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20182026
most citedHydrodynamic Response of the Intergalactic Medium to Reionization

68 citations · 296 across the 28 of their papers we have counts for

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24 papers · 1 filter

astro-ph.CO2026

Constraints on Reionization from Planck Low- EE Polarization and the Lyman-Series Forests

Garett Lopez, Anson D'Aloisio, Christopher Cain

CMB measurements tightly constrain the Thomson scattering optical depth (), but they still permit a broad range of degenerate reionization histories. Incorporating Lyma…

astro-ph.CO2026

The Atacama Cosmology Telescope: Constraints on the anisotropic screening and birefringence effects with DR6

Darby M. Kramer, Alexander van Engelen, Frank J. Qu +14

While we have learned much from recent surveys of the mm-wave sky, many secondary anisotropies of the CMB remain under-explored. We consider two of these here: the anisotropic scre…

astro-ph.CO2026

Characterising the epoch of reionisation using the cross-correlation of the kSZ effect and CMB lensing

Niall MacCrann, Christopher Cain, Aleksandra Kusiak +5

We investigate the cross-correlation of the kinematic Sunyaev-Zeldovich (kSZ) effect with lensing of the cosmic microwave background (CMB) as a probe of the epoch of reionisation.…

astro-ph.CO2026

Fireworks at Cosmic Dawn: relieving BAO-CMB tensions with the Pop III.1 Flash

Yash Aggarwal, Christopher Cain, Garett Lopez +4

A Cosmic Microwave Background (CMB) optical depth of , several in excess of the latest Planck low- EE polarization measurement, has been proposed as a way to…

astro-ph.CO2026

A self-consistent analytical model for both the photoionization rate and reionization history

Christopher Cain, Kevin S. Croker, Anson D'Aloisio +4

Recent developments at the intersection of cosmology and astrophysics have highlighted the need for improved analytical models of observables that probe the Epoch of Reionization.…

astro-ph.CO2026★ 1 cited

An emulator for the ionizing photon mean free path in ultra-high resolution simulations: the implications of mean free path measurements for the reionization history

Hurum Maksora Tohfa, Christopher Cain, Matthew McQuinn +1

Measurements of the mean free path of ionizing photons from high-redshift quasar spectra at - constrain the reionization history, but interpreting them requires modeli…

astro-ph.CO2025

Probing the ionizing photon output of galaxies near cosmic dawn with the patchy kSZ effect

Garett Lopez, Anson D'Aloisio, Christopher Cain

A key result from JWST's first cycles is that galaxy formation was well underway by . The implications of these early galaxies for reionization are less clear, however. The C…

astro-ph.CO2025

The CMB optical depth constrains the duration of reionization

Christopher Cain, Alexander Van Engelen, Kevin S. Croker +3

Recently, it was pointed out that invoking a large value of the CMB optical depth, , could help resolve tensions between DESI DR2 BAO data and the CMB. This is…

astro-ph.CO2025★ 1 cited

Kiloparsec-scale turbulence driven by reionization may grow intergalactic magnetic fields

Christopher Cain, Matthew McQuinn, Evan Scannapieco +2

The intergalactic medium (IGM) underwent intense heating that resulted in pressure disequilibrium in the wake of ionization fronts during cosmic reionization. The dynamical relaxat…

astro-ph.CO2025★ 1 cited

Cross-correlating the patchy screening and kinetic Sunyaev-Zel'dovich effects as a new probe of reionization

Darby Kramer, Alexander van Engelen, Christopher Cain +5

The kinetic Sunyaev-Zel'dovich effect (kSZ) and patchy screening effect are two complementary cosmic microwave background (CMB) probes of the reionization era. The kSZ effect is a…

astro-ph.CO2024★ 1 cited

FlexRT -- A fast and flexible cosmological radiative transfer code for reionization studies I: Code validation

Christopher Cain, Anson D'Aloisio

The wealth of high-quality observational data from the epoch of reionization that will become available in the next decade motivates further development of modeling techniques for…

astro-ph.CO2024★ 3 cited

Chasing the beginning of reionization in the JWST era

Christopher Cain, Garett Lopez, Anson D'Aloisio +4

Recent JWST observations at may imply galactic ionizing photon production above prior expectations. Under observationally motivated assumptions about escape fractions, thes…

astro-ph.CO2024★ 1 cited

On the correlation between Ly forest opacity and galaxy density in late reionization models

