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Nickel-62

Index Nickel-62

Nickel-62 is an isotope of nickel having 28 protons and 34 neutrons. [1]

18 relations: Alpha process, Iron-56, Isotope, Isotopes of cobalt, Isotopes of nickel, Isotopes of zinc, Neutron, Neutron capture, Nickel, Nuclear binding energy, Nucleon, Nuclide, Photodisintegration, Proton, R-process, Stable isotope ratio, Stellar nucleosynthesis, Universe.

Alpha process

The alpha process, also known as the alpha ladder, is one of two classes of nuclear fusion reactions by which stars convert helium into heavier elements, the other being the triple-alpha process.

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Iron-56

Iron-56 (56Fe) is the most common isotope of iron.

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Isotope

Isotopes are variants of a particular chemical element which differ in neutron number.

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Isotopes of cobalt

Naturally occurring cobalt (27Co) is composed of 1 stable isotope, 59Co.

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Isotopes of nickel

Naturally occurring nickel (28Ni) is composed of five stable isotopes;,,, and with being the most abundant (68.077% natural abundance).

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Isotopes of zinc

Naturally occurring zinc (30Zn) is composed of the 5 stable isotopes 64Zn, 66Zn, 67Zn, 68Zn, and 70Zn with 64Zn being the most abundant (48.6% natural abundance).

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Neutron

| magnetic_moment.

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Neutron capture

Neutron capture is a nuclear reaction in which an atomic nucleus and one or more neutrons collide and merge to form a heavier nucleus.

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Nickel

Nickel is a chemical element with symbol Ni and atomic number 28.

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Nuclear binding energy

Nuclear binding energy is the minimum energy that would be required to disassemble the nucleus of an atom into its component parts.

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Nucleon

In chemistry and physics, a nucleon is either a proton or a neutron, considered in its role as a component of an atomic nucleus.

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Nuclide

A nuclide (from nucleus, also known as nuclear species) is an atomic species characterized by the specific constitution of its nucleus, i.e., by its number of protons Z, its number of neutrons N, and its nuclear energy state.

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Photodisintegration

Photodisintegration (also called phototransmutation) is a nuclear process in which an atomic nucleus absorbs a high-energy gamma ray, enters an excited state, and immediately decays by emitting a subatomic particle.

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Proton

| magnetic_moment.

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R-process

The rapid neutron-capture process, or so-called r-process, is a set of nuclear reactions that in nuclear astrophysics is responsible for the creation (nucleosynthesis) of approximately half the abundances of the atomic nuclei heavier than iron, usually synthesizing the entire abundance of the two most neutron-rich stable isotopes of each heavy element.

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Stable isotope ratio

The term stable isotope has a meaning similar to stable nuclide, but is preferably used when speaking of nuclides of a specific element.

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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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Universe

The Universe is all of space and time and their contents, including planets, stars, galaxies, and all other forms of matter and energy.

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Redirects here:

Mass per nucleon, Ni-62.

References

[1] https://en.wikipedia.org/wiki/Nickel-62

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