Gravitational Radiation from Primordial Helical Inverse Cascade MHD Turbulence

Abstract

We consider the generation of gravitational waves by primordial helical inverse cascade magnetohydrodynamic (MHD) turbulence produced by bubble collisions at the electroweak phase transition. We extend the previous study \cite{kgr08} by considering both currently discussed models of MHD turbulence. For popular electroweak phase transition parameter values, the generated gravitational wave spectrum is only weakly dependent on the MHD turbulence model. Compared to the unmagnetized electroweak phase transition case, the spectrum of MHD-turbulence-generated gravitational waves peaks at lower frequency with larger amplitude and can be detected by the proposed Laser Interferometer Space Antenna

13 pages, 4 figures; typos corrected

References in corpus (26)

• Gravitational Wave Production by Collisions: More Bubbles
• Gravitational Waves from Phase Transitions at the Electroweak Scale and Beyond
• Gravitational wave generation from bubble collisions in first-order phase transitions: an analytic approach
• Theory and Numerics of Gravitational Waves from Preheating after Inflation
• A Gravitational Wave Background from Reheating after Hybrid Inflation
• Gravitational waves from stochastic relativistic sources: primordial turbulence and magnetic fields
• Dynamics of Non-renormalizable Electroweak Symmetry Breaking
• The Spectrum of Gravitational Radiation from Primordial Turbulence
• Circular Polarization of Primordial Gravitational Waves in String-inspired Inflationary Cosmology
• Gravitational Waves from Warped Spacetime
• CMB anisotropies from primordial inhomogeneous magnetic fields
• Production of Gravitational Waves in the nMSSM
• Probing polarization states of primordial gravitational waves with CMB anisotropies
• Magnetic field production during preheating at the electroweak scale
• Detectability of Gravitational Waves from Phase Transitions
• Prospects for direct detection of primordial gravitational waves
• The Beginning and Evolution of the Universe
• Nonlinear current helicity fluxes in turbulent dynamos and alpha quenching
• Evolution of Magnetic Fields in Freely Decaying Magnetohydrodynamic Turbulence
• Prospects for direct detection of circular polarization of gravitational-wave background
• Gravitational Waves From the End of Inflation: Computational Strategies
• Phenomenology of the nMSSM from colliders to cosmology
• Scaling laws in decaying helical hydromagnetic turbulence
• Gravitational Radiation from Primordial Helical MHD Turbulence
• Gravitational waves from deflagration bubbles in first-order phase transitions
• Gravitational Wave Sources from New Physics

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