Conformal Unification in a Quiver Theory and Gravitational Waves
arXiv:2005.12216 · doi:10.1016/j.physletb.2020.135909
Abstract
The detection of a stochastic background of gravitational waves can reveal details about first-order phase transitions (FOPTs) at a time of of the early universe. We specifically discuss quiver-type GUTs which avoid both proton decay and a desert hypothesis. A quiver based on which breaks at a GeV to trinification has a much larger () number of effective massless degrees of freedom than the Standard Model. Assuming a FOPT for this model we investigate the strain sensitivity of this model for a wide range of FOPT parameters.
arXiv comment19 pages, 7 Figs. Revised final version, to appear on Phys. Lett. B
References in corpus (35)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- The Large N Limit of Superconformal Field Theories and Supergravity
- Multi-messenger Observations of a Binary Neutron Star Merger
- Laser Interferometer Space Antenna
- Science with the space-based interferometer eLISA. II: Gravitational waves from cosmological phase transitions
- Gravitational Radiation from First-Order Phase Transitions
- Detecting gravitational waves from cosmological phase transitions with LISA: an update
- Energy Budget of Cosmological First-order Phase Transitions
- Gravitational Wave Production by Collisions: More Bubbles
- Gravitational waves from the sound of a first order phase transition
- Numerical simulations of acoustically generated gravitational waves at a first order phase transition
- Gravitational Radiation from Colliding Vacuum Bubbles: Envelope Approximation to Many-Bubble Collisions
- The stochastic gravitational wave background from turbulence and magnetic fields generated by a first-order phase transition
- Strong Electroweak Phase Transitions in the Standard Model with a Singlet
- Prospects for Fundamental Physics with LISA
- Cosmological Backgrounds of Gravitational Waves and eLISA/NGO: Phase Transitions, Cosmic Strings and Other Sources
- AEDGE: Atomic Experiment for Dark Matter and Gravity Exploration in Space
- On the Maximal Strength of a First-Order Electroweak Phase Transition and its Gravitational Wave Signal
- Gravitational wave energy budget in strongly supercooled phase transitions
- Postmerger Gravitational-Wave Signatures of Phase Transitions in Binary Mergers
- Gravitational waves from first-order cosmological phase transitions: lifetime of the sound wave source
- Gravitational waves from a first order electroweak phase transition: a brief review
- Vorticity, kinetic energy, and suppressed gravitational wave production in strong first order phase transitions
- Numerical Simulations of Gravitational Waves from Early-Universe Turbulence
- Models for Little Rip Dark Energy
- Gravitational Waves from Supercool Axions
- Primordial Anisotropies in the Gravitational Wave Background from Cosmological Phase Transitions
- Cosmological Phase Transitions in Warped Space: Gravitational Waves and Collider Signatures
- Bubble wall velocities in the Standard Model and beyond
- Mid-band gravitational wave detection with precision atomic sensors
- Composite Dynamics in the Early Universe
- ADS/CFT String Duality and Conformal Gauge Field Theories
- Strong-Electroweak Unification at About 4 TeV
- Two-field cosmological phase transitions and gravitational waves in the singlet Majoron model
- Robustness and Predictivity of 4 TeV Unification