Quantifying the tension between cosmological models and JWST red candidate massive galaxies
arXiv:2311.02866 · doi:10.1088/1674-4527/ad2cd3
Abstract
We develop a Python tool to estimate the tail distribution of the number of dark matter halos beyond a mass threshold and in a given volume in a light-cone. The code is based on the extended Press-Schechter model and is computationally efficient, typically taking a few seconds on a personal laptop for a given set of cosmological parameters. The high efficiency of the code allows a quick estimation of the tension between cosmological models and the red candidate massive galaxies released by the James Webb Space Telescope, as well as scanning the theory space with the Markov Chain Monte Carlo method. As an example application, we use the tool to study the cosmological implication of the candidate galaxies presented in Labbé et al. (2023). The standard cold dark matter (CDM) model is well consistent with the data if the star formation efficiency can reach at high redshift. For a low star formation efficiency , CDM model is disfavored at - confidence level.
6 pages, 3 figures
References in corpus (39)
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
- Exploring the Expansion History of the Universe
- An excursion set model of hierarchical clustering: Ellipsoidal collapse and the moving barrier
- A population of red candidate massive galaxies ~600 Myr after the Big Bang
- Cosmic Variance and Its Effect on the Luminosity Function Determination in Deep High z Surveys
- Stress Testing CDM with High-redshift Galaxy Candidates
- The universality of the virial halo mass function and models for non-universality of other halo definitions
- On the stunning abundance of super-early, massive galaxies revealed by JWST
- Evolution of the Mass Function of Dark Matter Haloes
- CEERS Spectroscopic Confirmation of NIRCam-Selected z > 8 Galaxy Candidates with JWST/NIRSpec: Initial Characterization of their Properties
- Galaxy evolution near groups and clusters: ejected satellites and the spatial extent of environmental quenching
- Extreme Value Statistics of the Halo and Stellar Mass Distributions at High Redshift: are JWST Results in Tension with ΛCDM?
- CEERS Key Paper V: A triality on the nature of HST-dark galaxies
- Further evidence for a population of dark-matter-deficient dwarf galaxies
- Dark energy in light of the early JWST observations: case for a negative cosmological constant?
- Has JWST already falsified dark-matter-driven galaxy formation?
- High-Redshift Galaxies from Early JWST Observations: Constraints on Dark Energy Models
- Primordial power spectrum in light of JWST observations of high redshift galaxies
- The distribution of ejected subhalos and its implication for halo assembly bias
- LAGER Ly Luminosity Function at , Implications for Reionization
- Alleviating the need for exponential evolution of JWST galaxies in 10 haloes at by a modified CDM power spectrum
- The Cosmic Timeline Implied by the JWST High-redshift Galaxies
- Flybys, orbits, splashback: subhalos and the importance of the halo boundary
- Early Structure Formation from Cosmic String Loops in Light of Early JWST Observations
- SILVERRUSH XI: Constraints on the Ly luminosity function and cosmic reionization at with Subaru/Hyper Suprime-Cam
- JWST high-z galaxy constraints on warm and cold dark matter models
- Cosmological Model Tests with JWST
- Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
- Modeling the JWST high-redshift galaxies with a general formation scenario and the consistency with the CDM model
- Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at ?
- Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
- Black holes as the source of dark energy: a stringent test with high-redshift JWST AGNs
- Excess of high- galaxies as a test for bumpy power spectrum of density perturbations
- Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
- Virial halo mass function in the cosmology
- The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
- High-redshift Mini-haloes from Modulated Preheating
- Impact of the primordial fluctuation power spectrum on the reionization history
Cited by in corpus (10)
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
- Transition dynamics in the CDM model: Implications for bound cosmic structures
- Key drivers of the preference for dynamic dark energy
- Measuring neutrino masses with joint JWST and DESI DR2 data
- Can Dark Stars account for the star formation efficiency excess at very high redshifts?
- Stringent constraint on the CCC+TL cosmology with Measurements
- Curvature perturbations from kinetic preheating after -attractor inflation
- Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies
- Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST