Electron shell: Difference between revisions

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In [[atomic spectroscopy]], an '''electron shell''' is  set of spatial orbitals with the same [[principal quantum number]] ''n''. There are ''n''<sup>2</sup> spatial orbitals in a shell, see [[hydrogen-like atom]]s. For instance, the ''n'' = 3 shell contains nine orbitals: one 3''s''-, three 3''p''-, and five 3''d''-orbitals. A shell is '''closed''' if all orbitals in it are doubly occupied, once with spin up (&alpha;) and once with spin down (&beta;). For example, the closed ''n'' = 1, 2, and 3 shells contain 2, 8, and 18 electrons, respectively.
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An  '''subshell''' is a set of 2''l''+1 spatial orbitals with a given principal quantum number ''n'' and a given [[Angular momentum (quantum)#Orbital angular momentum|orbital angular momentum quantum number]] ''l''. A subshell is  ''closed'', if there are 2(2''l''+1) electrons in the subshell.For instance the 2''p'' subshell in the neon atom contains 6 electrons and hence it is closed. Likewise in the cupper atom the 3''d'' subshell is closed (contains 10 electrons).  
In [[atomic spectroscopy]], an '''electron shell''' is   set of spatial orbitals with the same [[principal quantum number]] ''n''. There are ''n''<sup>2</sup> spatial orbitals in a shell; see [[hydrogen-like atom]]s. For instance, the ''n'' = 3 shell contains nine orbitals: one 3''s'', three 3''p'', and five 3''d'' orbitals. A shell is '''closed''' if all orbitals in it are doubly occupied, once with spin up (&alpha;) and once with spin down (&beta;). For example, the closed ''n'' = 1, 2, and 3 shells contain 2, 8, and 18 electrons, respectively.  
A subshell ''l''  containing a number of  electrons ''N'', with 1 &le; ''N'' < 2(2''l''+1), is called ''open''.  The  fluorine 2''p'' subshell, with electronic configuration 2''p''<sup>5</sup>, is open.  


A closed subshell is an eigenstate of total [[Angular momentum (quantum)#Orbital angular momentum|orbital angular momentum operator]] squared  '''L'''<sup>2</sup>  with quantum number ''L'' = 0. That is, the eigenvalue of '''L'''<sup>2</sup>, which has the general form ''L''(''L''+1), is zero. A closed subshell is also an eigenstate of total [[Angular momentum (quantum)#Spin angular momentum|spin angular momentum operator]] squared  '''S'''<sup>2</sup>  with quantum number ''S'' = 0. That is, the eigenvalue of '''S'''<sup>2</sup>, which has the general form ''S''(''S''+1), is zero.  The proof of these two statements will be omitted. Briefly, they rest on the fact that closed (sub)shells have wavefunctions that are [[Slater determinant#Atomic closed shells|Slater determinant]]s and that closed-shell Slater determinants  are invariant under the orbit and spin rotation groups, SO(3) and SU(2), respectively.
An  '''subshell''' is a set of 2''l'' + 1 spatial orbitals with a given principal quantum number ''n'' and a given [[Angular momentum (quantum)#Orbital angular momentum|orbital angular momentum quantum number]] ''l''. A subshell is  ''closed'', if there are 2(2''l'' + 1) electrons in the subshell. For instance, the 2''p'' subshell in the neon atom contains 6 electrons and, hence, it is closed. Likewise in the copper atom the 3''d'' subshell is closed (contains 10 electrons).
A subshell ''l''  containing a number of  electrons ''N'', with 1 &le; ''N'' < 2(2''l'' + 1),  is called ''open''.  The  fluorine 2''p'' subshell, with electronic configuration 2''p''<sup>5</sup>, is open.
 
