To solve this problem, we apply the concept of energy level transitions in the Bohr model of the atom. When an electron transitions between energy levels, it emits or absorbs radiation. The wavelength of the radiation is related to the energy difference between the initial and final states by the equation:
\(E = \dfrac{hc}{\lambda}\)
where:
Given:
We need to find the wavelength of the radiation emitted during the transition from state A to state B, denoted as \(\lambda_{AB}\).
To find this, we use the relationship between these wavelengths implied by Bohr's model:
Now, substituting the known wavelengths into the energy relations gives:
Thus, the energy difference for the transition from A to B is:
\(E_{AB} = \dfrac{hc}{2000 \text{ Å}} - \dfrac{hc}{6000 \text{ Å}}\)
Combining these terms gives us:
\(E_{AB} = hc \left(\dfrac{1}{2000} - \dfrac{1}{6000}\right)\)
Finding a common denominator:
\(E_{AB} = hc \left(\dfrac{3-1}{6000}\right) = hc \left(\dfrac{2}{6000}\right) = \dfrac{hc}{3000 \text{ Å}}\)
Thus, \(\lambda_{AB} = 3000 \text{ Å}\), which means the correct option is 3000 Å.
Step 1: Use the Rydberg formula. The energy of a photon emitted during a transition is inversely proportional to the wavelength.
Let $\lambda_{AC}$ be the wavelength for A to C, $\lambda_{BC}$ be the wavelength for B to C, and $\lambda_{AB}$ be the wavelength for A to B. Then, the energy relationships are: \[ \frac{1}{\lambda_{AC}} = \frac{1}{\lambda_{AB}} + \frac{1}{\lambda_{BC}} \] Step 2: Substitute the given values. We have $\lambda_{AC} = 2000$ Å and $\lambda_{BC} = 6000$ Å. We want to find $\lambda_{AB}$. \[ \frac{1}{2000} = \frac{1}{\lambda_{AB}} + \frac{1}{6000} \] Step 3: Solve for $\lambda_{AB}$. \[ \frac{1}{\lambda_{AB}} = \frac{1}{2000} - \frac{1}{6000} = \frac{3}{6000} - \frac{1}{6000} = \frac{2}{6000} = \frac{1}{3000} \] \[ \lambda_{AB} = 3000 { Å} \] Therefore, the wavelength of the radiation emitted during the transition of electrons from state A to state B is 3000 Å. The correct answer is (1).
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 : \(A_2 \rightleftharpoons 2A\)