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Introduction

Atoms are fundamental units of matter, once thought indivisible but now known to consist of subatomic particles: electrons, protons, and neutrons. Understanding atomic structure is key to explaining chemical and physical properties of elements.

Discovery of Subatomic Particles

1. Electron (J.J. Thomson, 1897):

  • Identified via cathode ray experiments; negatively charged, mass ~1/1837 of H atom.
  • Charge: -1.602 × 10⁻¹⁹ C; Mass: 9.109 × 10⁻³¹ kg.

2. Proton (Rutherford, 1919):

  • Found via anode rays (canal rays); positively charged, mass ~1836 times electron.
  • Charge: +1.602 × 10⁻¹⁹ C; Mass: 1.672 × 10⁻²⁷ kg.

3. Neutron (James Chadwick, 1932):

  • Neutral particle, slightly heavier than proton; Mass: 1.675 × 10⁻²⁷ kg.
  • Charge and Mass Comparison:

Structure of Atom Revision Notes | Chemistry Class 11 - NEET

Atomic Models

 1. Thomson’s Model (1904)

  • Atom as a positively charged sphere with embedded electrons (plum pudding model).
  • Limitation: Could not explain electron stability or spectral lines.Structure of Atom Revision Notes | Chemistry Class 11 - NEET

2. Rutherford’s Model (1911)

  • Based on alpha particle scattering:Structure of Atom Revision Notes | Chemistry Class 11 - NEET
    • Nucleus: Small, dense, positively charged center containing most mass.
    • Electrons: Orbit nucleus like planets around the sun.
  • Limitation: Electrons should emit energy and spiral into nucleus, contradicting atomic stability.

Atomic Number and Mass Number

  • Atomic Number (Z): Number of protons (defines element), e.g., H (Z=1), C (Z=6).
  • Mass Number (A): Protons + neutrons, e.g., ¹²C (A=12, Z=6, neutrons=6).
  • Isotopes: Same Z, different A (e.g., ¹²C, ¹⁴C).
  • Isobars: Same A, different Z (e.g., ¹⁴C, ¹⁴N).
  • Notation: ⁿₘX, where X is element, m is A, n is Z (e.g., ¹²₆C).

Developments Leading to Bohr’s Model

  • Electromagnetic Waves: Maxwell’s theory; light as waves with wavelength (λ), frequency (ν), speed (c = λν).
  • Planck’s Quantum Theory (1900): Energy emitted/absorbed in quanta (E = hν, h = 6.626 × 10⁻³⁴ J s).
  • Einstein’s Photoelectric Effect (1905): Light quanta (photons) eject electrons; energy threshold required.
  • Atomic Spectra:
    • Emission: Light emitted by energized atoms (e.g., hydrogen’s line spectrum).
    • Absorption: Light absorbed by atoms, forming dark lines.
  • Hydrogen Spectrum: Lyman (UV), Balmer (visible), Paschen, Brackett, Pfund (IR); Rydberg formula: 1/λ = R(1/n₁² - 1/n₂²), R = 109677 cm⁻¹.

Bohr’s Model for Hydrogen Atom (1913)

  • Postulates:
    • Electrons orbit nucleus in fixed energy levels (orbits) without radiating energy.
    • Energy levels quantized: Eₙ = -2.18 × 10⁻¹⁸/n² J (n = principal quantum number).
    • Electron transitions emit/absorb energy: ΔE = E₂ - E₁ = hν.
  • Radius: rₙ = 0.529 × n²/Z Å (H: n=1, r=0.529 Å).
  • Velocity: vₙ = 2.188 × 10⁶ × Z/n m/s.
  • Success: Explained hydrogen spectrum, atomic stability.
  • Limitations: Failed for multi-electron atoms, ignored electron spin, contradicted Heisenberg’s uncertainty principle.

Towards Quantum Mechanical Model

Dual Nature of Matter:

  • de Broglie (1924): Particles have wave properties; λ = h/mv (h = Planck’s constant, m = mass, v = velocity).
  • Example: Electron at 100 V, λ = 1.227/√V nm.Structure of Atom Revision Notes | Chemistry Class 11 - NEET

Heisenberg’s Uncertainty Principle (1927): Cannot know exact position and momentum simultaneously; Δx × Δp ≥ h/4π.

