Given that \( 2P(x=2) = 3P(x=1) \), we can express the probabilities using the binomial distribution formula. \[ 2P(x=2) = 3P(x=1) \] \[ 2 \times \binom{n}{2} p^2 (1-p)^{n-2} = 3 \times \binom{n}{1} p (1-p)^{n-1} \] Simplifying: \[ 2 \times \frac{n(n-1)}{2} \times p^2 (1-p)^{n-2} = 3 \times n \times p \times (1-p)^{n-1} \] \[ \Rightarrow n(n-1)p^2 = 3n(1-p)p \] \[ \Rightarrow (n-1)p = 3(1-p) \quad \text{(Equation 1)} \] From here, we simplify further to find the value of \( p \) and \( n \).
Step 1: Solve for \( p \) and \( n \). From Equation 1: \[ (n-1)p = 3(1-p) \] \[ np - p = 3 - 3p \] \[ np + 3p = 3 + p \] \[ p(n + 3) = 3 \] \[ p = \frac{3}{n+3} \] Substitute this value of \( p \) into the equation for the variance and mean difference.
Step 2: Apply the condition for the mean and variance. The mean of a binomial distribution is \( \mu = np \), and the variance is \( \sigma^2 = np(1-p) \). Given that the difference between the mean and variance is 1: \[ np - np(1-p) = 1 \] Simplify this equation and solve for \( n \).
Step 3: Solve for \( n \). We find that \( n = 4 \).
Step 4: Find \( n^2 P(X > 1) \). Now, we compute \( P(X > 1) \) for \( n = 4 \) and \( p = \frac{1}{2} \). \[ P(X > 1) = 1 - P(X = 0) - P(X = 1) \] \[ P(X = 0) = \binom{4}{0} \left( \frac{1}{2} \right)^0 \left( \frac{1}{2} \right)^4 = \frac{1}{16} \] \[ P(X = 1) = \binom{4}{1} \left( \frac{1}{2} \right)^1 \left( \frac{1}{2} \right)^3 = \frac{4}{16} = \frac{1}{4} \] \[ P(X > 1) = 1 - \frac{1}{16} - \frac{4}{16} = \frac{11}{16} \] Now calculate \( n^2 P(X > 1) \): \[ n^2 P(X > 1) = 4^2 \times \frac{11}{16} = 16 \times \frac{11}{16} = 11 \]
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,