Can Little Red Dots Contribute To The Early Universe Cosmic Dust Budget?
Abstract
The origin of dust in the early Universe remains uncertain. We explore whether Little Red Dots (LRDs) could provide a high-redshift dust-production channel. Motivated by an analogy with Type IIn supernovae, we investigate whether LRDs may share the efficient dust-forming conditions. We consider dust formation in outer winds and later in a shielded cold dense shell after the central source fades. Such dust may avoid a global remnant-phase reverse shock, while longer LRD lifetimes may promote grain growth. We model the SEDs of two low-redshift LRD analogs as a thermal pseudo-photosphere plus optically thin dust components, obtaining dust reservoirs of order 102-103 M⊙. Although photometry cannot exclude pre-existing dust, the narrow Balmer components of both analogs are close to the Case B ratio and their narrow-line environments are metal-poor, disfavoring a dominant diffuse host-ISM origin for the inferred reservoir. Formation within the LRD outflow is consistent with our optical-depth, sublimation, and energy-balance checks. In this scenario, the large dust masses do not produce a strong optical attenuation because a clumpy or asymmetric distribution can leave the dominant optical sightlines relatively unobscured. Our population calculation shows that the LRD contribution to early-Universe dust production can range from negligible to dominant. At higher efficiencies, LRDs can approach or exceed the lower CCSN contribution above z≈5, whereas less favorable assumptions yield a minor contribution. We therefore propose that LRDs can act as early-Universe dust factories and, under some conditions, may dominate over CCSNe or provide seed grains for subsequent growth in the early ISM.
Related
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BibTeX
@misc{ashall2026little,
title = {{Can Little Red Dots Contribute To The Early Universe Cosmic Dust Budget?}},
author = {Chris Ashall and Rohan P. Naidu and Alberto Torralba and Irene Shivaei and John Chisholm and Hanpu Liu and Zhaoran Liu and Jorryt Matthee and Kyle Medler and Tyco Mera and Takashi J. Moriya and Devesh Nandal and Robert A. Simcoe and Wendy Q. Sun},
howpublished = {arXiv},
year = {2026},
month = aug,
doi = {10.48550/arxiv.2608.29011},
eprint = {2608.29011},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2608.29011},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Can Little Red Dots Contribute To The Early Universe Cosmic Dust Budget?
AU - Chris Ashall
AU - Rohan P. Naidu
AU - Alberto Torralba
AU - Irene Shivaei
AU - John Chisholm
AU - Hanpu Liu
AU - Zhaoran Liu
AU - Jorryt Matthee
AU - Kyle Medler
AU - Tyco Mera
AU - Takashi J. Moriya
AU - Devesh Nandal
AU - Robert A. Simcoe
AU - Wendy Q. Sun
PY - 2026
DA - 2026/08/29
PB - arXiv
DO - 10.48550/arxiv.2608.29011
UR - https://arxiv.org/abs/2608.29011
AB - The origin of dust in the early Universe remains uncertain. We explore whether Little Red Dots (LRDs) could provide a high-redshift dust-production channel. Motivated by an analogy with Type IIn supernovae, we investigate whether LRDs may share the efficient dust-forming conditions. We consider dust formation in outer winds and later in a shielded cold dense shell after the central source fades. Such dust may avoid a global remnant-phase reverse shock, while longer LRD lifetimes may promote grain growth. We model the SEDs of two low-redshift LRD analogs as a thermal pseudo-photosphere plus optically thin dust components, obtaining dust reservoirs of order 10^2-10^3 M_⊙. Although photometry cannot exclude pre-existing dust, the narrow Balmer components of both analogs are close to the Case B ratio and their narrow-line environments are metal-poor, disfavoring a dominant diffuse host-ISM origin for the inferred reservoir. Formation within the LRD outflow is consistent with our optical-depth, sublimation, and energy-balance checks. In this scenario, the large dust masses do not produce a strong optical attenuation because a clumpy or asymmetric distribution can leave the dominant optical sightlines relatively unobscured. Our population calculation shows that the LRD contribution to early-Universe dust production can range from negligible to dominant. At higher efficiencies, LRDs can approach or exceed the lower CCSN contribution above z≈5, whereas less favorable assumptions yield a minor contribution. We therefore propose that LRDs can act as early-Universe dust factories and, under some conditions, may dominate over CCSNe or provide seed grains for subsequent growth in the early ISM.
ER -