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Term symbol

From Wikipedia, the free encyclopedia
Notation in quantum physics
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Inatomic physics, aterm symbol is an abbreviated description of the total spin and orbitalangular momentum quantum numbers of the electrons in a multi-electronatom. So while the wordsymbol suggests otherwise, it represents an actualvalue of aphysical quantity.

For a givenelectron configuration of an atom, its state depends also on its total angular momentum, including spin and orbital components, which are specified by the term symbol. The usual atomic term symbols assumeLS coupling (also known as Russell–Saunders coupling) in which the all-electron total quantum numbers for orbital (L), spin (S) and total (J) angular momenta aregood quantum numbers.

In the terminology ofatomic spectroscopy,L andS together specify aterm;L,S, andJ specify alevel; andL,S,J and the magnetic quantum numberMJ specify astate. The conventional term symbol has the form2S+1LJ, whereJ is written optionally in order to specify a level.L is written usingspectroscopic notation: for example, it is written "S", "P", "D", or "F" to representL = 0, 1, 2, or 3 respectively. For coupling schemes other that LS coupling, such as thejj coupling that applies to some heavy elements, other notations are used to specify the term.

Term symbols apply to both neutral and charged atoms, and to their ground and excited states. Term symbols usually specify the total for all electrons in an atom, but are sometimes used to describe electrons in a givensubshell or set of subshells, for example to describe eachopen subshell in an atom having more than one. Theground state term symbol for neutral atoms is described, in most cases, byHund's rules. Neutral atoms of the chemical elements have the same term symbolfor each column in thes-block and p-block elements, but differ in d-block and f-block elements where the ground-state electron configuration changes within a column, where exceptions to Hund's rules occur. Ground state term symbols for the chemical elements are givenbelow.

Term symbols are also used to describe angular momentum quantum numbers foratomic nuclei and for molecules. Formolecular term symbols, Greek letters are used to designate the component of orbital angular momenta along the molecular axis.

The use of the wordterm for an atom's electronic state is based on theRydberg–Ritz combination principle, an empirical observation that the wavenumbers of spectral lines can be expressed as the difference of twoterms. This was later summarized by theBohr model, which identified the terms with quantized energy levels, and the spectral wavenumbers of these levels with photon energies.

Tables of atomic energy levels identified by their term symbols are available for atoms and ions in ground and excited states from theNational Institute of Standards and Technology (NIST).[1]

Term symbols withLS coupling

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The usual atomic term symbols assumeLS coupling (also known as Russell–Saunders coupling), in which the atom's total spin quantum numberS and the total orbital angular momentum quantum numberL are "good quantum numbers". (Russell–Saunders coupling is named afterHenry Norris Russell andFrederick Albert Saunders, who described it in 1925[2]). Thespin-orbit interaction then couples the total spin and orbital moments to give the total electronic angular momentum quantum numberJ. Atomic states are then well described by term symbols of the form:

2S+1LJ{\displaystyle ^{2S+1}L_{J}}

where

The orbital symbols S, P, D and F are derived from the characteristics of the spectroscopic lines corresponding to s, p, d, and f orbitals:sharp,principal,diffuse, andfundamental; the rest are named in alphabetical order from G onwards (omitting J, S and P). When used to describe electronic states of an atom, the term symbol is often written following theelectron configuration. For example, 1s22s22p2 3P0 represents the ground state of a neutralcarbon atom. The superscript 3 indicates that the spin multiplicity 2S + 1 is 3 (it is atriplet state), soS = 1; the letter "P" is spectroscopic notation forL = 1; and the subscript 0 is the value ofJ (in this caseJ =LS).[1]

Small letters refer to individual orbitals or one-electron quantum numbers, whereas capital letters refer to many-electron states or their quantum numbers.

