3.2 Many-electron atoms and electron configurations
4 min read•july 30, 2024
Many-electron atoms are complex systems that require sophisticated models to understand. The quantum mechanical approach becomes increasingly challenging as the number of electrons grows, necessitating approximation methods to solve the Schrödinger equation.
Electron configurations describe how electrons are arranged in atoms. The , , and govern these arrangements. Understanding these principles is crucial for predicting atomic properties and chemical behavior.
Multi-electron atoms
Quantum mechanical model for multi-electron atoms
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The Schrödinger equation can be applied to atoms with multiple electrons, but it becomes increasingly complex and cannot be solved exactly for atoms with more than one electron
The wave function for a multi-electron atom depends on the coordinates of all the electrons, making it a function of many variables
Approximation methods, such as the and density functional theory, are used to solve the Schrödinger equation for multi-electron atoms
Principles governing electron arrangement in multi-electron atoms
The Pauli exclusion principle states that no two electrons in an atom can have the same set of quantum numbers (n, l, ml, ms), which determines the arrangement of electrons in an atom
The aufbau principle describes the order in which electrons fill orbitals in a multi-electron atom, starting from the lowest energy orbital and progressing to higher energy orbitals
Electrons fill orbitals in the order of increasing energy: 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d, 5p, 6s, 4f, 5d, 6p, 7s, 5f, 6d, 7p
Hund's rule states that when there are degenerate orbitals (same n and l quantum numbers), electrons will occupy separate orbitals with parallel spins before pairing up in the same orbital with opposite spins
This minimizes electron-electron repulsion and results in a lower energy state for the atom
Electron configuration notation
Standard notation for electron configurations
Electron configurations are written using the standard notation, which includes the (n), the orbital type (s, p, d, f), and the number of electrons in each orbital as a superscript
For example, the electron configuration of carbon (Z=6) is 1s²2s²2p², and the electron configuration of iron (Z=26) is 1s²2s²2p⁶3s²3p⁶4s²3d⁶
The superscript indicates the number of electrons in each orbital, and the order of the orbitals follows the aufbau principle
Noble gas notation for electron configurations
The electron configuration can also be abbreviated using the , where the electron configuration of the preceding noble gas is represented by its chemical symbol in square brackets
For example, the electron configuration of iron can be written as [Ar] 4s²3d⁶, where [Ar] represents the electron configuration of argon (1s²2s²2p⁶3s²3p⁶)
This notation simplifies the representation of electron configurations for elements with many electrons
Ground state electron configuration
Determining the ground state electron configuration
The electron configuration of an atom can be determined by following the aufbau principle, Pauli exclusion principle, and Hund's rule
Electrons are added to the lowest available energy orbitals first, with no more than two electrons per orbital (Pauli exclusion principle) and with parallel spins in degenerate orbitals (Hund's rule)
For example, the ground state electron configuration of phosphorus (Z=15) is 1s²2s²2p⁶3s²3p³, which follows the aufbau principle and Hund's rule
Exceptions to the aufbau principle
Exceptions to the aufbau principle occur when the energy difference between two orbitals is small, and half-filled or completely filled subshells are more stable
For example, chromium (Z=24) has the electron configuration [Ar] 4s¹3d⁵ instead of [Ar] 4s²3d⁴, because the half-filled 3d subshell is more stable
Similarly, copper (Z=29) has the electron configuration [Ar] 4s¹3d¹⁰ instead of [Ar] 4s²3d⁹, because the completely filled 3d subshell is more stable
Valence electrons and chemical properties
Definition and significance of valence electrons
Valence electrons are the electrons in the outermost shell (highest principal quantum number) of an atom, which participate in chemical bonding and reactions
The number of valence electrons determines an element's chemical properties, such as its reactivity, oxidation state, and the types of bonds it can form
For example, alkali metals (group 1) have one valence electron and are highly reactive, while noble gases (group 18) have a complete octet of valence electrons and are chemically inert
Relationship between valence electrons and periodic trends
Elements in the same group of the periodic table have similar chemical properties because they have the same number of valence electrons
As you move down a group, the valence electrons are in higher principal quantum number shells, resulting in a larger and lower
As you move from left to right across a period, the number of valence electrons increases, resulting in a smaller atomic radius, higher ionization energy, and higher
Octet rule and chemical reactivity
Atoms tend to gain, lose, or share electrons to achieve a stable octet configuration (8 valence electrons) in their outermost shell, which is similar to the electron configuration of the nearest noble gas
The reactivity of an element is related to its electron configuration and the stability of its valence shell
Elements with one or two valence electrons (alkali and alkaline earth metals) tend to lose electrons and form cations
Elements with six or seven valence electrons (halogens and chalcogens) tend to gain electrons and form anions
For example, sodium (Na) has one valence electron and readily loses it to form Na⁺, while chlorine (Cl) has seven valence electrons and readily gains one to form Cl⁻, resulting in the formation of the ionic compound NaCl