
We start with the given equation:
\( \frac{y - 5}{2} + \frac{y - 0}{2} + \frac{y - x + 10}{1} = 0 \)
Expanding and simplifying:
\( y - 5 + y + 2y - 2x + 20 = 0 \)
\( 4y - 2x + 15 = 0 \quad \ldots (1) \)
Next, consider the equation:
\( \frac{x - 5}{4} + \frac{x - 0}{4} + \frac{x - 10 - y}{1} = 0 \)
Expanding this equation:
\( x - 5 + x + 4x - 40 - 4y = 0 \)
\( 6x - 4y - 45 = 0 \quad \ldots (i) \)
Now solving equations (1) and (i):
\( -2x + 4y + 15 = 0 \quad \ldots (ii) \)
and \( 4x - 30 = 0 \)
From these, we get:
\( x = \frac{15}{2} \) and \( 4y - 15 + 15 = 0 \Rightarrow y = 0 \)
Now, the current \( i \) is given by:
\( i = \frac{y - x + 10}{1} \)
Substituting the values of \( x \) and \( y \):
\( i = \frac{0 - 7.5 + 10}{1} \)
\( i = 2.5 \, \text{A} = \frac{n}{10} \, \text{A} \)
Therefore,
\( n = 25 \)
Let the potentials at points A, B, and C be \( x \), \( y \), and \( 0 \), respectively.
Applying Kirchhoff’s Current Law (KCL) at node B:
\[ \frac{y - 5}{2} + \frac{y - 0}{2} + \frac{y - x + 10}{1} = 0 \] \[ \Rightarrow 4y - 2x + 15 = 0 \quad \text{(i)} \]
Applying KCL at node A:
\[ \frac{x - 5}{4} + \frac{x - 0}{4} + \frac{x - 10 - y}{1} = 0 \] \[ \Rightarrow 6x - 4y - 45 = 0 \quad \text{(ii)} \]
Solving equations (i) and (ii):
From (i): \( y = \frac{15}{4}x - \frac{15}{4} \)
Substituting in (ii): \( x = \frac{15}{2}, \, y = 0 \)
The current through the \( 1 \, \Omega \) resistor is:
\[ i = \frac{y - x + 10}{1} = \frac{0 - 7.5 + 10}{1} = 2.5 \, \text{A}. \]
Therefore: \[ i = \frac{n}{10}, \quad n = 25. \]
Final Answer: \( n = 25 \).
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,




What will be the equilibrium constant of the given reaction carried out in a \(5 \,L\) vessel and having equilibrium amounts of \(A_2\) and \(A\) as \(0.5\) mole and \(2 \times 10^{-6}\) mole respectively?
The reaction : \(A_2 \rightleftharpoons 2A\)
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,