Scale-Dependent Bias of Galaxies from Baryonic Acoustic Oscillations
arXiv:1009.1393 · doi:10.1111/j.1365-2966.2011.18922.x
Abstract
Baryonic acoustic oscillations (BAOs) modulate the density ratio of baryons to dark matter across large regions of the Universe. We show that the associated variation in the mass-to-light ratio of galaxies should generate an oscillatory, scale-dependent bias of galaxies relative to the underlying distribution of dark matter. A measurement of this effect would calibrate the dependence of the characteristic mass-to-light ratio of galaxies on the baryon mass fraction in their large scale environment. This bias, though, is unlikely to significantly affect measurements of BAO peak positions.
6 pages, 3 figures, submitted to MNRAS
References in corpus (6)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- The physics driving the cosmic star formation history
- The recycling of gas and metals in galaxy formation: predictions of a dynamical feedback model
- The formation and gas content of high redshift galaxies and minihalos
- Cosmological perturbation theory for baryons and dark matter I: one-loop corrections in the RPT framework
- Scale-dependent Galaxy Bias
Cited by in corpus (24)
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- Large-Scale Galaxy Bias
- Suppression and Spatial Variation of Early Galaxies and Minihalos
- The Rise of the First Stars: Supersonic Streaming, Radiative Feedback, and 21-cm Cosmology
- Simulations of Early Baryonic Structure Formation with Stream Velocity: II. The Gas Fraction
- Line-Intensity Mapping: Theory Review
- The effect of relative velocity and density perturbations between baryons and dark matter on the clustering of galaxies
- Robust Velocity-induced Acoustic Oscillations at Cosmic Dawn
- Galaxy bias and primordial non-Gaussianity: insights from galaxy formation simulations with IllustrisTNG
- Low-mass suppression of the satellite luminosity function due to the supersonic baryon--cold-dark-matter relative velocity
- Probing correlated compensated isocurvature perturbations using scale-dependent galaxy bias
- Baryon-CDM isocurvature galaxy bias with IllustrisTNG
- The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
- How Density Environment Changes the Influence of the Dark Matter-Baryon Streaming Velocity on the Cosmological Structure Formation
- Constraining the relative velocity effect using the Baryon Oscillation Spectroscopic Survey
- Large scale distribution of total mass versus luminous matter from Baryon Acoustic Oscillations: First search in the SDSS-III BOSS Data Release 10
- Imprints of Reionization in Galaxy Clustering
- Compensated Isocurvature Perturbations in the Galaxy Power Spectrum
- Formation of First Galaxies inside Density Peaks and Voids under the Influence of Dark Matter-Baryon Streaming Velocity, I: Initial Condition and Simulation Scheme
- Large scale distribution of mass versus light from Baryon Acoustic Oscillations: Measurement in the final SDSS-III BOSS Data Release 12
- Cosmological Constraints on the Global Star Formation Law of Galaxies: Insights From Baryon Acoustic Oscillation Intensity Mapping
- Effects of chemically homogeneous evolution of the first stars on the 21-cm signal and reionization
- The Effects of Dark Matter Annihilation and Dark Matter-Baryon Velocity Offsets at Cosmic Dawn
- Cosmic voids and BAO with relative baryon-CDM perturbations