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A black coloured solid sphere of radius R and mass M is inside a cavity with a vacuum inside. The walls of the cavity are maintained at temperature T0. The initial temperature of the sphere is 3T0. If the specific heat o

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Concept: Stefan-Boltzmann Law, Heat Capacity

Question

A black coloured solid sphere of radius R and mass M is inside a cavity with a vacuum inside. The walls of the cavity are maintained at temperature T0. The initial temperature of the sphere is 3T0. If the specific heat of the material of the sphere varies as α T^3 per unit mass with the temperature T of the sphere, where α is a constant, then the time taken for the sphere to cool down to temperature 2T0 will be (σ is Stefan Boltzmann constant)
(A) Mα 16π R^2σ ((3)/(2) )
(B) Mα 16π R^2σ ((16)/(3) )
(C) Mα 4π R^2σ ((3)/(2) )
(D) Mα 4π R^2σ ((16)/(3) )

Try it yourself first

Hint: Pehle, aap Stefan-Boltzmann Law use karke rate of heat loss ka expression likho, aur phir usko specific heat ke term mein temperature change se relate karo.

Step-by-step solution

  1. 1

    Given parameters

    Sphere radius RR, mass MM, initial temperature 3T03T_0, final temperature 2T02T_0, cavity temperature T0T_0. Specific heat c=αT3c = \alpha T^3. Stefan-Boltzmann constant σ\sigma.
  2. 2

    Rate of heat loss

    Rate of heat loss by radiation from a black body is given by Stefan-Boltzmann Law.
    dQ/dt=Aσ(T4−T04)dQ/dt = A\sigma(T^4 - T_0^4)
  3. 3

    Relate heat loss to temperature change

    Heat lost by sphere dQ=mcdTdQ = mc dT. Equate this with radiation heat loss and integrate.
    mcdT=−Aσ(T4−T04)dtmc dT = -A\sigma(T^4 - T_0^4) dt
  4. 4

    Substitute values

    Substitute A=4πR2A = 4\pi R^2 and c=αT3c = \alpha T^3 into the equation.
    M(αT3)dT=−4πR2σ(T4−T04)dtM(\alpha T^3) dT = -4\pi R^2\sigma(T^4 - T_0^4) dt
  5. 5

    Rearrange for integration

    Separate variables TT and tt for integration.
    dt=−MαT34πR2σ(T4−T04)dTdt = -\frac{M\alpha T^3}{4\pi R^2\sigma(T^4 - T_0^4)} dT
  6. 6

    Integrate both sides

    Integrate tt from 00 to τ\tau and TT from 3T03T_0 to 2T02T_0.
    ∫0τdt=−Mα4πR2σ∫3T02T0T3T4−T04dT\int_0^\tau dt = -\frac{M\alpha}{4\pi R^2\sigma} \int_{3T_0}^{2T_0} \frac{T^3}{T^4 - T_0^4} dT
  7. 7

    Solve the integral

    Use substitution u=T4−T04u = T^4 - T_0^4, so du=4T3dTdu = 4T^3 dT.
    ∫T3T4−T04dT=14ln⁡∣T4−T04∣\int \frac{T^3}{T^4 - T_0^4} dT = \frac{1}{4} \ln|T^4 - T_0^4|
  8. 8

    Evaluate definite integral

    Substitute limits and simplify to find τ\tau.
    τ=Mα16πR2σ[ln⁡(T4−T04)]2T03T0\tau = \frac{M\alpha}{16\pi R^2\sigma} [\ln(T^4 - T_0^4)]_{2T_0}^{3T_0}
  9. 9

    Final time $\tau$

    Simplify the logarithmic terms.
    \tau = \frac{M\alpha}{16\pi R^2\sigma} \ln\left(\frac{81T_0^4 - T_0^4}{16T_0^4 - T_0^4}\right) = \frac{M\alpha}{16\pi R^2\sigma} \ln\left(\frac{80T_0^4}{15T_0^4}\right) = \frac{M\alpha}{16\pi R^2\sigm

Final answer

(b) Mα/(16πR2σ)×(16/3)M\alpha / (16\pi R^2\sigma) \times (16/3)

Remember: Stefan-Boltzmann law aur variable specific heat ke integration ko yaad rakho.

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Quick check · test yourself

Ek object ka temperature TT hai aur surrounding ka temperature TsT_s hai. Agar object ka temperature double ho jaye, toh uski net rate of heat loss by radiation kaise change hogi, assuming TsT_s constant hai aur T≫TsT \gg T_s?

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