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In-Depth Notes on Electronic Structure of Atoms

Electronic Structure of Atoms

Introduction to Electronic Structure
  • Nucleus Composition: An atom's nucleus consists of protons and neutrons, while electrons orbit around this nucleus.

  • Size Comparison: Electrons are approximately 1800 times smaller in mass than protons.

  • Wave Properties: Small particles can be described using wave properties in physics.

Understanding Electromagnetic Radiation
  • Nature of Electromagnetic Radiation: To comprehend an atom's electronic structure, one must understand electromagnetic radiation, which propagates as waves at the speed of light.

Key Terms
  • Wavelength ($\lambda$): Distance between corresponding points on adjacent waves.

  • Frequency ($v$): Number of waves that pass a given point in a specific time frame.

  • Relationship: For waves traveling at the same velocity, longer wavelengths correlate to smaller frequencies.

Properties of Electromagnetic Radiation
  • Speed of Light: All electromagnetic radiation travels at the speed of light, $c = 3 \times 10^8 \, m/s$.

  • Wavelength-Frequency Relationship: The relationship is given by the equation ( c = \lambda v ).

  • Visible Spectrum: Humans can only perceive a narrow region of the electromagnetic spectrum.

Types of Electromagnetic Radiation
  • Common Wavelength Units:

    • Angstrom ($10^{-10}$ m): X-ray

    • Nanometer (nm, $10^{-9}$ m): Ultraviolet, visible

    • Micrometer ($\mu m$, $10^{-6}$ m): Infrared

    • Millimeter (mm, $10^{-3}$ m): Microwave

    • Centimeter (cm, $10^{-2}$ m): Microwave

    • Meter (m): Television, radio

    • Kilometer (km, $10^{3}$ m): Radio

  • Diversity in Radiation: Types of electromagnetic radiation vary in wavelength and energy.

Quantized Energy and Photons
  • Key Observations of Atomic Interaction with Electromagnetic Radiation:

    1. Black Body Radiation: The light emitted from heated objects.

    2. Photoelectric Effect: Emission of electrons when light strikes a metal surface.

    3. Emission Spectra: Light emitted from excited gas atoms.

  • Wave Limitations: These phenomena cannot be solely explained through wave theories.

Black Body Radiation
  • Emission Mechanism: An object emits light when its temperature increases, which classical physics fails to explain adequately, predicting emissions of UV and X-rays that are not observed.

Concept of Quanta
  • Max Planck: Proposed energy exists in discrete packets called quanta (singular: quantum).

  • Analogy: Quanta can be likened to stairs (discrete) versus a ramp (continuous).

Photoelectric Effect
  • Einstein's Explanation: Quanta explain the photoelectric effect, where specific metals emit electrons at certain energy levels. The relation is expressed asE = h v

    • Where (h) is Planck's constant (6.626 \times 10^{-34} \, J \, s).

Atomic Emission of Gas
  • Emission Spectra Observations: Different line spectra are emitted from energy observed from gas atoms.

Line Spectra and the Bohr Model
  • Discrete Spectra: Only discrete wavelengths are observed for elements instead of continuous spectra.

  • Unique Spectra: Each element has a unique line spectrum.

The Hydrogen Spectrum and Rydberg's Formula
  • Mathematical Relationships: Rydberg derived formulas correlating wavelength with integers, termed Rydberg's constant ($R_H$).

  • Bohr's Assumptions: Energy exists in small packets (quanta), as described by Planck.

The Bohr Model (Hydrogen Atom)
  1. Allowed Orbits: Only certain orbits (specific radii) are permitted.

  2. Energy States: An electron in an allowed orbit is in an allowed energy state and does not radiate energy.

  3. Energy Transitions: Energy is emitted or absorbed as the electron changes states, expressed as:
    E = h v

Ground State and Excited State
  • Lowest Energy State: Electrons in the lowest energy state are termed the ground state (n=1).

  • Higher Energy States: Energy states are termed excited state (n>1).

Energy Transition Calculation
  • Energy Change: Calculating energy change between levels:
    \Delta E = Ef - Ei = -2.18 \times 10^{-18} J \left( \frac{1}{nf^2} - \frac{1}{ni^2} \right)

Energy and Photon Emission
  • Photon Emission: A positive (\Delta E) indicates energy absorption (photon absorbed) while a negative (\Delta E) indicates energy release (photon emitted).

