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相关论文: Solution of JWST and HST problems by primordial bl…

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Recent data released by James Webb Space Telescope (JWST) and, somewhat earlier, the data presented by Hubble Space Telescope (HST) are commonly understood as a strong indication for breaking of the canonical $\Lambda$CDM cosmology. It is…

宇宙学与河外天体物理 · 物理学 2025-08-13 A. D. Dolgov

It is argued that the data presented by Hubble Space Telescope and James Webb Space Telescope, that seem to be at odds with the canonical big bang cosmology, find simple explanation if galaxy formation is seeded by massive primordial black…

宇宙学与河外天体物理 · 物理学 2023-04-07 A. D. Dolgov

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

A group of massive galaxies at redshifts of $z\gtrsim 7$ have been recently detected by the James Webb Space Telescope (JWST), which were unexpected to form so early within the framework of standard Big Bang cosmology. In this work, we…

宇宙学与河外天体物理 · 物理学 2024-08-13 Guan-Wen Yuan , Lei Lei , Yuan-Zhu Wang , Bo Wang , Yi-Ying Wang , Chao Chen , Zhao-Qiang Shen , Yi-Fu Cai , Yi-Zhong Fan

Recent observations from the James Webb Space Telescope have identified a population of massive galaxy sources ($\mathrm{>10^{10}\ M_\odot}$) at $z>7-10$, formed less than 700 Myr after the Big Bang. Such massive galaxies do not have enough…

广义相对论与量子宇宙学 · 物理学 2023-12-25 A. A. Coley

The James Webb Space Telescope (JWST) has unearthed black holes as massive as $10^{6.2-8.1}M_\odot$ at redshifts of $z \sim 8.5-10.6$ with many systems showing unexpectedly high black hole to stellar mass ratios >=30%, posing a crucial…

星系天体物理 · 物理学 2024-10-09 Pratika Dayal

Observations with the James Webb Space Telescope (JWST) have identified an abundant population of supermassive black holes (SMBHs) already in place during the first few hundred million years of cosmic history. Most of them appear…

The presence of supermassive black holes (SMBHs) at high redshifts ($z>5$), as revealed by James Webb Space Telescope (JWST), challenges standard black hole (BH) formation scenarios. We propose a mechanism in which non-annihilating dark…

高能物理 - 唯象学 · 物理学 2026-01-05 Sulagna Bhattacharya , Debajit Bose , Basudeb Dasgupta , Jaya Doliya , Ranjan Laha

The high redshift ($z>10$) galaxies GHZ9 and UHZ1 observed by the James Webb Space Telescope (JWST) are very massive and have exceptionally high black hole-to-star mass ratios with the central black hole masses $M\gtrsim 10^7\rm~M_\odot$.…

星系天体物理 · 物理学 2024-10-10 Hai-Long Huang , Yu-Tong Wang , Yun-Song Piao

The James Webb Space Telescope (JWST) has begun to revolutionize our view of the Cosmos. The discovery of Blue Monsters (i.e., ultra-compact yet very bright high-z galaxies) and the Little Red Dots (i.e., very compact dustless strong Balmer…

星系天体物理 · 物理学 2026-01-07 Cosmin Ilie , Jillian Paulin , Andreea Petric , Katherine Freese

In this paper, we show that the initial clustering of supermassive primordial black holes (SMPBHs) beyond a Poisson distribution can efficiently enhance the matter power spectrum, and thus the halo mass function. As a result, the population…

宇宙学与河外天体物理 · 物理学 2024-07-23 Hai-Long Huang , Jun-Qian Jiang , Yun-Song Piao

The origin of supermassive black holes (SMBHs) remains a long-standing problem in astrophysics. Recent JWST observations reveal an unexpectedly abundant population of overmassive black holes at z>4-6, where the BH masses lie far above local…

星系天体物理 · 物理学 2026-01-09 Sunmyon Chon , Shingo Hirano , Tomoaki Ishiyama , Seok-Jun Chang , Volker Springel

A review of the astronomical data of several last years on an astonishingly high amount of black holes in the contemporary and early ($z\sim 10$) universe is presented. Also the data on the recently observed peculiar stars in the Galaxy are…

宇宙学与河外天体物理 · 物理学 2019-11-07 A. D. Dolgov

It is argued that the bulk of black holes (BH) in the universe are primordial (PBH). This assertion is strongly supported by the recent astronomical observations, which allow to conclude that supermassive BHs with $M= (10^6 - 10^9) M_\odot$…

宇宙学与河外天体物理 · 物理学 2017-12-27 A. D. Dolgov

This Letter explores the potential role of primordial black holes (PBHs) to address cosmological tensions as the presence of more massive than expected galaxies at high redshifts, as indicated by recent James Webb Space Telescope…

宇宙学与河外天体物理 · 物理学 2024-04-23 P. E. Colazo , F. Stasyszyn , N. Padilla

JWST has revealed the apparent evolution of the black hole (BH)-stellar mass ($M_\mathrm{BH}$-$M_\rm{\ast}$) relation in the early Universe, while remaining consistent with the BH-dynamical mass ($M_\mathrm{BH}$-$M_\mathrm{dyn}$) relation.…

It has long been suggested that a fraction of the dark matter in the Universe could exist in the form of primordial black holes (PBHs) that have existed since the radiation dominated era. Recent studies have suggested that these PBHs may be…

星系天体物理 · 物理学 2025-09-03 Lewis R. Prole , John A. Regan , Daxal Mehta , Peter Coles , Pratika Dayal

Recent observations with JWST have identified several bright galaxy candidates at $z\gtrsim 10$, some of which appear unusually massive (up to $\sim 10^{11}\ \rm M_{\odot}$). Such early formation of massive galaxies is difficult to…

宇宙学与河外天体物理 · 物理学 2022-10-05 Boyuan Liu , Volker Bromm

Next-generation ground-based gravitational wave (GW) detectors are expected to observe millions of binary black hole mergers, a fraction of which will be strongly lensed by intervening galaxies or clusters, producing multiple images with…

宇宙学与河外天体物理 · 物理学 2026-01-16 Huan Zhou , Bin Liu , Zheng-Xiang Li , Xi-Jing Wang , Kai Liao

A brief review of the recent astronomical data, indicating that the universe is abundantly populated by heavy black holes (BH), is presented. Conventional astrophysics and cosmology cannot explain such a high population of BHs. A mechanism…

宇宙学与河外天体物理 · 物理学 2018-12-05 A. D. Dolgov
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