Atomic Physics: Bohr Theory, Spectral Series, X-rays, and Lasers

Boher's Theory and the Concept of Wave Number

  • Definition of Wave Number: Wave number (1/λ1/\lambda) represents the number of waves present in a length of 1 meter.

  • Mathematical Equation: The equation for the wave number is derived from Bohr's theory as:     1λ=RH×(1nf21ni2)\frac{1}{\lambda} = R_H \times \left( \frac{1}{n_f^2} - \frac{1}{n_i^2} \right)

  • Rydberg Constant (RHR_H):

    • Exact value: 1.097×107m11.097 \times 10^7 \, \text{m}^{-1}.

    • Simplified calculation value (for non-calculator exams): 1×107m11 \times 10^7 \, \text{m}^{-1}.

  • State Definitions:

    • nfn_f: Final state or final shell where the electron transitions to (destination).

    • nin_i: Initial state or initial shell where the electron originates from.

  • Electron Transitions:

    • Excitation: Electron moves from lower to higher energy levels, absorbing energy.

    • De-excitation: Electron moves from higher to lower levels, emitting energy in the form of a photon with a specific wavelength and energy.

Hydrogen Emission Spectrum

  • Concept of Spectrum: A spectrum is essentially a graph-like representation used to plot the wavelengths of different emitted photons or electromagnetic radiations.

  • Line Spectrum vs. Continuous Spectrum:

    • Rutherford's model predicted a continuous spectrum.

    • The observed reality is a Line Spectrum, consisting of discrete spectral lines corresponding to specific wavelengths.

  • Emission Spectrum: This occurs when an electron releases energy (emits radiation) as it jumps from a high energy level to a low energy level.

  • Absorption Spectrum: This occurs when an electron acquires energy to move from a ground state to a higher excitation state. Note: This is not the primary focus of the current study session.

Hydrogen Spectral Series

The series are classified based on the final state (nfn_f) to which the electron falls:

  • Lyman Series:

    • Final state: nf=1n_f = 1

    • Initial states: ni=2,3,4,,n_i = 2, 3, 4, \dots, \infty

    • Region: Ultraviolet (UV) region.

  • Balmer Series:

    • Final state: nf=2n_f = 2

    • Initial states: ni=3,4,5,,n_i = 3, 4, 5, \dots, \infty

    • Region: Visible region (can be seen with the naked eye).

    • Wavelength range: Approximately 400nm400 \, \text{nm} to 720nm720 \, \text{nm} (4000A˚4000 \, \text{Å} to 7000A˚7000 \, \text{Å}).

  • Paschen Series:

    • Final state: nf=3n_f = 3

    • Initial states: ni=4,5,6,,n_i = 4, 5, 6, \dots, \infty

    • Region: Infrared (IR) region (specifically Lower Infrared).

  • Brackett Series:

    • Final state: nf=4n_f = 4

    • Initial states: ni=5,6,7,,n_i = 5, 6, 7, \dots, \infty

    • Region: Infrared (IR) region.

  • Pfund Series:

    • Final state: nf=5n_f = 5

    • Initial states: ni=6,7,8,,n_i = 6, 7, 8, \dots, \infty

    • Region: Infrared (IR) region (specifically Far Infrared).

Longest and Shortest Wavelengths

  • Core Principle: Energy and wavelength have an inverse relationship:     E=hcλE = \frac{hc}{\lambda}

  • Shortest Wavelength (Maximum Energy):

    • Occurs when the electron transitions from the furthest possible distance (ni=n_i = \infty) to the destination shell (nfn_f).

    • Energy is maximum because the transition spans the widest gap.

  • Longest Wavelength (Minimum Energy):

    • Occurs when the electron transitions from the shell immediately above the destination shell.

    • Condition: ni=nf+1n_i = n_f + 1.

Case Study: Calculations for Balmer Series

  • Balmer Shortest Wavelength:

    • nf=2n_f = 2, ni=n_i = \infty

    • 1λ=R(12212)\frac{1}{\lambda} = R \left( \frac{1}{2^2} - \frac{1}{\infty^2} \right)

    • 1λ=R×14λ=4R\frac{1}{\lambda} = R \times \frac{1}{4} \Rightarrow \lambda = \frac{4}{R}

    • Using R=1×107R = 1 \times 10^7, λ=4×107m=400nm\lambda = 4 \times 10^{-7} \, \text{m} = 400 \, \text{nm}.

