Cosmology and Static universe

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between Cosmology and Static universe

Cosmology vs. Static universe

Cosmology (from the Greek κόσμος, kosmos "world" and -λογία, -logia "study of") is the study of the origin, evolution, and eventual fate of the universe. A static universe, also referred to as a "stationary" or "infinite" or "static infinite" universe, is a cosmological model in which the universe is both spatially infinite and temporally infinite, and space is neither expanding nor contracting.

Accelerating expansion of the universe

The accelerating expansion of the universe is the observation that the universe appears to be expanding at an increasing rate, so that the velocity at which a distant galaxy is receding from the observer is continuously increasing with time.

Accelerating expansion of the universe and Cosmology · Accelerating expansion of the universe and Static universe · See more »

Albert Einstein

Albert Einstein (14 March 1879 – 18 April 1955) was a German-born theoretical physicist who developed the theory of relativity, one of the two pillars of modern physics (alongside quantum mechanics).

Albert Einstein and Cosmology · Albert Einstein and Static universe · See more »

Big Bang

The Big Bang theory is the prevailing cosmological model for the universe from the earliest known periods through its subsequent large-scale evolution.

Big Bang and Cosmology · Big Bang and Static universe · See more »

Big Crunch

The Big Crunch is one possible scenario for the ultimate fate of the universe, in which the metric expansion of space eventually reverses and the universe recollapses, ultimately causing the cosmic scale factor to reach zero or causing a reformation of the universe starting with another Big Bang.

Big Crunch and Cosmology · Big Crunch and Static universe · See more »

Cosmic microwave background

The cosmic microwave background (CMB, CMBR) is electromagnetic radiation as a remnant from an early stage of the universe in Big Bang cosmology.

Cosmic microwave background and Cosmology · Cosmic microwave background and Static universe · See more »

Cosmological constant

In cosmology, the cosmological constant (usually denoted by the Greek capital letter lambda: Λ) is the value of the energy density of the vacuum of space.

Cosmological constant and Cosmology · Cosmological constant and Static universe · See more »

Dark energy

In physical cosmology and astronomy, dark energy is an unknown form of energy which is hypothesized to permeate all of space, tending to accelerate the expansion of the universe.

Cosmology and Dark energy · Dark energy and Static universe · See more »

Edwin Hubble

Edwin Powell Hubble (November 20, 1889 – September 28, 1953) was an American astronomer.

Cosmology and Edwin Hubble · Edwin Hubble and Static universe · See more »

Expansion of the universe

The expansion of the universe is the increase of the distance between two distant parts of the universe with time.

Cosmology and Expansion of the universe · Expansion of the universe and Static universe · See more »

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.

Cosmology and Friedmann–Lemaître–Robertson–Walker metric · Friedmann–Lemaître–Robertson–Walker metric and Static universe · See more »

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 Static universe · See more »

Georges Lemaître

Georges Henri Joseph Édouard Lemaître, RAS Associate (17 July 1894 – 20 June 1966) was a Belgian Catholic Priest, astronomer and professor of physics at the Catholic University of Leuven.

Cosmology and Georges Lemaître · Georges Lemaître and Static universe · See more »

Milne model

The Milne model was a special-relativistic cosmological model proposed by Edward Arthur Milne in 1935.

Cosmology and Milne model · Milne model and Static universe · See more »

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 Static universe · See more »

Plasma cosmology

Plasma cosmology is a non-standard cosmology whose central postulate is that the dynamics of ionized gases and plasmas play important, if not dominant, roles in the physics of the universe beyond the Solar System.

Cosmology and Plasma cosmology · Plasma cosmology and Static universe · See more »

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.

Cosmology and Redshift · Redshift and Static universe · See more »

Richard C. Tolman

Richard Chace Tolman (March 4, 1881 – September 5, 1948) was an American mathematical physicist and physical chemist who was an authority on statistical mechanics.

Cosmology and Richard C. Tolman · Richard C. Tolman and Static universe · See more »

Shape of the universe

The shape of the universe is the local and global geometry of the universe.

Cosmology and Shape of the universe · Shape of the universe and Static universe · See more »

Speed of light

The speed of light in vacuum, commonly denoted, is a universal physical constant important in many areas of physics.

Cosmology and Speed of light · Speed of light and Static universe · See more »

Steady State theory

In cosmology, the Steady State theory is an alternative to the Big Bang model of the evolution of our universe.

Cosmology and Steady State theory · Static universe and Steady State theory · See more »