Gravitational Waves at Strong Coupling from an Effective Action
arXiv:2110.14442 · doi:10.1103/PhysRevLett.128.131101
Abstract
Using a holographic derivation of a quantum effective action for a scalar operator at strong coupling, we compute quasi-equilibrium parameters relevant for the gravitational wave signal from a first order phase transition in a simple dual model. We discuss how the parameters of the phase transition vary with the effective number of degrees of freedom of the dual field theory. Our model can produce an observable signal at LISA if the critical temperature is around a TeV, in a parameter region where the field theory has an approximate conformal symmetry.
arXiv comment6 pages, 3 figures
References in corpus (54)
- AdS/CFT Correspondence and Symmetry Breaking
- Is There a Hot Electroweak Phase Transition at $m_H\gsim m_W$?
- The NANOGrav 12.5-year Data Set: Search For An Isotropic Stochastic Gravitational-Wave Background
- Detecting gravitational waves from cosmological phase transitions with LISA: an update
- Quasinormal modes and holography
- Energy Budget of Cosmological First-order Phase Transitions
- Shape of the acoustic gravitational wave power spectrum from a first order phase transition
- Composite Higgses
- SU(N) gauge theories at large N
- Basics of thermal field theory -- a tutorial on perturbative computations
- Electroweak Bubble Wall Speed Limit
- How fast can the wall move? A study of the electroweak phase transition dynamics
- The Growth of Bubbles in Cosmological Phase Transitions
- The high temperature phase transition in SU(N) gauge theories
- Theoretical uncertainties for cosmological first-order phase transitions
- Properties of the deconfining phase transition in SU(N) gauge theories
- Vorticity, kinetic energy, and suppressed gravitational wave production in strong first order phase transitions
- Bubble Wall Velocity at the Electroweak Phase Transition
- Gravitational waves from a first order electroweak phase transition: a brief review
- Gravitational waves from first order cosmological phase transitions in the Sound Shell Model
- Cosmological Consequences of Nearly Conformal Dynamics at the TeV scale
- Phase transitions in the early universe
- Designer Gravity and Field Theory Effective Potentials
- Model-independent energy budget of cosmological first-order phase transitions
- Searching For Gravitational Waves From Cosmological Phase Transitions With The NANOGrav 12.5-year dataset
- Bubble wall velocity: heavy physics effects
- Model-independent energy budget for LISA
- Nonperturbative analysis of the gravitational waves from a first-order electroweak phase transition
- A Strong Electroweak Phase Transition up to m_H ~ 105 GeV
- On the perturbative expansion at high temperature and implications for cosmological phase transitions
- Testing the dark SU(N) Yang-Mills theory Confined Landscape: From the Lattice to Gravitational Waves
- Massive black hole binary systems and the NANOGrav 12.5 year results
- Bubble wall velocities in the Standard Model and beyond
- Holographic QCD in the Veneziano limit and neutron stars
- Thermodynamics, transport and relaxation in non-conformal theories
- Lattice study of an electroweak phase transition at m_h ~ 126 GeV
- Bubble Wall Velocity at Strong Coupling
- Gravitational Waves from Holographic Neutron Star Mergers
- Unified weak/strong coupling framework for nuclear matter and neutron stars
- Bubble Wall Velocity from Holography
- Gravitational Waves from Dark Yang-Mills Sectors
- Lectures on walking technicolor, holography and gauge/gravity dualities
- The bubble wall velocity in the minimal supersymmetric light stop scenario
- Wall speed and shape in singlet-assisted strong electroweak phase transitions
- Exotic holographic RG flows at finite temperature
- Gravitational waves from a holographic phase transition
- Holographic quantum criticality from multi-trace deformations
- The holographic quantum effective potential at finite temperature and density
- Effective actions and bubble nucleation from holography
- Heating up Exotic RG Flows with Holography
- Revisiting Coleman-de Luccia transitions in the AdS regime using holography
- Black brane evaporation through D-brane bubble nucleation
- TASI Lectures on Early Universe Cosmology: Inflation, Baryogenesis and Dark Matter
- A simple description of holographic domain walls in confining theories -- extended hydrodynamics
Cited by in corpus (15)
- Echo of the Dark: gravitational waves from dark SU(3) Yang-Mills theory
- Gravitational Waves and Primordial Black Hole Productions from Gluodynamics by Holography
- Holographic Bubbles with Jecco: Expanding, Collapsing and Critical
- A perfect fluid hydrodynamic picture of domain wall velocities at strong coupling
- Effective actions and bubble nucleation from holography
- Constraints on holographic QCD phase transitions from PTA observations
- Bubble expansion at strong coupling
- Gravitational Waves from dark composite dynamics
- Dynamical stability from quasi normal modes in 2nd, 1st and 0th order holographic superfluid phase transitions
- Bubble nucleation and gravitational wave from holography
- General bubble expansion at strong coupling
- Thermal Emission of Gravitational Waves from Weak to Strong Coupling
- Spinodal Gravitational Waves
- Bubbles kick off primordial black holes to form more binaries
- Testing the effective action approach to bubble nucleation in holography