activity
20242026
most citedLyman- feedback prevails at Cosmic Dawn: Implications for the first galaxies, stars, and star clusters

16 citations · 22 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

Force convergence in Monte Carlo Lyman-alpha radiative transfer

Joshua Kasiri, Aaron Smith, Kevin Lorinc +2

Monte Carlo radiative transfer (MCRT) is widely used to model Lyman-alpha (Lya) resonant-line transport, but convergence is difficult to assess in optically thick media where photo…

astro-ph.GA2026

Lyman-alpha Pressure Strongly Enhances Pre-Supernova Feedback at Cosmic Dawn: The First Multi-Dimensional Lyman-alpha Radiation Hydrodynamics Simulations

Olof Nebrin, Aaron Smith, Garrelt Mellema +2

The dynamical role of Lyman- (Ly) radiation pressure feedback has been debated for nearly a century, with recent analytical and 1D numerical studies highlighting its potentia…

astro-ph.GA2026

Lyman-alpha Radiation Pressure in Dense Star Clusters: Implications for Star Formation and Winds at Cosmic Dawn

Shyam H Menon, Aaron Smith

Observations with the JWST in lensed fields have revealed that galaxies at cosmic dawn may concentrate their star formation in highly dense, compact, star clusters. The high column…

astro-ph.CO2026★ 1 cited

Double-Peaked Ly Emission during Reionization Requires Nearby Voids and a Favorable Local Ionizing Background

Hyunbae Park, Aaron Smith, Intae Jung +11

Several Lyman-alpha (Ly) emitters deep into the reionization era exhibit double-peaked Ly emission profiles, raising the question of how the intergalactic medium can transmit…

astro-ph.GA2025

Core-wing transitions and the breakdown of diffusion in Lyman- radiative transfer

Kevin Lorinc, Aaron Smith, Olof Nebrin +1

The Lyman alpha (LyA) line of neutral hydrogen plays a central role in observations of star-forming galaxies. However, resonant scattering makes it difficult to directly interpret…

astro-ph.CO2025

The THESAN project: Lyman-alpha intensity mapping of cosmic reionization

Mouza Almualla, Aaron Smith, Rahul Kannan +6

Line Intensity Mapping (LIM) has garnered attention as a powerful cosmological probe, with next-generation instruments such as SPHEREx preparing to map the evolution of large-scale…

astro-ph.GA2025

Multi-Resonant-Line Radiative Transfer: Lyman-Alpha Fine Structure and Deuterium Coupling

Ethan Stace, Aaron Smith, Kevin Lorinc +1

Resonance lines encode rich information about astrophysical sources and their environments, yet fully analytic treatments of multi-line radiative transfer remain almost entirely un…

astro-ph.GA2025★ 5 cited

Lyman-alpha resonant-line radiative transfer in expanding media

Aaron Smith, Kevin Lorinc, Olof Nebrin +1

The Lyman-alpha (LyA) line of atomic hydrogen encodes crucial information about both the intrinsic sources and surrounding environments of star-forming regions throughout the Unive…

astro-ph.CO2024

Cosmic Ly Emission from Diffuse Gas

Sung-Han Tsai, Ke-Jung Chen, Aaron Smith +1

The Ly emission has emerged as a powerful tool for probing diffuse gas within the large-scale structure of the universe. In this paper, we investigate cosmic Ly emission by p…

astro-ph.GA2024★ 16 cited

Lyman- feedback prevails at Cosmic Dawn: Implications for the first galaxies, stars, and star clusters

Olof Nebrin, Aaron Smith, Kevin Lorinc +4

Radiation pressure from Lyman- (Ly) scattering is a potentially dominant form of early stellar feedback, capable of injecting up to more momentum into th…