Nakul Gangolli, Anson D'Aloisio, Christopher Cain +2

The relationship between Ly forest opacity and local galaxy density (the opacity-density relation) is a key observational test of late reionization models. Using narrow-band sur…

astro-ph.CO2024★ 1 cited

Quantifying Lyman- emissions from reionization fronts

Bayu Wilson, Anson D'Aloisio, Christopher Cain +2

During reionization, intergalactic ionization fronts (I-fronts) are sources of Ly line radiation produced by collisional excitation of hydrogen atoms within the fronts. In princ…

astro-ph.CO2024

The hydrodynamic response of small-scale structure to reionization drives large IGM temperature fluctuations that persist to z = 4

Christopher Cain, Evan Scannapieco, Matthew McQuinn +2

The thermal history and structure of the intergalactic medium (IGM) at is an important boundary condition for reionization, and a key input for studies using the Ly f…

astro-ph.CO2023★ 1 cited

On the rise and fall of galactic ionizing output at the end of reionization

Christopher Cain, Anson D'Aloisio, Garett Lopez +2

Quasar absorption spectra measurements suggest that reionization proceeded rapidly, ended late at , and was followed by a flat ionizing background evolution. Simulation…

astro-ph.CO2023★ 1 cited

The effect of reionization on direct measurements of the mean free path

Joshua T. Roth, Anson D'Aloisio, Christopher Cain +3

Recent measurements of the ionizing photon mean free path (MFP) based on composite quasar spectra may point to reionization ending at . These measurements are challenging beca…

astro-ph.CO2023★ 2 cited

Probing Ultra-late Reionization: Direct Measurements of the Mean Free Path over

Yongda Zhu, George D. Becker, Holly M. Christenson +22

The mean free path of ionizing photons, , is a critical parameter for modeling the intergalactic medium (IGM) both during and after reionization. We present direct mea…

astro-ph.CO2022★ 23 cited

The Morphology of Reionization in a Dynamically Clumpy Universe

Christopher Cain, Anson D'Aloisio, Nakul Gangolli +1

A recent measurement of the Lyman-limit mean free path at suggests it may have been very short, motivating a better understanding of the role that ionizing photon sinks pla…

astro-ph.CO2022★ 8 cited

Small-scale clumping of dark matter and the mean free path of ionizing photons at

Christopher Cain, Anson D'Aloisio, Vid Irsic +2

Recently, the mean free path of ionizing photons in the intergalactic medium (IGM) was measured to be very short, presenting a challenge to existing reionization models. At…

astro-ph.CO2021★ 26 cited

Hydrodynamic Response of the Intergalactic Medium to Reionization II: Physical Characteristics and Dynamics of Ionizing Photon Sinks

Fahad Nasir, Christopher Cain, Anson D'Aloisio +2

Becker et al. 2021 measured the mean free path of Lyman limit photons in the IGM at . The short value suggests that absorptions may have played a prominent role in reionizatio…

astro-ph.CO2021★ 67 cited

A short mean free path at favors late and rapid reionization by faint galaxies

Christopher Cain, Anson D'Aloisio, Nakul Gangolli +1

Recent measurements of the ionizing photon mean free path () at suggest that the IGM was rapidly evolving at those times. We use radiative transfer s…

astro-ph.CO2020★ 17 cited

A Model-Insensitive Baryon Acoustic Oscillation Feature in the 21 cm Signal from Reionization

Christopher Cain, Anson D'Aloisio, Vid Iršič +2

We examine the impact of baryon-dark matter relative velocities on intergalactic small-scale structure and the 21 cm signal during reionization. Streaming velocities reduced clumpi…

astro-ph.CO2020★ 68 cited

Hydrodynamic Response of the Intergalactic Medium to Reionization

Anson D'Aloisio, Matthew McQuinn, Hy Trac +2

The intergalactic medium is expected to clump on scales down to M before the onset of reionization. The impact of these small-scale structures on reionization…