Step 1: State Wien's Displacement Law. Wien's law states that the wavelength at which a black body emits the maximum amount of radiation, \( \lambda_{\text{max}} \), is inversely proportional to its absolute temperature \(T\). \[ \lambda_{\text{max}} T = b \] where \(b\) is Wien's displacement constant (\( \approx 2.898 \times 10^{-3} \) m⋅K).
Step 2: Set up a ratio for the two bodies P and Q. Since \( \lambda_{\text{max}} T \) is constant for any black body: \[ \lambda_{P} T_{P} = \lambda_{Q} T_{Q} \]
Step 3: Rearrange the formula to solve for the unknown temperature, \(T_Q\). \[ T_Q = T_P \left( \frac{\lambda_P}{\lambda_Q} \right) \]
Step 4: Substitute the given values and calculate \(T_Q\). - \( T_P = 1000 \) K - \( \lambda_P = 3000 \) nm - \( \lambda_Q = 550 \) nm Note that since we are using a ratio, we do not need to convert nanometers to meters. \[ T_Q = 1000 \times \frac{3000}{550} = 1000 \times \frac{300}{55} = 1000 \times \frac{60}{11} \approx 1000 \times 5.4545 \] \[ T_Q \approx 5454.5 \text{ K} \]
If \(f(t)\) is the inverse Laplace transform of \( F(s) = \frac{s+1+s^{-2}}{s^2-1} \), then \(f(t)\) is
Match LIST-I with LIST-II
LIST-I (Differential Equation)
(A) \(\frac{dy}{dx} = 2x(y-x^2+1)\)
(B) \(x\frac{dy}{dx} + 2(x^2+1)y=6\)
(C) \((x^2+1)\frac{dy}{dx} + 2xy = x \sin x\)
(D) \(x^3\frac{dy}{dx} + 2xy = 2x^2e^{x^2}\)
LIST-II (Integrating Factor)
(I) \(x^2\)
(II) \(e^{-x^2}\)
(III) \(x^2e^x\)
(IV) \(1+x^2\)
Choose the correct answer from the options given below: