Gravitational Waves from Preheating in Inflation with Weyl Symmetry
arXiv:2311.00239 · doi:10.1103/PhysRevD.109.083542
Abstract
Inflation with Weyl scaling symmetry provides a viable scenario that can generate both the nearly scaling invariant primordial density fluctuation and a dark matter candidate. Here we point out that, in additional to the primordial gravitational waves (GWs) from quantum fluctuations, the production of high-frequency GWs from preheating in such inflation models can provide an another probe of the inflationary dynamics. We conduct both linear analytical analysis and nonlinear numerical lattice simulation in a typical model. We find that significant stochastic GWs can be produced and the frequency band is located around Hz Hz, which might be probed by future resonance-cavity experiments.
21 pages, 6 figures
References in corpus (34)
- The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background
- Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array
- Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I
- The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- The NANOGrav 15-year Data Set: Search for Signals from New Physics
- Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies
- Theory and Numerics of Gravitational Waves from Preheating after Inflation
- CMB-S4: Forecasting Constraints on Primordial Gravitational Waves
- Improved limits on the tensor-to-scalar ratio using BICEP and Planck
- Superconformal Symmetry, NMSSM, and Inflation
- A solution to the hierarchy problem from an almost decoupled hidden sector within a classically scale invariant theory
- Scale invariant extension of the standard model with strongly interacting hidden sector
- Search for a stochastic background of 100-MHz gravitational waves with laser interferometers
- CosmoLattice
- DEFROST: A New Code for Simulating Preheating after Inflation
- Gravitational Waves from Oscillons with Cuspy Potentials
- Gravitational wave production from preheating: parameter dependence
- The Art of Lattice and Gravity Waves from Preheating
- Electromagnetic Antennas for the Resonant Detection of the Stochastic Gravitational Wave Background
- Inflation from Broken Scale Invariance
- Detecting Planetary-mass Primordial Black Holes with Resonant Electromagnetic Gravitational Wave Detectors
- Inflation in Metric-Affine Quadratic Gravity
- Sensitivity of the spherical gravitational wave detector MiniGRAIL operating at 5 K
- Implication of Compensator Field and Local Scale Invariance in the Standard Model
- Dark matter as a Weyl geometric effect
- Exploring High Frequency Gravitational Waves with Magnons
- Observation of the Fundamental Nyquist Noise Limit in an Ultra-High -Factor Cryogenic Bulk Acoustic Wave Cavity
- Limits on High-Frequency Gravitational Waves in Planetary Magnetospheres
- Gravitational wave search through electromagnetic telescopes
- Dark Matter Production in Weyl Inflation
- Inflation in Weyl Scaling Invariant Gravity with Extensions
- Cosmic inflation from broken conformal symmetry
- On Conformal Transformation with Multiple Scalar Fields and Geometric Property of Field Space with Einstein-like Solutions
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- Nonlinear dynamics of oscillons and transients during preheating after single field inflation
- Dynamically induced spin-2 mass in a Weyl-invariant framework
- Revisiting local-scale invariant gravitational theory
- Inflation in light of ACT/SPT: A new perspective from Weyl gravity
- Inflationary assessment of Einstein-Cartan models