Step 1: Write the characteristic equation.
The differential equation is:
\[
\frac{d^2y}{dx^2} + 5\frac{dy}{dx} + 6y = 0
\]
Characteristic equation:
\[
r^2 + 5r + 6 = 0 $\Rightarrow$ (r + 2)(r + 3) = 0
\]
\[
r = -2, -3
\]
Step 2: General solution.
\[
y(x) = A e^{-2x} + B e^{-3x}
\]
Step 3: Apply initial conditions.
For \(x = 0,\ y(0) = 2:\)
\[
A + B = 2 (1)
\]
Derivative:
\[
\frac{dy}{dx} = -2A e^{-2x} - 3B e^{-3x}
\]
At \(x=0,\ \frac{dy}{dx} = 0:\)
\[
-2A - 3B = 0 $\Rightarrow$ 2A + 3B = 0 (2)
\]
Solving (1) and (2):
Multiply (1) by 2 → \(2A + 2B = 4\)
Subtract from (2):
\[
(2A + 3B) - (2A + 2B) = 0 - 4 $\Rightarrow$ B = -4
\]
Substitute in (1):
\[
A - 4 = 2 $\Rightarrow$ A = 6
\]
Step 4: Substitute constants.
\[
y(x) = 6 e^{-2x} - 4 e^{-3x}
\]
At \(x = 1:\)
\[
y(1) = 6 e^{-2} - 4 e^{-3} = 6(0.1353) - 4(0.0498) = 0.8118 - 0.1992 = 0.6126
\]
Rounded to two decimals: \(y(1) = 0.61\).
Step 5: Conclusion.
Hence, \(y(1) = 0.61\).
Let \( f : \mathbb{R} \to \mathbb{R} \) be a twice differentiable function such that \( f(x + y) = f(x) f(y) \) for all \( x, y \in \mathbb{R} \). If \( f'(0) = 4a \) and \( f \) satisfies \( f''(x) - 3a f'(x) - f(x) = 0 \), where \( a > 0 \), then the area of the region R = {(x, y) | 0 \(\leq\) y \(\leq\) f(ax), 0 \(\leq\) x \(\leq\) 2 is :

At a particular temperature T, Planck's energy density of black body radiation in terms of frequency is \(\rho_T(\nu) = 8 \times 10^{-18} \text{ J/m}^3 \text{ Hz}^{-1}\) at \(\nu = 3 \times 10^{14}\) Hz. Then Planck's energy density \(\rho_T(\lambda)\) at the corresponding wavelength (\(\lambda\)) has the value \rule{1cm}{0.15mm} \(\times 10^2 \text{ J/m}^4\). (in integer)
[Speed of light \(c = 3 \times 10^8\) m/s]
(Note: The unit for \(\rho_T(\nu)\) in the original problem was given as J/m³, which is dimensionally incorrect for a spectral density. The correct unit J/(m³·Hz) or J·s/m³ is used here for the solution.)