Category:Physical cosmology
 | This category is overpopulated. It is suggested that the contents of the category be subcategorized. |
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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 10 subcategories, out of 23 total.
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- Inflation (cosmology) (25 P)
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- Observational cosmology (6 P)
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- Philosophers of cosmology (19 P)
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- Cosmological simulation (10 P)
- Standard candles (13 P)
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- Physical cosmology stubs (61 P)
Pages in category "Physical cosmology"
The following 103 pages are in this category, out of approximately 231 total. This list may not reflect recent changes.
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- Partial impact theory
- Particle horizon
- Particle physics in cosmology
- Photon epoch
- Physics applications of asymptotically safe gravity
- Physics beyond the Standard Model
- Picard horn
- Planck scale
- Planetary nebula luminosity function
- Plasma cosmology
- Polarization (cosmology)
- Pressuron
- Primordial fluctuations
- Primordial isocurvature baryon model
- Protogalaxy
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- Sachs–Wolfe effect
- Scalar–tensor theory
- Scalar–vector–tensor decomposition
- Scale factor (cosmology)
- Self-indication assumption
- Self-sampling assumption
- Sigma-D relation
- Source counts
- Static universe
- Steady-state model
- Stebbins–Whitford effect
- String cosmology
- String phenomenology
- String theory landscape
- Synchronous frame