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24 relations: Alpha process, Electronvolt, Future of an expanding universe, Heat death of the universe, Iron, Iron star, Iron-55, Isotope, Isotopes of cobalt, Isotopes of iron, Isotopes of manganese, Isotopes of nickel, Neutron, Nickel-62, Nuclear binding energy, Nuclear fission, Nuclear fusion, Nucleon, Nuclide, Photodisintegration, Proton, Pure and Applied Chemistry, 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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Electronvolt
In physics, the electronvolt (symbol eV, also written electron-volt and electron volt) is a unit of energy equal to approximately joules (symbol J).
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Future of an expanding universe
Observations suggest that the expansion of the universe will continue forever.
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Heat death of the universe
The heat death of the universe is a plausible ultimate fate of the universe in which the universe has diminished to a state of no thermodynamic free energy and therefore can no longer sustain processes that increase entropy.
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Iron
Iron is a chemical element with symbol Fe (from ferrum) and atomic number 26.
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Iron star
In astronomy, an iron star is a hypothetical type of compact star that could occur in the universe in the extremely far future, after perhaps 101500 years.
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Iron-55
Iron-55 or 55Fe is a radioactive isotope of iron with a nucleus containing 26 protons and 29 neutrons.
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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 iron
Naturally occurring iron (26Fe) consists of four stable isotopes: 5.845% of 54Fe (possibly radioactive with a half-life over 3.1×1022 years), 91.754% of 56Fe, 2.119% of 57Fe and 0.282% of 58Fe.
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Isotopes of manganese
Naturally occurring manganese (25Mn) is composed of 1 stable isotope, 55Mn.
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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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Neutron
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Nickel-62
Nickel-62 is an isotope of nickel having 28 protons and 34 neutrons.
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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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Nuclear fission
In nuclear physics and nuclear chemistry, nuclear fission is either a nuclear reaction or a radioactive decay process in which the nucleus of an atom splits into smaller parts (lighter nuclei).
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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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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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Pure and Applied Chemistry
Pure and Applied Chemistry (abbreviated Pure Appl. Chem.) is the official journal for the International Union of Pure and Applied Chemistry (IUPAC).
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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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References
[1] https://en.wikipedia.org/wiki/Iron-56