Limitations of the Bohr Model
  1. Hydrogen Specific: Functional only for hydrogen (one electron).

  2. Assumption: Electrons do not spiral into the nucleus, a reality contradicting classical physics.

  3. Wave Properties: Electrons exhibit wave-like properties that the model does not address.

Important Ideas from the Bohr Model
  • Discrete Energy Levels: Electrons occupy specific energy levels defined by quantum numbers.

  • Energy Transitions: Energy involvement is crucial in electron state transitions.

Wave Behavior of Matter
  • Louis de Broglie: Proposed that if light can exhibit material properties, matter should demonstrate wave properties, with the relationship given by:
    \lambda = \frac{h}{mv}

Uncertainty Principle
  • Heisenberg's Conclusion: The more accurately the momentum is known, the less accurately the position can be determined:
    \Delta x \Delta p \geq \frac{h}{4\pi}

Quantum Mechanics and Atomic Orbitals
  • Schrödinger's Wave Equation: Provides a mathematical description of wave-particle duality, yielding wave functions for electrons. The square of a wave function gives electron density probabilities.

Orbitals and Quantum Numbers
  • Wave Functions: Solving the wave equation defines orbitals and their energies; an orbital represents the spatial distribution of electron density.

  • Electron Capacity: Each orbital can hold a maximum of two electrons.

Principal Quantum Number (n)
  • Energy Level Description: Positive integral values corresponding to energy levels; as n increases, orbitals become larger and the electrons are less tightly bound.

Angular Momentum Quantum Number (l)
  • Orbital Shape: Defines orbital shapes with integer values ranging 0 to n-1. Symbols for l:

    • s (l=0): Spherical

    • p (l=1): Dumbbell-shaped

    • d (l=2): Cloverleaf-shaped

    • f (l=3): Complex shapes

Magnetic Quantum Number (mₗ)
  • Orbital Orientation: Describes the 3D orientation of orbitals. Varies from -l to l, allowing multiple orbital configurations.

Quantum Numbers Summary
  • Electron Shells: Orbitals with the same n value form an electron shell. Subshells refer to different orbital types within the same energy level.

Representation of Orbitals
  • s Orbitals: Spherical shape; number of peaks corresponds to n; number of nodes (zero probability of finding electrons) is n-1.

  • p Orbitals: Two lobes with one node between them.

  • d Orbitals: Complex shapes with four of five d orbitals displaying lobes and one resembling a p orbital with a doughnut.

  • f Orbitals: Very complex with seven equivalent orbitals.

Hydrogen Atom Orbital Energies
  • All orbitals at the same energy level are degenerate for one-electron hydrogen atoms.

Many-Electron Atoms
  • In multi-electron atoms, electron repulsion causes orbital energy levels to vary; not all orbitals at the same energy level are degenerate.

Spin Quantum Number (mₛ)
  • Electron Spin: Two electrons in the same orbital exhibit different energies due to their spins, which can only take values of +1/2 or -1/2.

Pauli Exclusion Principle
  • Quantum Number Uniqueness: No two electrons can have identical sets of four quantum numbers, necessitating differences across at least one quantum number.

Electron Configurations
  • Definition: Distribution of electrons within an atom; the most stable arrangement occurs at the lowest energy state.

  • Components: Each electron configuration includes a number (energy level), a letter (type of orbital), and superscript (number of electrons).

Orbital Diagrams
  • Visualization: Orbital diagrams depict orbitals and their electron fills, utilizing arrows denoting electron spin direction, adhering to Hund's Rule and Pauli's Exclusion Principle.

Condensed Electron Configurations
  • Core and Valence Electrons: Core electrons are primarily from noble gases; only valence electrons are listed in condensed electronic configurations.

Transition Metals and Anomalies
  • Electron Filling Sequence: Transition metals fill the 4s orbital before the 3d, with special configurations observed during half-filled or filled states.

  • Examples: Chromium exhibits anomalies in electron configurations due to energy proximity of the 4s and 3d orbitals.

Conclusion
  • Understanding the electronic structure of atoms requires the combination of concepts from classical and quantum physics, resulting in a more comprehensive model of atomic behavior.

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