Chasing ancient demons : tools for measuring 21 cm fluctuations before reionization
Name
1029767890-MIT.pdf
Description
Full printable version
Size
46.48 MB
Format
Adobe PDF
Checksum (MD5)
28b9fa748502a045b28765d5370d0fc8
Author(s)
Ewall-Wice, Aaron
Advisor(s)
Jacqueline Hewitt.
Alternative Title
Tools for measuring 21 cm fluctuations before reionization
Date Issued
2017
Publisher
Massachusetts Institute of Technology
Abstract
In this thesis, we take the first steps towards measuring the fluctuations in HI emission before reionization which carry information on the first X-ray emitting compact objects and hot interstellar gas heated by the deaths of the first stars (ancient demons). First, we show that existing and planned interferometers are sensitive enough to place interesting constraints on the astrophysics of X-ray heating. Second, we obtain first upper limits on the pre-reionization fluctuations with the Murchison Widefield Array. We also use these measurements to explore the impact of low-frequency systematics, such as increased foreground brightness and the ionosphere. We discover that contamination by fine-scale frequency structure introduced by the instrument is the leading obstacle to measuring the 21 cm power spectrum before reionization. This motivates the design of a next-generation experiment, HERA, with acceptable levels of intrinsic spectral structure. We also perform a careful examination of whether traditional calibration strategies are sufficient to suppress instrumental spectral structure. We find that while existing calibration techniques have critical flaws, there exist promising strategies to overcome these deficiencies which we are now pursuing.
Description
Thesis: Ph. D., Massachusetts Institute of Technology, Department of Physics, 2017.
Cataloged from PDF version of thesis.
Includes bibliographical references (pages 379-428).
Subjects
Physics.
MIT Department
Massachusetts Institute of Technology. Department of Physics
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