5.1 Multi-electron atoms and the Pauli exclusion principle
4 min read•july 31, 2024
Multi-electron atoms are complex systems where electrons interact with each other and the nucleus. The , which states that no two electrons can have identical quantum states, shapes the electronic structure of these atoms.
This principle leads to the filling of electron orbitals in a specific order, forming shells and subshells. It explains periodic trends and is responsible for the stability of matter, preventing all electrons from collapsing into the lowest energy state.
Pauli Exclusion Principle Implications
Fundamental Concept and Atomic Structure
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Pauli exclusion principle states no two electrons in an atom can have the same set of quantum numbers
Shapes electronic structure of multi-electron atoms
Leads to filling of electron orbitals in specific order ( and )
Results in formation of electron shells and subshells
Determines chemical and physical properties of elements
Explains periodic trends across the periodic table
Atomic size
Ionization energy
Electron affinity
Stability and Consequences
Responsible for stability of matter
Prevents all electrons from collapsing into lowest energy state
Violation would lead to dramatic changes in behavior of matter and universe
Collapse of atomic structures (atoms would shrink dramatically)
Changes in chemical bonding (molecules would become unstable)
Alteration of stellar evolution (stars would behave differently)
Electron Spin in Atomic Structure
Fundamental Properties
Electron spin intrinsic angular momentum of electron
Characterized by spin quantum number (s) with values of +1/2 or -1/2
Quantum mechanical property with no classical analogue
Often visualized as electron rotating about its axis (not physically accurate)
Spin magnetic moment interacts with external magnetic fields
Leads to phenomena like Zeeman effect (splitting of in magnetic field)
Experimental Evidence and Applications
Stern-Gerlach experiment provided evidence for quantization of electron spin
Beam of silver atoms split into two distinct beams in non-uniform magnetic field
Crucial role in determining magnetic properties of atoms and materials
Ferromagnetism (iron, nickel, cobalt)
Antiferromagnetism (manganese oxide, chromium)
Spin-orbit coupling interaction between electron's spin and orbital angular momentum
Leads to fine structure in atomic spectra (splitting of spectral lines)
Quantum Mechanical Considerations
Combination of spin and spatial wavefunctions must be antisymmetric for fermions like electrons
Required by Pauli exclusion principle
Spin states can be represented as |↑⟩ and |↓⟩ in quantum mechanics
Spin angular momentum magnitude given by s(s+1)ℏ where s = 1/2 for electrons
Electron Configurations for Multi-electron Atoms
Notation and Orbital Filling
Electron configurations written using spectroscopic notation
Orbitals denoted by (n) and angular momentum quantum number (l)
Example: 1s² 2s² 2p⁶ 3s² 3p⁶ 4s² 3d¹⁰ (for zinc)
Maximum number of electrons in each subshell determined by 2(2l+1)
s orbitals (l=0): 2 electrons
p orbitals (l=1): 6 electrons
d orbitals (l=2): 10 electrons
f orbitals (l=3): 14 electrons
Hund's rule states electrons in degenerate orbitals occupy them singly with parallel spins before pairing
Minimizes
Example: Carbon ground state 1s² 2s² 2p² (two unpaired electrons in 2p orbitals)
Aufbau Principle and Exceptions
Aufbau principle dictates order of orbital filling: 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d, 5p, 6s, 4f, 5d, 6p, 7s, 5f, 6d, 7p
Exceptions occur due to increased stability of half-filled or completely filled subshells
Chromium: [Ar] 4s¹ 3d⁵ instead of [Ar] 4s² 3d⁴
Copper: [Ar] 4s¹ 3d¹⁰ instead of [Ar] 4s² 3d⁹
Lanthanides and actinides show complex filling patterns due to similar energies of f, d, and s orbitals
Valence Electrons and Excited States
in outermost shell largely determine chemical properties
Can be predicted using periodic table (group number for main group elements)
Excited state configurations involve promotion of electrons to higher energy levels
Subject to selection rules based on changes in quantum numbers (Δl = ±1, Δm = 0, ±1)
Example: Sodium excited state 1s² 2s² 2p⁶ 3p¹ (instead of ground state 3s¹)
Electron Shielding and Atomic Properties
Shielding Effect and Effective Nuclear Charge
Electron shielding (screening) reduces effective nuclear charge experienced by outer electrons
Shielding effect increases with principal quantum number (n) and decreases with angular momentum quantum number (l)
Penetration affects degree of shielding
Probability of electron being found close to nucleus
Order of penetration: s > p > d > f for orbitals of same principal quantum number
Effective nuclear charge (Zeff) calculated as actual nuclear charge minus shielding effect
Determines strength of electron-nucleus attraction
Example: Lithium Zeff for 2s electron ≈ 1.3 (actual Z = 3)
Periodic Trends and Anomalies
Shielding explains trend of decreasing ionization energy and increasing atomic radius across a period
Outer electrons less tightly bound due to increased shielding
Responsible for irregular trends in first ionization energies
Beryllium anomaly (higher than expected ionization energy due to filled 2s subshell)
Nitrogen anomaly (higher than oxygen due to half-filled 2p subshell)
Affects electron affinity trends
Noble gases have very low electron affinities due to complete outer shells
Multi-electron Atom Behavior
Shielding effect leads to departure from hydrogen-like behavior in multi-electron atoms
Results in more complex electron energy levels and spectral patterns
Splitting of energy levels due to electron-electron interactions
Multiple emission lines in spectra (compared to simple hydrogen spectrum)
Influences chemical bonding and molecular properties
Affects electronegativity and atomic size, impacting bond strengths and molecular geometries