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Nuclear fusion
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{{Short description|Process of combining atomic nuclei}} {{hatnote group| {{About|the nuclear reaction|its use in producing energy|Fusion power|the journal|Nuclear Fusion (journal){{!}}''Nuclear Fusion'' (journal)|the song|Nuclear Fusion (song)}} {{Distinguish|Nuclear fission}} }} {{Use dmy dates|date=December 2022}} {{Use American English|date=December 2022}}{{multiple image | perrow = 2/1/2/2 | total_width = 410 | image1 = NASA's SDO Satellite Captures First Image of 2012 Venus Transit (Full Disc).jpg | image2 = VLTI reconstructed view of the surface of Antares.jpg | image3 = DominicHousatonic.gif | image4 = Operation Greenhouse George Device 001.jpg | image5 = Ivy Mike Sausage device.jpg | image6 = EAST Tokamak plasma image3.jpg | image7 = NIF implosion converging beams.jpg | footer = From top, left to right # [[The Sun]], powered by the [[proton–proton chain|proton–proton]] fusion chain # [[Antares]], a star massive enough for [[silicon burning]] # [[Operation Dominic|Dominic Housatonic]], largest fusion yield from a US nuclear test # [[Greenhouse George]]'s Cylinder device, the first artificial thermonuclear fusion experiment # [[Ivy Mike]]'s Sausage device, the first [[Teller–Ulam]] bomb # Fusion plasma in China's [[Experimental Advanced Superconducting Tokamak]] # Implosion lasers firing at [[National Ignition Facility]], the world's largest [[inertial confinement fusion]] experiment }} {{Nuclear physics}} '''Nuclear fusion''' is a [[nuclear reaction|reaction]] in which two or more [[atomic nuclei]] combine to form a larger nuclei, nuclei/[[neutrons|neutron]] by-products. The difference in mass between the reactants and products is manifested as either the release or [[absorption (electromagnetic radiation)|absorption]] of [[energy]]. This difference in mass arises as a result of the difference in [[nuclear binding energy]] between the atomic nuclei before and after the fusion reaction. Nuclear fusion is the process that powers all active [[stars]], via many [[Stellar nucleosynthesis|reaction pathways]]. Fusion processes require an extremely large [[Lawson criterion|triple product]] of temperature, density, and confinement time. These conditions occur only in [[Stellar core|stellar cores]], advanced [[Nuclear weapon design|nuclear weapons]], and are approached in [[List of fusion experiments|fusion power experiments]]. A nuclear fusion process that produces atomic nuclei lighter than [[nickel-62]] is generally [[exothermic]], due to the positive gradient of the [[Nuclear binding energy#Nuclear binding energy curve|nuclear binding energy curve]]. The most fusible nuclei are among the lightest, especially [[deuterium]], [[tritium]], and [[helium-3]]. The opposite process, [[nuclear fission]], is most energetic for very heavy nuclei, especially the [[actinides]]. Applications of fusion include [[fusion power]], [[thermonuclear weapons]], [[Boosted fission weapon|boosted fission weapons]], [[Neutron source|neutron sources]], and [[superheavy element]] production.
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