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c 3 e − h ν k T {\displaystyle u_{\nu }={\frac {8\pi h\nu ^{3}}{c^{3}}}e^{-{\frac {h\nu }{kT}}}} On retrouve alors la loi de Wien. <<Physique atomique
Wikibooks (fr) · 3702 kelime · Physique atomique
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