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Planck's blackbody formula
دیسول ِ سیهجسم ِ پلانک
disul-e siyah jesm-e Planck
Fr.: formule du corps noir de Planck
A formula that determines the distribution of intensity of radiation
that prevails under conditions of thermal equilibrium at a temperature
T:
Bv = (2hν3 / c2)[exp(hν / kT) - 1]-1
where h is Planck’s constant
and ν is the frequency.
See also: → Planck; → blackbody;
→ formula.
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