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The James Webb Space Telescope (JWST) has discovered a new population of objects, the Little Red Dots (LRDs), characterized by V-shaped spectra indicative of strong breaks around the Balmer limit and compact morphology that gave them their…

The discovery by JWST of a substantial population of compact "Little Red Dots" (LRDs) presents a major puzzle: their observed spectra defy standard astrophysical interpretations. Here, we show that LRD spectra are naturally reproduced by…

星系天体物理 · 物理学 2026-01-22 Fabio Pacucci , Andrea Ferrara , Dale D. Kocevski

The James Webb Space Telescope has detected massive black holes (BHs) with masses of $\sim 10^{6-8}~M_\odot$ within the first billion years of the universe. One of the remarkable findings is the identification of "Little Red Dots" (LRDs), a…

星系天体物理 · 物理学 2025-07-17 Kohei Inayoshi

The James Webb Space Telescope (JWST) has revealed a previously unknown population of compact, red galaxies at $z \sim 5$, known as "Little Red Dots" (LRDs). With effective radii of $\sim 100$ pc and stellar masses of $10^9-10^{11} \,…

星系天体物理 · 物理学 2025-11-14 Fabio Pacucci , Lars Hernquist , Michiko Fujii

The rapid emergence of supermassive black holes (SMBHs) in the early Universe poses a challenge to current models of black hole growth. One promising formation pathway is the direct collapse black hole (DCBH) scenario, in which gas in…

The James Webb Space Telescope (JWST) observations have identified a class of compact galaxies at high redshifts ($4 \lesssim z \lesssim 11$), dubbed "little red dots" (LRDs). The supermassive black holes (SMBHs) of…

宇宙学与河外天体物理 · 物理学 2025-07-24 Borui Zhang , Wei-Xiang Feng , Haipeng An

The James Webb Space Telescope (JWST) has uncovered a population of compact, high-redshift sources, the Little Red Dots (LRDs), which may host supermassive black holes (BHs) significantly heavier than their stellar content compared with…

宇宙学与河外天体物理 · 物理学 2025-12-23 Valerio De Luca , Loris Del Grosso , Gabriele Franciolini , Konstantinos Kritos , Emanuele Berti , Daniel D'Orazio , Joseph Silk

Observations of high-redshift quasars indicate that super massive black holes (SMBHs) with masses greater than ${\sim}10^9~M_\odot$ were assembled within the first billion years after the Big Bang. It is unclear how such massive black holes…

星系天体物理 · 物理学 2018-09-26 Eli Visbal , Zoltan Haiman

We investigate the possibility that the recently identified population of high-redshift, obscured quasars - known as "Little Red Dots" (LRDs) - originates from early black hole seed formation driven by ultra-strongly self-interacting dark…

星系天体物理 · 物理学 2026-03-10 M. Grant Roberts , Lila Braff , Aarna Garg , Stefano Profumo , Tesla Jeltema

The existence of massive, compact galaxies (Little Red Dots, LRDs) at $z \sim 2$ challenges early structure formation models, suggesting rapid stellar and black hole (BH) assembly. While LRDs are efficient environments for BH growth, many…

星系天体物理 · 物理学 2026-04-01 M. Liempi , D. R. G. Schleicher , M. A. Latif , R. Schneider , F. Flammini Dotti , A. Escala , M. C. Vergara

Direct-collapse black holes (DCBHs) are currently one of the leading contenders for the origins of the first quasars in the universe, over 300 of which have now been found at $z >$ 6. But the birth of a DCBH in an atomically-cooling halo…

Little Red Dots (LRDs) are a newly identified class of active galactic nuclei (AGNs) uncovered by JWST deep surveys. Their enigmatic properties challenge the canonical AGN paradigm and have stimulated ideas on early massive black hole (BH)…

星系天体物理 · 物理学 2025-12-04 Kohei Inayoshi , Luis C. Ho

Since the launch of James Webb Space Telescope (JWST) in late 2021, our understanding of high-redshift objects has faced several upheavals. JWST has discovered much more massive galaxies and supermassive black holes (SMBH) than cosmological…

星系天体物理 · 物理学 2026-01-05 David D Vaida , Ryan Jeffrey Farber

The James Webb Space Telescope (JWST) has uncovered an abundant population of compact, extremely red, and X-ray weak objects at $z\gtrsim4$, knows as ``Little Red Dots" (LRDs). These objects exhibit spectral energy distributions that…

星系天体物理 · 物理学 2024-10-29 Hai-Long Huang , Jun-Qian Jiang , Jibin He , Yu-Tong Wang , Yun-Song Piao

Little red dots (LRDs) newly discovered with JWST are active galactic nuclei (AGN) that may represent black hole (BH) growth at the earliest cosmic epochs. These sources show puzzling features unlike typical AGNs, including red optical…

星系天体物理 · 物理学 2026-03-04 Hiroya Umeda , Kohei Inayoshi , Yuichi Harikane , Kohta Murase

We address the origin of the Little Red Dots (LRDs) seen by JWST at cosmic morning ($z \!=\! 4 \!-\! 8$) as compact stellar systems with over-massive black holes (BHs). We propose that LRDs form naturally after feedback-free starbursts…

Little Red Dots (LRDs), among the most enigmatic high-redshift discoveries by JWST, are commonly believed to be powered by accreting supermassive black holes. Here, we explore the possibility that these sources are globular clusters in…

JWST has revealed an abundant population of compact, low-metallicity "Little Red Dots" (LRDs) at high redshift, challenging conventional scenarios in which supermassive black holes (SMBHs) grow from stellar-mass seeds. We consider a…

高能物理 - 唯象学 · 物理学 2026-04-03 Jinhui Guo , Jia Liu , Masanori Tanaka , Xiao-Ping Wang , Huangyu Xiao

We present a statistical study of black hole (BH) formation and growth seeded by gravothermal core collapse of self-interacting dark matter (SIDM) halos at high redshift, using a cosmological semi-analytical framework based on Monte Carlo…

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