Faster access than browser!Similarities between N-body simulation and Observable universe
N-body simulation and Observable universe have 15 things in common (in Unionpedia): Astrophysics, Bolshoi Cosmological Simulation, Cold dark matter, Comoving and proper distances, Dark matter, Earth, Friedmann–Lemaître–Robertson–Walker metric, Galaxy filament, General relativity, Gravitational constant, Observable universe, Photon, Physical cosmology, Redshift, Scale factor (cosmology).
Astrophysics
Astrophysics is the branch of astronomy that employs the principles of physics and chemistry "to ascertain the nature of the astronomical objects, rather than their positions or motions in space".
Astrophysics and N-body simulation · Astrophysics and Observable universe ·
Bolshoi Cosmological Simulation
The Bolshoi simulation, run in 2010 on the Pleiades supercomputer at the NASA Ames Research Center, was the most accurate cosmological simulation to that date of the evolution of the large-scale structure of the universe.
Bolshoi Cosmological Simulation and N-body simulation · Bolshoi Cosmological Simulation and Observable universe ·
Cold dark matter
In cosmology and physics, cold dark matter (CDM) is a hypothetical form of dark matter whose particles moved slowly compared to the speed of light (the cold in CDM) since the universe was approximately one year old (a time when the cosmic particle horizon contained the mass of one typical galaxy); and interact very weakly with ordinary matter and electromagnetic radiation (the dark in CDM).
Cold dark matter and N-body simulation · Cold dark matter and Observable universe ·
Comoving and proper distances
In standard cosmology, comoving distance and proper distance are two closely related distance measures used by cosmologists to define distances between objects.
Comoving and proper distances and N-body simulation · Comoving and proper distances and Observable universe ·
Dark matter
Dark matter is a theorized form of matter that is thought to account for approximately 80% of the matter in the universe, and about a quarter of its total energy density.
Dark matter and N-body simulation · Dark matter and Observable universe ·
Earth
Earth is the third planet from the Sun and the only astronomical object known to harbor life.
Earth and N-body simulation · Earth and Observable universe ·
Friedmann–Lemaître–Robertson–Walker metric
The Friedmann–Lemaître–Robertson–Walker (FLRW) metric is an exact solution of Einstein's field equations of general relativity; it describes a homogeneous, isotropic, expanding or contracting universe that is path connected, but not necessarily simply connected.
Friedmann–Lemaître–Robertson–Walker metric and N-body simulation · Friedmann–Lemaître–Robertson–Walker metric and Observable universe ·
Galaxy filament
The distribution reveals fine, filamentary structures.
Galaxy filament and N-body simulation · Galaxy filament and Observable universe ·
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.
General relativity and N-body simulation · General relativity and Observable universe ·
Gravitational constant
The gravitational constant (also known as the "universal gravitational constant", the "Newtonian constant of gravitation", or the "Cavendish gravitational constant"), denoted by the letter, is an empirical physical constant involved in the calculation of gravitational effects in Sir Isaac Newton's law of universal gravitation and in Albert Einstein's general theory of relativity.
Gravitational constant and N-body simulation · Gravitational constant and Observable universe ·
Observable universe
The observable universe is a spherical region of the Universe comprising all matter that can be observed from Earth at the present time, because electromagnetic radiation from these objects has had time to reach Earth since the beginning of the cosmological expansion.
N-body simulation and Observable universe · Observable universe and Observable universe ·
Photon
The photon is a type of elementary particle, the quantum of the electromagnetic field including electromagnetic radiation such as light, and the force carrier for the electromagnetic force (even when static via virtual particles).
N-body simulation and Photon · Observable universe and Photon ·
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.
N-body simulation and Physical cosmology · Observable universe and Physical cosmology ·
Redshift
In physics, redshift happens when light or other electromagnetic radiation from an object is increased in wavelength, or shifted to the red end of the spectrum.
N-body simulation and Redshift · Observable universe and Redshift ·
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.
N-body simulation and Scale factor (cosmology) · Observable universe and Scale factor (cosmology) ·
The list above answers the following questions
- What N-body simulation and Observable universe have in common
- What are the similarities between N-body simulation and Observable universe
N-body simulation and Observable universe Comparison
N-body simulation has 71 relations, while Observable universe has 128. As they have in common 15, the Jaccard index is 7.54% = 15 / (71 + 128).
References
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