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  • '''Nuclear fusion''' is a process in which small atomic nuclei fuse and release energy. In a To derive useful power from nuclear fusion, the nuclei need to be confined at pressures and temperatures far higher th
    1 KB (233 words) - 14:56, 23 May 2023
  • 813 bytes (131 words) - 11:32, 23 May 2023

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  • '''Nuclear fusion''' is a process in which small atomic nuclei fuse and release energy. In a To derive useful power from nuclear fusion, the nuclei need to be confined at pressures and temperatures far higher th
    1 KB (233 words) - 14:56, 23 May 2023
  • ...he nuclei of atoms, including [[radioactivity]], [[nuclear fission]] and [[nuclear fusion]]. Radioactivity includes both the gain of [[neutron]]s changing the mass o
    363 bytes (49 words) - 19:54, 12 May 2010
  • {{r|Nuclear fusion}}
    1 KB (155 words) - 17:08, 22 March 2024
  • {{rpl|Nuclear fusion}}
    2 KB (223 words) - 20:33, 23 April 2024
  • {{r|nuclear fusion}}
    796 bytes (122 words) - 22:21, 3 March 2022
  • ...delayed (i.e., fallout) ionizing radiation by means of nuclear fission or nuclear fusion.<ref name=Glasstone>{{citation
    7 KB (1,063 words) - 16:23, 30 March 2024
  • ...e induced to do so by [[nuclear fission]] (splitting of the nucleus) or [[nuclear fusion]] (merging of nuclei). Energy release is in the [[X-ray]], [[gamma radiati
    5 KB (827 words) - 17:02, 22 March 2024
  • ...device''' is any assembly of components that can produce an explosion from nuclear fusion. A '''fission bomb''' can be dropped from an airplane, or at least transpor
    20 KB (3,072 words) - 10:33, 18 March 2024
  • ...ts of [[hydrogen]], which it converts to [[helium]] through a process of [[nuclear fusion]], providing the heat and light that allowed [[life]] to form here on our p
    3 KB (381 words) - 20:54, 21 July 2020
  • ...used to study nuclear reactions such as [[nuclear fission|fission]] and [[nuclear fusion|fusion]]. Some early evidence for nuclear fission was the formation of a sh
    10 KB (1,653 words) - 08:27, 12 September 2013
  • ...//lenr-canr.org/acrobat/Fleischmanelectroche.pdf Electrochemically induced nuclear fusion of deuterium] ''J. Electroanal Chem'' p. 301 errata in Vol. 263</ref><ref> ...and produces [[tritium]] in equal amounts. The established theory is that nuclear fusion reactions cannot be initiated without the input of significant energy to ov
    27 KB (4,108 words) - 00:45, 8 October 2013
  • ...Thermonuclear weapons are based on the energy released by [[Fusion device|nuclear fusion]] reactions or, more simply, the fusion of atoms. ...ecifically designed as a test device to validate the concept of creating a nuclear fusion weapon. It weighed about 74 [[tonne]]s (82 [[U.S. customary units|short ton
    19 KB (2,853 words) - 09:20, 22 April 2024
  • Red dwarfs [[Nuclear fusion|fuse]] [[hydrogen]] to [[helium]] via the [[Pp chain|proton-proton (PP) cha
    7 KB (1,111 words) - 11:24, 30 July 2022
  • ...ants are thought to be created after a star exhausted its capacities for [[nuclear fusion]]. It is estimated that for a star to be capable of compaction into a [[Sin
    9 KB (1,324 words) - 08:30, 31 July 2023
  • ...are still working on reactors capable of producing energy by controlled [[nuclear fusion]]. Our sun shines from energy produced through [[Hydrogen fusion]] in its
    20 KB (3,081 words) - 21:57, 31 March 2022
  • ...used to study nuclear reactions such as [[nuclear fission|fission]] and [[nuclear fusion|fusion]]. Some early evidence for nuclear fission was the formation of a sh
    31 KB (4,881 words) - 12:55, 15 March 2024
  • ...an only be affected by other particles through the weak force (e.g. in the nuclear fusion in the stars). Because they do not react readily, they can pass through alm
    18 KB (2,817 words) - 20:15, 27 October 2020
  • ...is the core region, a volume of sufficient temperature and pressure for [[nuclear fusion]] to occur. Above the core is the [[radiation zone]], where the plasma conv ...m a [[protostar]]. A sufficiently dense and hot core region will trigger [[nuclear fusion]] and it becomes a [[main-sequence star]].<ref name="sead">{{cite web | url
    46 KB (6,796 words) - 10:08, 28 February 2024
  • ...tructures called [[ascus|asci]] (''sing.'' ascus), in which [[karyogamy]] (nuclear fusion) occurs. These asci are embedded in an [[ascocarp]], or fruiting body, of t
    21 KB (3,091 words) - 09:52, 5 August 2023
  • ...nent. Its large mass gives it an interior density high enough to sustain [[nuclear fusion]], which releases enormous amounts of [[energy]], mostly [[Radiant energy|r ..." for a star, in that it has not yet exhausted its store of hydrogen for [[nuclear fusion]]. The Sun is growing brighter; early in its history it was 75 percent as
    76 KB (11,605 words) - 21:48, 1 September 2020
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