Exascale applications: skin in the game

F Alexander, A Almgren, J Bell… - … of the Royal …, 2020 - royalsocietypublishing.org
As noted in Wikipedia, skin in the game refers to having 'incurred risk by being involved in
achieving a goal', where 'skin is a synecdoche for the person involved, and game is the …

A survey of high level frameworks in block-structured adaptive mesh refinement packages

A Dubey, A Almgren, J Bell, M Berzins, S Brandt… - Journal of Parallel and …, 2014 - Elsevier
Over the last decade block-structured adaptive mesh refinement (SAMR) has found
increasing use in large, publicly available codes and frameworks. SAMR frameworks have …

Hydrogen reionization ends by z = 5.3: Lyman-α optical depth measured by the XQR-30 sample

SEI Bosman, FB Davies, GD Becker… - Monthly Notices of …, 2022 - academic.oup.com
The presence of excess scatter in the Ly-α forest at z∼ 5.5, together with the existence of
sporadic extended opaque Gunn-Peterson troughs, has started to provide robust evidence …

Simulating cosmic structure formation with the gadget-4 code

V Springel, R Pakmor, O Zier… - Monthly Notices of the …, 2021 - academic.oup.com
Numerical methods have become a powerful tool for research in astrophysics, but their utility
depends critically on the availability of suitable simulation codes. This calls for continuous …

XQR-30: The ultimate XSHOOTER quasar sample at the reionization epoch

V D'Odorico, E Bañados, GD Becker… - Monthly Notices of …, 2023 - academic.oup.com
The final phase of the reionization process can be probed by rest-frame UV absorption
spectra of quasars at z≳ 6, shedding light on the properties of the diffuse intergalactic …

Quantitative constraints on the reionization history from the IGM dam** wing signature in two quasars at z> 7

FB Davies, JF Hennawi, E Bañados… - The Astrophysical …, 2018 - iopscience.iop.org
During reionization, neutral hydrogen in the intergalactic medium (IGM) imprints a dam**
wing absorption feature on the spectrum of high-redshift quasars. A detection of this …

Enzo: An adaptive mesh refinement code for astrophysics

GL Bryan, ML Norman, BW O'Shea… - The Astrophysical …, 2014 - iopscience.iop.org
This paper describes the open-source code Enzo, which uses block-structured adaptive
mesh refinement to provide high spatial and temporal resolution for modeling astrophysical …

A Significantly Neutral Intergalactic Medium Around the Luminous z= 7 Quasar J0252–0503

F Wang, FB Davies, J Yang, JF Hennawi… - The Astrophysical …, 2020 - iopscience.iop.org
Luminous z≥ 7 quasars provide direct probes of the evolution of supermassive black holes
(SMBHs) and the intergalactic medium (IGM) during the epoch of reionization (EoR). The …

Measurements of the z∼ 6 Intergalactic Medium Optical Depth and Transmission Spikes Using a New z> 6.3 Quasar Sample

J Yang, F Wang, X Fan, JF Hennawi… - The Astrophysical …, 2020 - iopscience.iop.org
We report new measurements of the intergalactic medium (IGM) Lyα and Lyβ effective
optical depth at 5.3< z< 6.5, using a new sample of quasar sight lines including 32 quasars …

Simulations of solitonic core mergers in ultralight axion dark matter cosmologies

B Schwabe, JC Niemeyer, JF Engels - Physical Review D, 2016 - APS
Using three-dimensional simulations, we study the dynamics and final structure of merging
solitonic cores predicted to form in ultralight axion dark matter halos. The classical …