Distance Probes of Dark Energy
arXiv:1309.5382 · doi:10.1016/j.astropartphys.2014.05.007
Abstract
This document presents the results from the Distances subgroup of the Cosmic Frontier Community Planning Study (Snowmass 2013). We summarize the current state of the field as well as future prospects and challenges. In addition to the established probes using Type IA supernovae and baryon acoustic oscillations, we also consider prospective methods based on clusters, active galactic nuclei, gravitational wave sirens and strong lensing time delays.
Report from the "Dark Energy and CMB" working group for the American Physical Society's Division of Particles and Fields long-term planning exercise ("Snowmass"). Accepted for publication in Astroparticle Physics
References in corpus (39)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
- Cosmological Constraints from the SDSS Luminous Red Galaxies
- Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
- Supernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey
- Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2
- Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
- Baryon Acoustic Oscillations in the Ly-α forest of BOSS quasars
- Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak
- SNLS3: Constraints on Dark Energy Combining the Supernova Legacy Survey Three Year Data with Other Probes
- Double Compact Objects II: Cosmological Merger Rates
- Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications
- Toward a New Geometric Distance to the Active Galaxy NGC 4258. III. Final Results and the Hubble Constant
- Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure
- The Spectroscopic Diversity of Type Ia Supernovae
- Cosmology and Astrophysics from Relaxed Galaxy Clusters II: Cosmological Constraints
- Inflation Physics from the Cosmic Microwave Background and Large Scale Structure
- Results from the Supernova Photometric Classification Challenge
- Type Ia Supernovae are Good Standard Candles in the Near Infrared: Evidence from PAIRITEL
- Cosmological baryonic and matter densities from 600,000 SDSS Luminous Red Galaxies with photometric redshifts
- Dark energy and curvature from a future baryonic acoustic oscillation survey using the Lyman-alpha forest
- Reconstructing Baryon Oscillations: A Lagrangian Theory Perspective
- Growth of Cosmic Structure: Probing Dark Energy Beyond Expansion
- Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
- Wide-Field InfraRed Survey Telescope (WFIRST) Final Report
- Calibrating the Baryon Oscillation Ruler for Matter and Halos
- Application of Stochastic Modeling to Analysis of Photometric Reverberation Mapping Data
- Galaxy Bias and its Effects on the Baryon Acoustic Oscillations Measurements
- The case for OH suppression at near-infrared wavelengths
- Calibrating Dark Energy
- The Hubble Sphere Hydrogen Survey
- Determining the Hubble constant from gravitational wave observations of merging compact binaries
- Wide-Field InfraRed Survey Telescope (WFIRST) Interim Report
- Improving Dark Energy Constraints with High Redshift Type Ia Supernovae from CANDELS and CLASH
- Measuring cosmic distances with galaxy clusters
- Large-Scale Structure and Future Surveys
- Photometric Calibrations for 21st Century Science
- Cosmology with the Ly-a forest
- Addressing the Photometric Calibration Challenge: Explicit Determination of the Instrumental Response and Atmospheric Response Functions, and Tying it All Together
Cited by in corpus (10)
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- Time Delay Cosmography
- Strong Dependence of Type Ia Supernova Standardization on the Local Specific Star Formation Rate
- Growth of Cosmic Structure: Probing Dark Energy Beyond Expansion
- Constraining the dark energy models with H(z) data: an approach independent of
- Neutrino flavor transformation in the lepton-asymmetric universe
- : Mock Challenge for a Forward Modeling Approach to Galaxy Clustering
- Measuring using X-ray and SZ effect observations of dynamically relaxed galaxy clusters
- SNe Ia as a cosmological probe