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相关论文: High-redshift Galaxies from JWST Observations in M…

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The James Webb Space Telescope (JWST) has unveiled a population of unexpectedly massive and luminous galaxies at redshifts $z \gtrsim 7$, posing a significant challenge to the standard $\Lambda$CDM cosmological paradigm. In this work, we…

星系天体物理 · 物理学 2026-03-17 Saeed Fakhry , Maryam Shiravand , Antonino Del Popolo

The James Webb Space Telescope (JWST) is unveiling astounding results about the first few hundred million years of life of the Universe, delivering images of galaxies at very high redshifts. Here, we develop a UV luminosity function model…

宇宙学与河外天体物理 · 物理学 2024-09-17 Fabio Iocco , Luca Visinelli

The James Webb Space Telescope (JWST) discovered several luminous high-redshift galaxy candidates with stellar masses of $M_{*} \gtrsim 10^{9} \, \rm{M_{\odot}}$ at photometric redshifts $z_{\mathrm{phot}} \gtrsim 10$ which allows to…

星系天体物理 · 物理学 2022-11-30 Moritz Haslbauer , Pavel Kroupa , Akram Hasani Zonoozi , Hosein Haghi

The discovery of massive, high redshift galaxies with the James Webb Space Telescope (JWST) has been argued to challenge $\Lambda$CDM (cold dark matter): such systems would require extremely rare halos and baryon-to-stellar-mass conversion…

星系天体物理 · 物理学 2026-04-28 Jay R. Krishnan , Kevork N. Abazajian

The James Webb Space Telescop (JWST) promises to revolutionise our understanding of the early Universe, and contrasting its upcoming observations with predictions of the $\Lambda$CDM model requires detailed theoretical forecasts. Here, we…

The James Webb Space Telescope (JWST) will enable observations of galaxies at redshifts z > 10 and hence allow to test our current understanding of structure formation at very early times. Previous work has shown that the very first…

宇宙学与河外天体物理 · 物理学 2011-05-10 Andreas H. Pawlik , Milos Milosavljevic , Volker Bromm

The James Webb Space Telescope (JWST), which has recently become operational, is capable of detecting objects at record-breaking redshifts, $z \gtrsim 15$. This is a crucial advance for observational cosmology, as at these redshifts the…

宇宙学与河外天体物理 · 物理学 2022-12-14 Nikita Lovyagin , Alexander. Raikov , Vladimir Yershov , Yuri Lovyagin

We compare properties of high-redshift galaxies observed by JWST with hydrodynamical simulations, in the standard cold dark matter model and in warm dark matter models with a suppressed linear matter power spectrum. We find that current…

宇宙学与河外天体物理 · 物理学 2023-04-05 Umberto Maio , Matteo Viel

Early observations with JWST have led to the discovery of an unexpected large density (stellar mass density $\rho_*\approx 10^{6}\,M_{\odot}\,Mpc^{-3}$) of massive galaxies (stellar masses $M_*\geq 10^{10.5}M_{\odot}$) at extremely high…

宇宙学与河外天体物理 · 物理学 2022-10-26 N. Menci , M. Castellano , P. Santini , E. Merlin , A. Fontana , F. Shankar

We propose a novel use of high-redshift galaxies, discovered in deep Hubble Space Telescope (HST) fields around strong lensing clusters. These fields probe small comoving volumes (about 1000 cubic Mpc) at high magnification ({\mu} > 10),…

宇宙学与河外天体物理 · 物理学 2013-08-15 Fabio Pacucci , Andrei Mesinger , Zoltan Haiman

We exploit the recent {\it James Webb Space Telescope} (JWST) determination of galaxy UV luminosity functions over the redshift range $z=9-14.5$ to derive constraints on warm dark matter (WDM) models. The delayed structure formation in WDM…

宇宙学与河外天体物理 · 物理学 2024-05-22 Bin Liu , Huanyuan Shan , Jiajun Zhang

Recent JWST observations of very early galaxies, at $\rm{z \gtrsim 10}$, have led to claims that tension exists between the sizes and luminosities of high-redshift galaxies and what is predicted by standard $\Lambda$CDM models. Here we use…

宇宙学与河外天体物理 · 物理学 2025-11-26 Hannah O'Brennan , John A. Regan , Chris Power , Saoirse Ward , John Brennan , Joe McCaffrey

The distribution of dark matter halo masses can be accurately predicted in the $\Lambda$CDM cosmology. The presence of a single massive halo or galaxy at a particular redshift, assuming some baryon and stellar fraction for the latter, can…

星系天体物理 · 物理学 2022-11-30 Christopher C. Lovell , Ian Harrison , Yuichi Harikane , Sandro Tacchella , Stephen M. Wilkins

We use a high resolution $\Lambda$CDM numerical simulation to calculate the mass function of dark matter haloes down to the scale of dwarf galaxies, back to a redshift of fifteen, in a 50 $h^{-1}$Mpc volume containing 80 million particles.…

天体物理学 · 物理学 2008-11-26 Darren Reed , Jeffrey Gardner , Thomas Quinn , Joachim Stadel , Mark Fardal , George Lake , Fabio Governato

The early-science observations made by the James Webb Space Telescope (JWST) have revealed an excess of ultra-massive galaxy candidates that appear to challenge the standard cosmological model ($\Lambda$CDM). Here, we argue that any…

宇宙学与河外天体物理 · 物理学 2024-02-14 Nashwan Sabti , Julian B. Muñoz , Marc Kamionkowski

The presence of massive galaxies at high $z$ as recently observed by JWST appears to contradict the current $\Lambda$CDM cosmology. Here we aim to alleviate this tension by incorporating uncertainties from three sources in counting…

星系天体物理 · 物理学 2025-04-08 Yangyao Chen , H. J. Mo , Kai Wang

With the advent of JWST, we can probe the rest-frame optical emission of galaxies at $z>3$ with high sensitivity and spatial resolution, making it possible to accurately characterise red, optically-faint galaxies and thus move towards a…

Warm Dark Matter (WDM) particles with masses ($\sim$ kilo electronvolt) offer an attractive solution to the small-scale issues faced by the Cold Dark Matter (CDM) paradigm. The delay of structure formation in WDM models and the associated…

宇宙学与河外天体物理 · 物理学 2024-01-11 Pratika Dayal , Sambit K. Giri

Early data from JWST have revealed a bevy of high-redshift galaxy candidates with unexpectedly high stellar masses. An immediate concern is the consistency of these candidates with galaxy formation in the standard cosmological model. In the…

宇宙学与河外天体物理 · 物理学 2023-06-22 Michael Boylan-Kolchin

The long-anticipated James Webb Space Telescope (JWST) will be able to directly detect large samples of galaxies at very high redshift. Using the well-established, computationally efficient Santa Cruz semi-analytic model, with recently…

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