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Reionization Through the Lens of Percolation Theory
Steven R. Furlanetto, S. Peng Oh
The reionization of intergalactic hydrogen has received intense theoretical scrutiny over the past two decades. Here, we approach the process formally as a percolation process and…
The Distribution of Bubble Sizes During Reionization
Yin Lin, S. Peng Oh, Steven R. Furlanetto +1
A key physical quantity during reionization is the size of HII regions. Previous studies found a characteristic bubble size which increases rapidly during reionization, with appare…
The [CII] Deficit in LIRGs and ULIRGs is Due to High-Temperature Saturation
Joseph A. Muñoz, S. Peng Oh
Current predictions for the line ratios from photo-dissociative regions (PDRs) in galaxies adopt theoretical models that consider only individual parcels of PDR gas each characteri…
Turbulence and Particle Acceleration in Giant Radio Halos: the Origin of Seed Electrons
Anders Pinzke, S. Peng Oh, Christoph Pfrommer
About 1/3 of X-ray-luminous clusters show smooth, unpolarized radio emission on ~Mpc scales, known as giant radio halos. One promising model for radio halos is Fermi-II acceleratio…