Cosmology and the Early Universe
arXiv:1903.09260
Abstract
This Astro-2020 White Paper deals with what we might learn from future gravitational wave observations about the early universe phase transitions and their energy scales, primordial black holes, Hubble parameter, dark matter and dark energy, modified theories of gravity and extra dimensions.
arXiv comment13 pages, 3 figures, White Paper submitted to the Astro-2020 (2020 Astronomy and Astrophysics Decadal Survey) by GWIC-3G Science Case Team (GWIC: Gravitational-Wave International Committee)
References in corpus (80)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- A gravitational-wave standard siren measurement of the Hubble constant
- Did LIGO detect dark matter?
- Primordial Black Hole Scenario for the Gravitational-Wave Event GW150914
- Gravitational Radiation from First-Order Phase Transitions
- Astrophysical Implications of the Binary Black-Hole Merger GW150914
- Using gravitational-wave standard sirens
- 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
- Shape of the acoustic gravitational wave power spectrum from a first order phase transition
- Science with the space-based interferometer LISA. IV: Probing inflation with gravitational waves
- Exploring short gamma-ray bursts as gravitational-wave standard sirens
- How generic is cosmic string formation in SUSY GUTs
- GW150914: Implications for the stochastic gravitational wave background from binary black holes
- Large Nongaussianity in Axion Inflation
- Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run
- Particle production during inflation and gravitational waves detectable by ground-based interferometers
- Short GRB and binary black hole standard sirens as a probe of dark energy
- Probing the early universe with inflationary gravitational waves
- Inference of the cosmological parameters from gravitational waves: application to second generation interferometers
- Ultra-high precision cosmology from gravitational waves
- Production and detection of relic gravitons in quintessential inflationary models
- Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
- Stochastic gravitational wave background from smoothed cosmic string loops
- GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences
- Anisotropic stress as signature of non-standard propagation of gravitational waves
- Cosmography with the Einstein Telescope
- Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information
- Science with the space-based interferometer eLISA. III: Probing the expansion of the Universe using gravitational wave standard sirens
- Cosmological perturbations and structure formation in nonlocal infrared modifications of general relativity
- Non-local gravity and dark energy
- Cosmology with the lights off: Standard sirens in the Einstein Telescope era
- The gravitational-wave luminosity distance in modified gravity theories
- Relating gravitational wave constraints from primordial nucleosynthesis, pulsar timing, laser interferometers, and the CMB: implications for the early universe
- Modified gravitational-wave propagation and standard sirens
- Gravitational-wave cosmology across 29 decades in frequency
- Finding the Electromagnetic Counterparts of Cosmological Standard Sirens
- Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
- Gravitational waves constraints on post-inflationary phases stiffer than radiation
- Constraints on cosmic strings using data from the first Advanced LIGO observing run
- Digging deeper: Observing primordial gravitational waves below the binary black hole produced stochastic background
- Generalized framework for testing gravity with gravitational-wave propagation. II. Constraints on Horndeski theory
- Stochastic Gravitational-Wave Background due to Primordial Binary Black Hole Mergers
- Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
- Searching for Dark Photon Dark Matter with Gravitational Wave Detectors
- Phantom dark energy from non-local infrared modifications of General Relativity
- Probing Gravity with Spacetime Sirens
- Anisotropy of the astrophysical gravitational wave background: analytic expression of the angular power spectrum and correlation with cosmological observations
- Metallicity-constrained merger rates of binary black holes and the stochastic gravitational wave background
- Anisotropies of Gravitational Wave Backgrounds: A Line Of Sight Approach
- An inflationary model with small scalar and large tensor nongaussianities
- First predictions of the angular power spectrum of the astrophysical gravitational wave background
- Gravitational Radiation from Primordial Helical Inverse Cascade MHD Turbulence
- Effect of lensing magnification on the apparent distribution of black hole mergers
- Anisotropies in the stochastic gravitational-wave background: Formalism and the cosmic string case
- Beyond Concordance Cosmology with Magnification of Gravitational-Wave Standard Sirens
- Cosmology with space-based gravitational-wave detectors --- dark energy and primordial gravitational waves ---
- The effect of matter structure on the gravitational waveform
- Revisiting the envelope approximation: gravitational waves from bubble collisions
- Detecting Relic Gravitational Waves by Pulsar Timing Arrays: Effects of Cosmic Phase Transitions and Relativistic Free-Streaming Gases
- The Standard Model Higgs as the origin of the hot Big Bang
- On the waveforms of gravitationally lensed gravitational waves
- The signal of the stochastic gravitational wave background and the angular correlation of its energy density
- Cosmological perturbation effects on gravitational-wave luminosity distance estimates
- Stochastic gravitational wave background from hydrodynamic turbulence in differentially rotating neutron stars
- A Systematic Study of the Stochastic Gravitational-Wave Background due to Stellar Core Collapse
- A Model of the Stochastic Gravitational-Wave Background due to Core Collapse to Black Holes
- Gravitational Radiation from Primordial Helical MHD Turbulence
- Measuring neutron-star ellipticity with measurements of the stochastic gravitational-wave background
- Integrated Sachs-Wolfe Effect for Gravitational Radiation
- A synthetic model of the gravitational wave background from evolving binary compact objects
- Gravitational wave background from population III binaries
- Multi-wavelength observations of cosmological phase transitions using LISA and Cosmic Explorer