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相关论文: Beasts in Lambda-CDM Zoo

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Recent discoveries of apparent large-scale features in the structure of the universe, extending over many hundreds of megaparsecs, have been claimed to contradict the large-scale isotropy and homogeneity foundational to the standard…

宇宙学与河外天体物理 · 物理学 2025-02-07 Till Sawala , Meri Teeriaho , Carlos S. Frenk , John Helly , Adrian Jenkins , Gabor Racz , Matthieu Schaller , Joop Schaye

The JWST discovery of a number of super-early (redshift $z>10$), blue galaxies requires these systems to be essentially dust-free in spite of their large stellar masses. A possible explanation is that dust is evacuated by radiatively-driven…

星系天体物理 · 物理学 2023-02-08 Fabrizio Fiore , Andrea Ferrara , Manuela Bischetti , Chiara Feruglio , Andrea Travascio

There has been remarkable progress recently in both observational and theoretical studies of galaxy formation and evolution. Largely due to a combination of deep Hubble Space Telescope imaging, Keck spectroscopy, and COBE far-IR background…

天体物理学 · 物理学 2007-05-23 Piero Madau

Under the assumption that General Relativity (GR) correctly describes the phenomenology of our Universe, astronomical observations provide compelling evidence that (1) the dynamics of cosmic structure is dominated by dark matter (DM), an…

天体物理学 · 物理学 2008-02-19 A. Diaferio

Observations from the James Webb Space Telescope (JWST) have uncovered supermassive black holes (SMBHs) with masses exceeding $10^6 \mathrm{M}_{\odot}$ at redshifts $z > 8$, posing significant challenges to existing models of early black…

星系天体物理 · 物理学 2026-01-22 Daxal H. Mehta , John A. Regan , Lewis Prole

Dark matter represents currently an outstanding problem in both cosmology and particle physics. In this review we discuss the possible explanations for dark matter and the experimental observables which can eventually lead to the discovery…

高能物理 - 唯象学 · 物理学 2021-04-26 A. Arbey , F. Mahmoudi

A possibility of existence of ultra-heavy (quasi)stable particles, mechanisms leading to their large life-time, their production in the early universe, and cosmological manifestations are reviewed.

高能物理 - 唯象学 · 物理学 2007-05-23 A. D. Dolgov

Recent observations suggest appreciable star formation activity in early-type galaxies down to redshift $z\sim 0.5$. If so, there is likely to be dust in these galaxies. We consider the possibility that obscuration by dust can reconcile the…

天体物理学 · 物理学 2007-05-23 M. Fukugita , P. J. E. Peebles

The evolution of marginally bound supercluster-like objects in an accelerating LambdaCDM Universe is followed, by means of cosmological simulations, from the present time to an expansion factor a = 100. The objects are identified on the…

We present results of cosmological N-body hydrodynamic chemistry simulations of primordial structure growth and evolution in a scenario with warm dark matter (WDM) having a mass of 3 keV (thermal relic) and compare with a model consisting…

宇宙学与河外天体物理 · 物理学 2015-06-23 Umberto Maio , Matteo Viel

The James Webb Space Telescope has recently detected massive, fully formed, galaxies at redshifts corresponding to few hundred million years after the Big-Bang. However, our current cosmological model cannot produce such massive systems so…

广义相对论与量子宇宙学 · 物理学 2025-11-26 Christos G. Tsagas

We show that seeds for quasar black holes could have originated from the initial cosmological collapse of overdense regions with unusually small rotation. The gas in these rare regions collapses into a compact disk that shrinks on a short…

天体物理学 · 物理学 2009-09-25 Daniel J. Eisenstein , Abraham Loeb

JWST's recent discovery of well-formed galaxies and supermassive black holes only a few hundred Myr after the big bang seriously challenges the timeline predicted by $\Lambda$CDM. Now, the latest identification of polycyclic aromatic…

宇宙学与河外天体物理 · 物理学 2024-07-23 Fulvio Melia

In the last decades, luminous accreting super-massive black holes have been discovered within the first Gyr after the Big Bang, but their origin is still an unsolved mystery. We discuss our state-of-the-art theoretical knowledge of their…

星系天体物理 · 物理学 2023-05-24 Elisabeta Lusso , Rosa Valiante , Fabio Vito

Several arguments suggest that quasars at z > 4 may be in the cores of future giant ellipticals, and forming at the very highest peaks of the primordial density field. A strong bias-driven primordial clustering is then expected in these…

天体物理学 · 物理学 2007-05-23 S. G. Djorgovski

High-redshift quasars ($z\gtrsim6$), powered by black holes (BHs) with large inferred masses, imply rapid BH growth in the early Universe. The most extreme examples have inferred masses of $\sim \! 10^9\,$M$_\odot$ at $z = 7.5$ and $\sim \!…

星系天体物理 · 物理学 2023-11-09 Jake S. Bennett , Debora Sijacki , Tiago Costa , Nicolas Laporte , Callum Witten

The James Webb Space Telescope (JWST) is challenging our understanding of the nature of the very first galaxies in the Universe, having discovered a surprising abundance of very massive galaxies in early cosmic epochs. By applying a model…

星系天体物理 · 物理学 2025-04-03 Maria Emilia De Rossi , Volker Bromm

One of the possible explanations for dark matter is that of compact dark objects of baryonic origin, such as black holes or even planets. Accumulating evidence, including the discovery of merging stellar mass black holes through…

宇宙学与河外天体物理 · 物理学 2025-07-04 Georgios Vernardos , James Hung Hsu Chan , Frederic Courbin

It is currently unknown whether the Universe was reionized by quasars or stars at z>5. We point out that quasars can be best distinguished from stellar systems by their X-ray emission. Based on a simple hierarchical CDM model, we predict…

天体物理学 · 物理学 2009-10-31 Zoltan Haiman , Abraham Loeb