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Atomkern-Fusions-Energie

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Die Energiefrage

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Zusammenfassung

Bei der Verschmelzung der leichtesten Atomkerne, der Wasserstoff-Atomkerne zu Kernen der nächstschwereren Atomsorte, zu Helium-Atomkernen (für Details siehe Abschnitt 5.1) wird der dabei auftretende Massenverlust von 0.007 kg bei der Fusion von 1 kg Wasserstoffkernen zu 0.993 kg Heliumkernen gemäß der Einstein-Beziehung

$$ Energie = Masse \times {(Lichtgeschwindigkeit)^2}$$

zu Energie in Höhe von

$$E = 0.007kg \times {(3 \times {10^8}m/\sec )^2} = 170MiokWh $$

, umgewandelt.

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Authors and Affiliations

  1. Physikalisches Institut, Universität Bonn, Nußallee 12, 53115, Bonn, Deutschland

    Prof. Dr. Klaus Heinloth

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  1. Prof. Dr. Klaus Heinloth
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© 2003 Friedr. Vieweg & Sohn Verlagsgesellschaft mbH, Braunschweig/Wiesbaden

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Heinloth, K. (2003). Atomkern-Fusions-Energie. In: Die Energiefrage. Vieweg+Teubner Verlag. https://doi.org/10.1007/978-3-322-80322-1_8

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  • DOI: https://doi.org/10.1007/978-3-322-80322-1_8

  • Publisher Name: Vieweg+Teubner Verlag

  • Print ISBN: 978-3-528-13106-7

  • Online ISBN: 978-3-322-80322-1

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