For \( \alpha, \beta, \gamma \in \mathbb{R} \), if \[ \lim_{x \to 0} \frac{x^2 \sin(\alpha x) + (\gamma - 1)e^{x^2}}{\sin(2x - \beta x)} = 3, \] then \( \beta + \gamma - \alpha \) is equal to:
We are asked to find the value of \( \beta + \gamma - \alpha \) for \( \alpha, \beta, \gamma \in \mathbb{R} \), given the following limit:
\[ \lim_{x \to 0} \frac{x^2 \sin \alpha x + (\gamma - 1)e^{x^2}}{\sin 2x - \beta x} = 3 \]To solve this limit problem, we will use the Maclaurin series (Taylor series expansion around \(x=0\)) for the functions involved. The key series expansions are:
The limit is in the indeterminate form \( \frac{0}{0} \). For the limit to result in a finite, non-zero constant, the lowest power of \( x \) in the numerator's series expansion must be the same as the lowest power of \( x \) in the denominator's expansion.
Step 1: Determine the value of \( \gamma \).
As \( x \to 0 \), the denominator \( D(x) = \sin 2x - \beta x \to \sin(0) - \beta(0) = 0 \). For the limit to be finite, the numerator \( N(x) \) must also approach 0.
\[ \lim_{x \to 0} \left( x^2 \sin \alpha x + (\gamma - 1)e^{x^2} \right) = 0^2 \sin(0) + (\gamma - 1)e^0 = 0 + (\gamma - 1)(1) = \gamma - 1 \]Setting the numerator to 0:
\[ \gamma - 1 = 0 \implies \gamma = 1 \]Step 2: Expand the numerator and denominator using Maclaurin series.
With \( \gamma = 1 \), the numerator becomes:
\[ N(x) = x^2 \sin(\alpha x) \]Using the expansion for \( \sin(\alpha x) \):
\[ N(x) = x^2 \left( \alpha x - \frac{(\alpha x)^3}{3!} + \dots \right) = \alpha x^3 - \frac{\alpha^3 x^5}{6} + \dots \]The denominator is:
\[ D(x) = \sin(2x) - \beta x \]Using the expansion for \( \sin(2x) \):
\[ D(x) = \left( 2x - \frac{(2x)^3}{3!} + \dots \right) - \beta x = (2 - \beta)x - \frac{8x^3}{6} + \dots = (2 - \beta)x - \frac{4}{3}x^3 + \dots \]Step 3: Determine the value of \( \beta \).
The limit expression is now:
\[ \lim_{x \to 0} \frac{\alpha x^3 - \frac{\alpha^3 x^5}{6} + \dots}{(2 - \beta)x - \frac{4}{3}x^3 + \dots} = 3 \]The lowest power of \( x \) in the numerator is \( x^3 \). For the limit to be a finite, non-zero value, the lowest power of \( x \) in the denominator must also be \( x^3 \). This means the coefficient of the lower power term (\(x\)) in the denominator must be zero.
\[ 2 - \beta = 0 \implies \beta = 2 \]Step 4: Determine the value of \( \alpha \).
After setting \( \beta = 2 \), the limit becomes:
\[ \lim_{x \to 0} \frac{\alpha x^3 - \frac{\alpha^3 x^5}{6} + \dots}{-\frac{4}{3}x^3 + \dots} = 3 \]We can evaluate this limit by taking the ratio of the coefficients of the lowest power terms (\(x^3\)):
\[ \frac{\alpha}{-\frac{4}{3}} = 3 \] \[ \alpha = 3 \times \left(-\frac{4}{3}\right) = -4 \]We have found the values of the parameters:
Now, we compute the required expression \( \beta + \gamma - \alpha \):
\[ \beta + \gamma - \alpha = 2 + 1 - (-4) = 3 + 4 = 7 \]Thus, the value of \( \beta + \gamma - \alpha \) is 7.
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,