Similarities between Cosmology and Warm inflation
Cosmology and Warm inflation have 5 things in common (in Unionpedia): Friedmann equations, General relativity, Inflation (cosmology), Physical cosmology, Scale factor (cosmology).
Friedmann equations
The Friedmann equations are a set of equations in physical cosmology that govern the expansion of space in homogeneous and isotropic models of the universe within the context of general relativity.
Cosmology and Friedmann equations · Friedmann equations and Warm inflation ·
General relativity
General relativity (GR, also known as the general theory of relativity or GTR) is the geometric theory of gravitation published by Albert Einstein in 1915 and the current description of gravitation in modern physics.
Cosmology and General relativity · General relativity and Warm inflation ·
Inflation (cosmology)
In physical cosmology, cosmic inflation, cosmological inflation, or just inflation, is a theory of exponential expansion of space in the early universe.
Cosmology and Inflation (cosmology) · Inflation (cosmology) and Warm inflation ·
Physical cosmology
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.
Cosmology and Physical cosmology · Physical cosmology and Warm inflation ·
Scale factor (cosmology)
The relative expansion of the universe is parametrized by a dimensionless scale factor a. Also known as the cosmic scale factor or sometimes the Robertson–Walker scale factor, this is a key parameter of the Friedmann equations.
Cosmology and Scale factor (cosmology) · Scale factor (cosmology) and Warm inflation ·
The list above answers the following questions
- What Cosmology and Warm inflation have in common
- What are the similarities between Cosmology and Warm inflation
Cosmology and Warm inflation Comparison
Cosmology has 249 relations, while Warm inflation has 7. As they have in common 5, the Jaccard index is 1.95% = 5 / (249 + 7).
References
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