Quantum Mechanical Model

  • Schrödinger’s Wave Equation: Treats electrons as waves, solved for orbitals (probability regions).
  • Orbitals: Defined by quantum numbers:
    • Principal (n): Energy level (1, 2, 3, …).
    • Azimuthal (l): Subshell (0 to n-1; s, p, d, f).
    • Magnetic (mₗ): Orbital orientation (-l to +l).
    • Spin (mₛ): Electron spin (+1/2 or -1/2).
  • Probability Density: ψ² gives electron likelihood.

Shapes of Atomic Orbitals

  • s-Orbital (l=0): Spherical, size increases with n.Structure of Atom Revision Notes | Chemistry Class 11 - NEET
  • p-Orbital (l=1): Dumbbell-shaped, three orientations (px, py, pz).Structure of Atom Revision Notes | Chemistry Class 11 - NEET
  • d-Orbital (l=2): Five orientations, complex shapes.Structure of Atom Revision Notes | Chemistry Class 11 - NEET
  • Nodes: Regions of zero electron density (e.g., 2s has one spherical node).

Energies of Orbitals

  • Hydrogen: Energy depends only on n (Eₙ = -13.6/n² eV).
  • Multi-electron Atoms: Energy depends on n and l (e.g., 3s < 3p < 3d due to penetration effect).Structure of Atom Revision Notes | Chemistry Class 11 - NEETEnergy Level Diagram

Filling of Orbitals

  • Aufbau Principle: Electrons fill lowest energy orbitals first (1s, 2s, 2p, 3s, …).
  • Pauli Exclusion Principle: No two electrons have identical four quantum numbers; max 2 electrons per orbital with opposite spins.
  • Hund’s Rule: Electrons pair only after singly occupying degenerate orbitals with parallel spins.
  • Configurations: e.g., C (Z=6): 1s²2s²2p²; exceptions like Cr (3d⁵4s¹) for stability.Structure of Atom Revision Notes | Chemistry Class 11 - NEETOrder of filling of orbitals

Summary

Atoms consist of electrons, protons, and neutrons. Thomson’s plum pudding model evolved into Rutherford’s nuclear model, refined by Bohr’s quantized orbits for hydrogen. Quantum mechanics, with de Broglie’s wave-particle duality and Schrödinger’s orbitals, describes electron probability via quantum numbers (n, l, mₗ, mₛ). Orbital shapes (s, p, d) and energy levels guide electron filling per Aufbau, Pauli, and Hund’s rules, explaining atomic properties.

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FAQs on Structure of Atom Revision Notes - Chemistry Class 11 - NEET

1. What are the key differences between the classical and quantum models of the atom?
Ans. The classical model depicts electrons moving in fixed orbits around the nucleus, similar to planets orbiting the sun. In contrast, the quantum model describes electrons as existing in probabilistic clouds or orbitals, where their exact position cannot be determined. The quantum model incorporates principles of wave-particle duality and uncertainty, which are not present in the classical model.
2. How do electromagnetic waves relate to atomic spectra?
Ans. Electromagnetic waves are produced when electrons transition between energy levels within an atom. When an electron absorbs energy, it can jump to a higher energy level; when it falls back to a lower level, it emits electromagnetic radiation. The wavelengths of this radiation correspond to specific frequencies and result in the atomic spectra unique to each element, often observed as lines in a spectrum.
3. What is the significance of quantum numbers in describing electron configurations?
Ans. Quantum numbers provide a way to describe the unique state of an electron in an atom. There are four quantum numbers: the principal quantum number (n), which indicates the energy level; the azimuthal quantum number (l), which indicates the subshell shape; the magnetic quantum number (m_l), which indicates the orientation of the orbital; and the spin quantum number (m_s), which indicates the spin direction of the electron. Together, these numbers help in determining the arrangement of electrons in an atom and their energy levels.
4. What is the concept of wave-particle duality in relation to electrons?
Ans. Wave-particle duality refers to the phenomenon where particles, such as electrons, exhibit both wave-like and particle-like properties. In the context of electrons, this means they can behave like waves, demonstrating interference and diffraction, while also behaving like particles with discrete locations. This duality is a fundamental principle of quantum mechanics and is crucial for understanding atomic behavior and electron interactions.
5. How does the stability of atomic spectra relate to electron configurations?
Ans. The stability of atomic spectra is closely tied to electron configurations because electrons occupy the lowest available energy levels first, following the Aufbau principle. Stable configurations, such as full or half-full subshells, tend to result in more distinct and clearer spectral lines. Conversely, unstable configurations can lead to more complex spectra due to the presence of excited states and transitions that are not as well-defined. This stability is important for predicting and understanding the behavior of elements in various chemical contexts.
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