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by
Dietrich, Phillip, author.
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Comparing Core Collapse Supernovae Models with Observations / Dietrich, Phillip, author.
by
Miles, Broxton, author.
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Type Ia Supernovae and Improving Detonation Models of Sub-Chandrasekhar Mass Type Ia Supernovae / Miles
by
Fang, Yuedong, author.
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Two-Point Statistics for Testing Models of Cosmic Structure / Fang, Yuedong, author.
by
Lewis, Tiffany R., author. (orcid)0000-0002-9854-1432
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Self-Consistent Physical Models for Blazar Jet Emission: Time Lags and Spectra for Mrk 421 & 3C 279 /
by
Susskind, Leonard, author.
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String models.
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Breivik, Katelyn, author. (orcid)0000-0001-5228-6598
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, theoretical models must be characterized to gain a fuller understanding of the underlying physics governing
by
Loutrel, Nicholas Peter, author.
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systems has been a long outstanding problem in astrophysics and relativity. Astrophysical models predict
by
Young, Edward, author.
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Gravitational waves are a prediction of many early Universe models. These waves generate a
by
Nhan, Bang D., author.
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foreground spectrum directly, without relying on any parametric foreground models as in conventional
by
Frazer, Christopher Charles, author.
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expected to disrupt any potentially star forming gas in its vicinity. Yet, numerical models indicate that
by
Holmes, Justin C., author. (orcid)0000-0002-5414-8604
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, solitary waves defy our expectations based on ideal physical models. In one instance, a type of solitary
by
Christie, Ian, author.
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origin of the gas remain elusive. Here, I explore several models for indirectly probing the properties of

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