A closed subshell is an eigenstate of total [[Angular momentum (quantum)#Orbital angular momentum|orbital angular momentum operator]] squared  '''L'''<sup>2</sup>  with quantum number ''L'' = 0. That is, the eigenvalue of '''L'''<sup>2</sup>, which has the general form ''L''(''L'' + 1), is zero. A closed subshell is also an eigenstate of total [[Angular momentum (quantum)#Spin angular momentum|spin angular momentum operator]] squared  '''S'''<sup>2</sup>  with quantum number ''S'' = 0. That is, the eigenvalue of '''S'''<sup>2</sup>, which has the general form ''S''(''S'' + 1), is zero.  The proof of these two statements will be omitted. Briefly, they rest on the fact that closed (sub)shells have wavefunctions that are [[Slater determinant#Atomic closed shells|Slater determinant]]s and that closed-shell Slater determinants  are invariant under the orbit and spin rotation groups, SO(3) and SU(2), respectively.


In the case of [[hydrogen-like atom|hydrogen-like]]&mdash;one-electron&mdash;atoms all  orbitals within one shell are degenerate, i.e., have the same orbital energy. In the case of more-electron atoms this degeneracy is lifted to a large extent. Provided the orbitals of more-electron atoms are solutions of rotationally invariant effective one-electron Hamiltonians, the orbitals of a ''subshell'' are still degenerate. This degeneracy of a subshell means that ''l'' is a "good" quantum number, that is, the one-particle angular momentum operator '''l'''<sup>2</sup> commutes with the effective one-electron Hamiltonian. This commutation occurs if, and only if, the effective one-electron Hamiltonian is rotationally invariant.
In the case of [[hydrogen-like atom|hydrogen-like]]&mdash;one-electron&mdash;atoms all  orbitals within one shell are degenerate, i.e., have the same orbital energy. In the case of more-electron atoms this degeneracy is lifted to a large extent. Provided the orbitals of more-electron atoms are solutions of rotationally invariant effective one-electron Hamiltonians, the orbitals of a ''subshell'' are still degenerate. This degeneracy of a subshell means that ''l'' is a "good" quantum number, that is, the one-particle angular momentum operator '''l'''<sup>2</sup> commutes with the effective one-electron Hamiltonian. This commutation occurs if, and only if, the effective one-electron Hamiltonian is rotationally invariant.


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In atomic spectroscopy, an electron shell is set of spatial orbitals with the same principal quantum number n. There are n2 spatial orbitals in a shell; see hydrogen-like atoms. For instance, the n = 3 shell contains nine orbitals: one 3s, three 3p, and five 3d orbitals. A shell is closed if all orbitals in it are doubly occupied, once with spin up (α) and once with spin down (β). For example, the closed n = 1, 2, and 3 shells contain 2, 8, and 18 electrons, respectively.

An subshell is a set of 2l + 1 spatial orbitals with a given principal quantum number n and a given orbital angular momentum quantum number l. A subshell is closed, if there are 2(2l + 1) electrons in the subshell. For instance, the 2p subshell in the neon atom contains 6 electrons and, hence, it is closed. Likewise in the copper atom the 3d subshell is closed (contains 10 electrons). A subshell l containing a number of electrons N, with 1 ≤ N < 2(2l + 1), is called open. The fluorine 2p subshell, with electronic configuration 2p5, is open.

A closed subshell is an eigenstate of total orbital angular momentum operator squared L2 with quantum number L = 0. That is, the eigenvalue of L2, which has the general form L(L + 1), is zero. A closed subshell is also an eigenstate of total spin angular momentum operator squared S2 with quantum number S = 0. That is, the eigenvalue of S2, which has the general form S(S + 1), is zero. The proof of these two statements will be omitted. Briefly, they rest on the fact that closed (sub)shells have wavefunctions that are Slater determinants and that closed-shell Slater determinants are invariant under the orbit and spin rotation groups, SO(3) and SU(2), respectively.

In the case of hydrogen-like—one-electron—atoms all orbitals within one shell are degenerate, i.e., have the same orbital energy. In the case of more-electron atoms this degeneracy is lifted to a large extent. Provided the orbitals of more-electron atoms are solutions of rotationally invariant effective one-electron Hamiltonians, the orbitals of a subshell are still degenerate. This degeneracy of a subshell means that l is a "good" quantum number, that is, the one-particle angular momentum operator l2 commutes with the effective one-electron Hamiltonian. This commutation occurs if, and only if, the effective one-electron Hamiltonian is rotationally invariant.

See also Hund's rules and Russell-Saunders coupling.