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(b) State Kirchhoff's law. From Stefan's law derive Newton's law of cooling. [6]

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JU-PHY2nd YearFinalThermal PhysicsRadiationStefan-Boltzmann law; Wien's displacement law. (Topic Practice)JU-PHY - ⚡ অনলাইন প্রশ্নব্যাংক দেখুন 💥
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Another Explanation (5):

Kirchhoff's Laws:

  1. Kirchhoff's Current Law (KCL): The algebraic sum of currents entering a node (junction) is zero. ΣIin = ΣIout
  2. Kirchhoff's Voltage Law (KVL): The algebraic sum of voltages around any closed loop in a circuit is zero. ΣV = 0

Derivation of Newton's Law of Cooling from Stefan's Law:

Stefan's Law: P = εσAT4 where P is power radiated, ε is emissivity, σ is Stefan-Boltzmann constant, A is surface area, and T is absolute temperature.

Consider an object at temperature T cooling in surroundings at temperature T0. The net power radiated is:

Pnet = εσA(T4 - T04)

If TT0, then we can approximate (using binomial expansion or Taylor series):

T4 - T04 ≈ 4T03(T - T0)

Substituting this into the net power equation gives:

Pnet ≈ 4εσAT03(T - T0)

Since power is related to the rate of heat loss (dQ/dt) and heat loss is related to temperature change (dQ = mc dT), we get (assuming constant specific heat capacity 'c' and mass 'm'):

mc(dT/dt) = -4εσAT03(T - T0)

This simplifies to Newton's Law of Cooling:

dT/dt = -k(T - T0) where k = (4εσAT03)/(mc)