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Hot dark matter and Universe

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

Difference between Hot dark matter and Universe

Hot dark matter vs. Universe

Hot dark matter (HDM) is a theoretical form of dark matter which consists of particles that travel with ultrarelativistic velocities. The Universe is all of space and time and their contents, including planets, stars, galaxies, and all other forms of matter and energy.

Similarities between Hot dark matter and Universe

Hot dark matter and Universe have 15 things in common (in Unionpedia): Big Bang, Cambridge University Press, Cold dark matter, Cosmic Background Explorer, Cosmic microwave background, Dark matter, Electromagnetic radiation, Electromagnetism, Galaxy, Gravity, Lambda-CDM model, Neutrino, Strong interaction, Supercluster, Weak interaction.

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 Hot dark matter · Big Bang and Universe · See more »

Cambridge University Press

Cambridge University Press (CUP) is the publishing business of the University of Cambridge.

Cambridge University Press and Hot dark matter · Cambridge University Press and Universe · See more »

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 Hot dark matter · Cold dark matter and Universe · See more »

Cosmic Background Explorer

The Cosmic Background Explorer (COBE), also referred to as Explorer 66, was a satellite dedicated to cosmology, which operated from 1989 to 1993.

Cosmic Background Explorer and Hot dark matter · Cosmic Background Explorer and 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 Hot dark matter · Cosmic microwave background and Universe · See more »

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 Hot dark matter · Dark matter and Universe · See more »

Electromagnetic radiation

In physics, electromagnetic radiation (EM radiation or EMR) refers to the waves (or their quanta, photons) of the electromagnetic field, propagating (radiating) through space-time, carrying electromagnetic radiant energy.

Electromagnetic radiation and Hot dark matter · Electromagnetic radiation and Universe · See more »

Electromagnetism

Electromagnetism is a branch of physics involving the study of the electromagnetic force, a type of physical interaction that occurs between electrically charged particles.

Electromagnetism and Hot dark matter · Electromagnetism and Universe · See more »

Galaxy

A galaxy is a gravitationally bound system of stars, stellar remnants, interstellar gas, dust, and dark matter.

Galaxy and Hot dark matter · Galaxy and Universe · See more »

Gravity

Gravity, or gravitation, is a natural phenomenon by which all things with mass or energy—including planets, stars, galaxies, and even light—are brought toward (or gravitate toward) one another.

Gravity and Hot dark matter · Gravity and Universe · See more »

Lambda-CDM model

The ΛCDM (Lambda cold dark matter) or Lambda-CDM model is a parametrization of the Big Bang cosmological model in which the universe contains a cosmological constant, denoted by Lambda (Greek Λ), associated with dark energy, and cold dark matter (abbreviated CDM).

Hot dark matter and Lambda-CDM model · Lambda-CDM model and Universe · See more »

Neutrino

A neutrino (denoted by the Greek letter ν) is a fermion (an elementary particle with half-integer spin) that interacts only via the weak subatomic force and gravity.

Hot dark matter and Neutrino · Neutrino and Universe · See more »

Strong interaction

In particle physics, the strong interaction is the mechanism responsible for the strong nuclear force (also called the strong force or nuclear strong force), and is one of the four known fundamental interactions, with the others being electromagnetism, the weak interaction, and gravitation.

Hot dark matter and Strong interaction · Strong interaction and Universe · See more »

Supercluster

A supercluster is a large group of smaller galaxy clusters or galaxy groups; it is among the largest-known structures of the cosmos.

Hot dark matter and Supercluster · Supercluster and Universe · See more »

Weak interaction

In particle physics, the weak interaction (the weak force or weak nuclear force) is the mechanism of interaction between sub-atomic particles that causes radioactive decay and thus plays an essential role in nuclear fission.

Hot dark matter and Weak interaction · Universe and Weak interaction · See more »

The list above answers the following questions

Hot dark matter and Universe Comparison

Hot dark matter has 27 relations, while Universe has 479. As they have in common 15, the Jaccard index is 2.96% = 15 / (27 + 479).

References

This article shows the relationship between Hot dark matter and Universe. To access each article from which the information was extracted, please visit:

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