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单词 Stefan’s law
释义
Stefan’s law

Physics
  • The total energy radiated per unit surface area of a black body in unit time is proportional to the fourth power of its thermodynamic temperature. The constant of proportionality, the Stefan constant (or Stefan–Boltzmann constant) has the value 5.6697×10−8 J s−1 m−2 K−4. The law was discovered by the Austrian physicist Joseph Stefan (1853–93) and theoretically derived by Ludwig Boltzmann.


Astronomy
  • An alternative name for the Stefan–Boltzmann law.


Chemical Engineering
  • A law of thermal radiation in which the radiation of all wavelengths per second per square metre from a black body at an absolute temperature T to surroundings at temperature To is proportional to the fourth power of the absolute temperatures: q=σ(T4To4). The proportionality constant, σ, is known as the Stefan–Boltzmann constant equal to 5.669 7 × 10−8 W m−2 K−4 . The law is named after Austrian physicists Josef Stefan (1853–93) and Ludwig Eduard Boltzmann (1844–1906) who theoretically derived the equation.


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