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Future Probes of Cosmology and the High-Redshift Universe

This thesis is a study in theoretical cosmology with an emphasis on the high-redshift universe and promising directions for future observations. In Chapters 2 and 3, we propose intensity mapping of spectral line emission from galaxies. This is a technique to observe the cumulative emission from many galaxies without resolving individual sources. We use analytic calculations and N-body simulations to predict the observational signal for different emission lines, including those from oxygen, carbon monoxide, and carbon. / Physics

Identiferoai:union.ndltd.org:harvard.edu/oai:dash.harvard.edu:1/11158272
Date09 October 2013
CreatorsVisbal, Elijah Francis
ContributorsLoeb, Abraham
PublisherHarvard University
Source SetsHarvard University
Languageen_US
Detected LanguageEnglish
TypeThesis or Dissertation
Rightsopen

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