Category:Physical cosmology
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Physical cosmology is the study of the largest-scale structures and dynamics of the Universe and is concerned with fundamental questions about its origin, structure, evolution, and ultimate fate. The subject matter of this field is studied using scholarly methodology, including the scientific method and reason. It is studied by scientists, such as astronomers, and theoretical physicists; and academic philosophers, such as metaphysicians, philosophers of physics, and philosophers of space and time.
Subcategories
This category has the following 4 subcategories, out of 22 total.
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Pages in category "Physical cosmology"
The following 50 pages are in this category, out of approximately 260 total. This list may not reflect recent changes.
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- Sachs–Wolfe effect
- Scalar–tensor theory
- Scalar–vector–tensor decomposition
- Scale factor (cosmology)
- Self-indication assumption
- Self-sampling assumption
- Shape of the universe
- Sigma (cosmology)
- Sigma-D relation
- Source counts
- Static universe
- Steady-state model
- Stebbins–Whitford effect
- String cosmology
- String phenomenology
- String theory
- String theory landscape
- Structure formation
- Sunyaev–Zeldovich effect
- Synchronous frame