills at Finite theta
Bruno Missoni, Enrico Morgante, Nicklas Ramberg
hep-ph, astro-ph.CO, hep-th
Submitted: 2026-07-21
Comments: 13 pages, 9 figures, comments are welcome
License: http://creativecommons.org/licenses/by/4.0/
The gist: We study the confinement phase transition in SU(N c) pure Yang-Mills theory at finite theta not equal to 0 using the Improved Holographic QCD (IHQCD) model.
Terminology
Abstract
We study the confinement phase transition in SU(N c) pure Yang-Mills theory at finite theta not equal to 0 using the Improved Holographic QCD (IHQCD) model. We show that the critical temperature, as a function of theta for large but fixed N c, is reduced, thus decreasing the amount of supercooling in the confinement phase transition. Upon completion of the confinement phase transition, a network of domain walls can be produced, owing to the multi-branched vacuum structure of Yang-Mills theory at finite theta. We highlight the potential interplay between the produced domain walls and the confinement phase transition dynamics. We emphasize that DW production from bubble coalescence in strongly coupled non-conformal FOPTs is a dynamical process of vacuum assignment, hydrodynamics, and local reheating effects, all potentially affecting the approach towards the scaling regime. Lastly, we demonstrate the level of tuning necessary for potentially interesting imprints from gravitational waves through domain wall annihilation and its interplay with the confinement PT.
Sources
- Twin-peaked gravitational wave signals from a Z 2 phase transition
- Domain wall networks from first-order phase transitions and gravitational waves
- Detector configuration of DECIGO/BBO and identification of cosmological neutron-star binaries
- Laser Interferometer Space Antenna
- Gravitational wave astronomy with the SKA
- Conformal model for gravitational waves and dark matter: A status update
- Gravitational waves from supercooled phase transitions: dimensional transmutation meets dimensional reduction
- QCD-sourced tachyonic phase transition in a supercooled Universe
- Supercool exit: Gravitational waves from QCD-triggered conformal symmetry breaking
- Impact of theoretical uncertainties on model parameter reconstruction from GW signals sourced by cosmological phase transitions
- Primordial gravitational waves in the nano-Hertz regime and PTA data -- towards solving the GW inverse problem
- A critical look at low-scale cosmological phase transitions in the PTA era
- Theoretical uncertainties for cosmological first-order phase transitions
- Beyond the Daisy Chain: Running and the 3D EFT View of Supercooled Phase Transitions
- Dark, Cold, and Noisy: Constraining Secluded Hidden Sectors with Gravitational Waves
- Leptophilic dark matter from gauged lepton number: Phenomenology and gravitational wave signatures
- Gravitational waves from the sound shell model: direct and inverse phase transitions in the early Universe
- Gravitational waves from defect-driven phase transitions: domain walls
- The Supercooled Universe
- Does NANOGrav observe a dark sector phase transition?
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