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Nuclear fusion and Universe

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

Difference between Nuclear fusion and Universe

Nuclear fusion vs. Universe

In nuclear physics, nuclear fusion is a reaction in which two or more atomic nuclei come close enough to form one or more different atomic nuclei and subatomic particles (neutrons or protons). 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 Nuclear fusion and Universe

Nuclear fusion and Universe have 36 things in common (in Unionpedia): Angular momentum, Annihilation, Antimatter, Astrophysics, Atomic nucleus, Cepheid variable, Deuterium, Electric charge, Electron, Energy, Energy density, Fermion, Helium, Hydrogen, Ion, Lithium, Massachusetts Institute of Technology, Mass–energy equivalence, Matter, Metallicity, Muon, Nature (journal), Neutrino, Neutron, Nuclear force, Nuclear fusion, Opacity (optics), Particle accelerator, Pauli exclusion principle, Plasma (physics), ..., Proton, Quantum mechanics, Star, Stellar nucleosynthesis, Strong interaction, Supernova nucleosynthesis. Expand index (6 more) »

Angular momentum

In physics, angular momentum (rarely, moment of momentum or rotational momentum) is the rotational equivalent of linear momentum.

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Annihilation

In particle physics, annihilation is the process that occurs when a subatomic particle collides with its respective antiparticle to produce other particles, such as an electron colliding with a positron to produce two photons.

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Antimatter

In modern physics, antimatter is defined as a material composed of the antiparticle (or "partners") to the corresponding particles of ordinary matter.

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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".

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Atomic nucleus

The atomic nucleus is the small, dense region consisting of protons and neutrons at the center of an atom, discovered in 1911 by Ernest Rutherford based on the 1909 Geiger–Marsden gold foil experiment.

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Cepheid variable

A Cepheid variable is a type of star that pulsates radially, varying in both diameter and temperature and producing changes in brightness with a well-defined stable period and amplitude.

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Deuterium

Deuterium (or hydrogen-2, symbol or, also known as heavy hydrogen) is one of two stable isotopes of hydrogen (the other being protium, or hydrogen-1).

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Electric charge

Electric charge is the physical property of matter that causes it to experience a force when placed in an electromagnetic field.

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Electron

The electron is a subatomic particle, symbol or, whose electric charge is negative one elementary charge.

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Energy

In physics, energy is the quantitative property that must be transferred to an object in order to perform work on, or to heat, the object.

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Energy density

Energy density is the amount of energy stored in a given system or region of space per unit volume.

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Fermion

In particle physics, a fermion is a particle that follows Fermi–Dirac statistics.

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Helium

Helium (from lit) is a chemical element with symbol He and atomic number 2.

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Hydrogen

Hydrogen is a chemical element with symbol H and atomic number 1.

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Ion

An ion is an atom or molecule that has a non-zero net electrical charge (its total number of electrons is not equal to its total number of protons).

Ion and Nuclear fusion · Ion and Universe · See more »

Lithium

Lithium (from lit) is a chemical element with symbol Li and atomic number 3.

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Massachusetts Institute of Technology

The Massachusetts Institute of Technology (MIT) is a private research university located in Cambridge, Massachusetts, United States.

Massachusetts Institute of Technology and Nuclear fusion · Massachusetts Institute of Technology and Universe · See more »

Mass–energy equivalence

In physics, mass–energy equivalence states that anything having mass has an equivalent amount of energy and vice versa, with these fundamental quantities directly relating to one another by Albert Einstein's famous formula: E.

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Matter

In the classical physics observed in everyday life, matter is any substance that has mass and takes up space by having volume.

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Metallicity

In astronomy, metallicity is used to describe the abundance of elements present in an object that are heavier than hydrogen or helium.

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Muon

The muon (from the Greek letter mu (μ) used to represent it) is an elementary particle similar to the electron, with an electric charge of −1 e and a spin of 1/2, but with a much greater mass.

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Nature (journal)

Nature is a British multidisciplinary scientific journal, first published on 4 November 1869.

Nature (journal) and Nuclear fusion · Nature (journal) 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.

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Neutron

| magnetic_moment.

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Nuclear force

The nuclear force (or nucleon–nucleon interaction or residual strong force) is a force that acts between the protons and neutrons of atoms.

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Nuclear fusion

In nuclear physics, nuclear fusion is a reaction in which two or more atomic nuclei come close enough to form one or more different atomic nuclei and subatomic particles (neutrons or protons).

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Opacity (optics)

Opacity is the measure of impenetrability to electromagnetic or other kinds of radiation, especially visible light.

Nuclear fusion and Opacity (optics) · Opacity (optics) and Universe · See more »

Particle accelerator

A particle accelerator is a machine that uses electromagnetic fields to propel charged particles to nearly light speed and to contain them in well-defined beams.

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Pauli exclusion principle

The Pauli exclusion principle is the quantum mechanical principle which states that two or more identical fermions (particles with half-integer spin) cannot occupy the same quantum state within a quantum system simultaneously.

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Plasma (physics)

Plasma (Henry George Liddell, Robert Scott, A Greek English Lexicon, on Perseus) is one of the four fundamental states of matter, and was first described by chemist Irving Langmuir in the 1920s.

Nuclear fusion and Plasma (physics) · Plasma (physics) and Universe · See more »

Proton

| magnetic_moment.

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Quantum mechanics

Quantum mechanics (QM; also known as quantum physics, quantum theory, the wave mechanical model, or matrix mechanics), including quantum field theory, is a fundamental theory in physics which describes nature at the smallest scales of energy levels of atoms and subatomic particles.

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Star

A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.

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Stellar nucleosynthesis

Stellar nucleosynthesis is the theory explaining the creation (nucleosynthesis) of chemical elements by nuclear fusion reactions between atoms within the stars.

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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.

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Supernova nucleosynthesis

Supernova nucleosynthesis is a theory of the nucleosynthesis of the natural abundances of the chemical elements in supernova explosions, advanced as the nucleosynthesis of elements from carbon to nickel in massive stars by Fred Hoyle in 1954.

Nuclear fusion and Supernova nucleosynthesis · Supernova nucleosynthesis and Universe · See more »

The list above answers the following questions

Nuclear fusion and Universe Comparison

Nuclear fusion has 150 relations, while Universe has 479. As they have in common 36, the Jaccard index is 5.72% = 36 / (150 + 479).

References

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

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