  • Balmer Longest Wavelength:

    • nf=2n_f = 2, ni=3n_i = 3

    • 1λ=R(122132)\frac{1}{\lambda} = R \left( \frac{1}{2^2} - \frac{1}{3^2} \right)

    • 1λ=R(1419)=R(536)\frac{1}{\lambda} = R \left( \frac{1}{4} - \frac{1}{9} \right) = R \left( \frac{5}{36} \right)

    • λ=365R\lambda = \frac{36}{5R}

    • Result: Approximately 720nm720 \, \text{nm}.

Concept of X-Rays

  • General Properties: X-rays are highly energetic electromagnetic radiations with very short wavelengths.

  • Wavelength Order: Typically on the order of 1010m10^{-10} \, \text{m} or 1Angstrom1 \, \text{Angstrom}.

  • Order Comparison: Visible light has an order of 107m10^{-7} \, \text{m}, whereas X-rays are 1010m10^{-10} \, \text{m}.

Generation of X-Rays

  • Apparatus Components:

    • Cathode: Fires fast-moving electrons.

    • High Voltage Source (VV): Used to accelerate electrons from the cathode to the target.

    • Target Metal: Usually a Tungsten disc or similar high-density metal.

  • Electron Speed Formula: Potential energy provides the kinetic energy for the electron:     qΔV=12mv2q \Delta V = \frac{1}{2}mv^2     v=2qΔVmv = \sqrt{\frac{2q \Delta V}{m}}

Types of X-Rays

  1. Characteristic X-Rays:

    • Process: A fast-moving incoming electron strikes an inner-shell electron (e.g., in the K-shell) and knocks it out of the atom (Knockout Phenomenon).

    • Vacancy Fulfillment: A vacancy or 'hole' is created. Electrons from higher shells (L, M, N) jump down to fill this gap, emitting a photon.

    • Labeling (Kα,KβK_\alpha, K_\beta):

      • Letter (K, L, M) identifies where the vacancy occurred.

      • Greek letter indicates the jump distance: α\alpha is from the adjacent shell, β\beta is from one shell further away.

    • Characteristic Property: These values are constant for a specific element (e.g., Tungsten) because the shell energy levels are fixed for that element.

  2. Continuous X-Rays (Bremsstrahlung):

    • Process: A fast-moving electron passes near the nucleus. The nucleus's positive charge exerts an attractive force, slowing the electron down.

    • Bremsstrahlung Meaning: German for "Braking Radiation."

    • Energy Conversion: The kinetic energy lost by the electron during deceleration is emitted as a photon.

    • Energy Range: Energies can vary continuously because the closeness of the electron to the nucleus (and thus the deceleration) is not quantized.

The Phenomenon of Lasers

  • Definition: Light Amplification by Stimulated Emission of Radiation.

  • Energy States:

    1. Ground State: Most stable, lowest energy.

    2. Excited State: Highly unstable, very short life (108s10^{-8} \, \text{s}).

    3. Metastable State: Partial stability, longer life (103s10^{-3} \, \text{s}).

The Three Steps of Laser Production

  1. Induced Absorption (Step 1):

    • Ground state electrons are given energy via Optical Pumping to jump into the Excited State.

  2. Spontaneous Emission (Step 2):

    • Electrons naturally and quickly fall from the Excited State to the Metastable State. This happens without external intervention.

  3. Induced/Stimulated Emission (Step 3):

    • Population Inversion: The process is repeated until more electrons reside in the Metastable state than in the Ground state.

    • Stimulation: An external photon triggers the electrons in the metastable state to fall to the ground state simultaneously.

    • Output: The result is a highly directional, intense, and phase-coherent beam of light known as a Laser.

Questions & Discussion

  • Homework Assignments:

    • Calculate the Longest and Shortest wavelengths for Lyman, Paschen, Brackett, and Pfund series.

    • Determine the first three spectral lines for Balmer, Paschen, Brackett, and Pfund series.

  • Clarification on Balmer Series Constraints: A student asked if ni=1n_i = 1 is possible for the Balmer series. The response: No, because that would require energy absorption to move from shell 1 to shell 2, creating an absorption spectrum. We are studying the emission spectrum, where electrons must move from higher shells to shell 2.

  • M-Alpha Photon Scenario: If an MαM_\alpha photon is emitted, where was the vacancy? The vacancy was in the M-shell, and the electron jumped from the N-shell to fill it.