Singlet Extended Mirror Standard Model World as Dark Matter and Gravitational Waves Imprints of a High Scale Mirror Phase Transitions
hep-ph, astro-ph.CO, gr-qc, hep-th
Submitted: 2026-08-14
Updated: 2026-08-14
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Simons Observatory: Astro2020 Decadal Project Whitepaper
- Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey
- Sensitivity Studies for Third-Generation Gravitational Wave Observatories
- The Laser Interferometer Space Antenna: Unveiling the Millihertz Gravitational Wave Sky
- LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources
- Beyond LISA: Exploring Future Gravitational Wave Missions
- Sensitivity to a Frequency-Dependent Circular Polarization in an Isotropic Stochastic Gravitational Wave Background
- Possibility of Direct Measurement of the Acceleration of the Universe Using 0.1 Hz Band Laser Interferometer Gravitational Wave Antenna in Space
- Current status of space gravitational wave antenna DECIGO and B-DECIGO
- Fundamental Physics with the Square Kilometre Array
- Cosmology with the Laser Interferometer Space Antenna
- Inflationary Cosmology
- Inflationary Cosmology after Planck 2013
- Recent Advances on Inflation
- The Quest for B Modes from Inflationary Gravitational Waves
- Tensor Perturbations in Inflationary Models as a Probe of Cosmology
- Probing the early universe with inflationary gravitational waves
- Relic Gravitational Waves in the Accelerating Universe
- Cosmological Backgrounds of Gravitational Waves
- Constraints on primordial gravitational waves from the Cosmic Microwave Background
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