Terminology: terms, levels, and states

[edit]

For a given electron configuration,

The product(2S+1)(2L+1){\displaystyle (2S+1)(2L+1)} as a number of possible states|S,MS,L,ML{\displaystyle |S,M_{S},L,M_{L}\rangle } with givenS andL is also a number of basis states in the uncoupled representation, whereS{\displaystyle S},MS{\displaystyle M_{S}},L{\displaystyle L},ML{\displaystyle M_{L}} (MS{\displaystyle M_{S}} andML{\displaystyle M_{L}} are z-axis components of total spin and total orbital angular momentum respectively) are good quantum numbers whose corresponding operators mutually commute. With givenS{\displaystyle S} andL{\displaystyle L}, the eigenstates|S,MS,L,ML{\displaystyle |S,M_{S},L,M_{L}\rangle } in this representation span function space of dimension(2S+1)(2L+1){\displaystyle (2S+1)(2L+1)}, asMS=S,S1,,S+1,S{\displaystyle M_{S}=S,S-1,\dots ,-S+1,-S} andML=L,L1,...,L+1,L{\displaystyle M_{L}=L,L-1,...,-L+1,-L}. In the coupled representation where total angular momentum (spin + orbital) is treated, the associated states (oreigenstates) are|J,MJ,S,L{\displaystyle |J,M_{J},S,L\rangle } and these states span the function space with dimension of

J=Jmin=|LS|Jmax=L+S(2J+1){\displaystyle \sum _{J=J_{\min }=|L-S|}^{J_{\max }=L+S}(2J+1)}

asMJ=J,J1,,J+1,J{\displaystyle M_{J}=J,J-1,\dots ,-J+1,-J}. Obviously, the dimension of function space in both representations must be the same.

As an example, forS=1,L=2{\displaystyle S=1,L=2}, there are(2×1+1)(2×2+1) = 15 different states (= eigenstates in the uncoupled representation) corresponding to the3Dterm, of which(2×3+1) = 7 belong to the3D3 (J = 3) level. The sum of(2J+1){\displaystyle (2J+1)} for all levels in the same term equals (2S+1)(2L+1) as the dimensions of both representations must be equal as described above. In this case,J can be 1, 2, or 3, so 3 + 5 + 7 = 15.

Term symbol parity

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The parity of a term symbol is calculated as

P=(1)ii,{\displaystyle P=(-1)^{\sum _{i}\ell _{i}},}

wherei{\displaystyle \ell _{i}} is the orbital quantum number for each electron.P=1{\displaystyle P=1} means even parity whileP=1{\displaystyle P=-1} is for odd parity. In fact, only electrons in odd orbitals (with{\displaystyle \ell } odd) contribute to the total parity: an odd number of electrons in odd orbitals (those with an odd{\displaystyle \ell } such as in p, f, ...) correspond to an odd term symbol, while an even number of electrons in odd orbitals correspond to an even term symbol. The number of electrons in even orbitals is irrelevant as any sum of even numbers is even. For any closed subshell, the number of electrons is2(2+1){\displaystyle 2(2\ell +1)} which is even, so the summation ofi{\displaystyle \ell _{i}} in closed subshells is always an even number. The summation of quantum numbersii{\textstyle \sum _{i}\ell _{i}} over open (unfilled) subshells of odd orbitals ({\displaystyle \ell } odd) determines the parity of the term symbol. If the number of electrons in thisreduced summation is odd (even) then the parity is also odd (even).

When it is odd, the parity of the term symbol is indicated by a superscript letter "o", otherwise it is omitted:

2Po
12
has odd parity, but3P0 has even parity.

Alternatively, parity may be indicated with a subscript letter "g" or "u", standing forgerade (German for "even") orungerade ("odd"):

2P12,u for odd parity, and3P0,g for even.

Ground state term symbol

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It is relatively easy to predict the term symbol for the ground state of an atom usingHund's rules. It corresponds to a state with maximumS andL.

  1. Start with the most stableelectron configuration. Full shells and subshells do not contribute to the overallangular momentum, so they are discarded.
    • If all shells and subshells are full then the term symbol is1S0.
  2. Distribute the electrons in the availableorbitals, following thePauli exclusion principle.
    • Conventionally, put 1 electron into orbital with highestm and then continue filling other orbitals in descendingm order with one electron each, until you are out of electrons, or all orbitals in the subshell have one electron. Assign, again conventionally, all these electrons a value +12 of quantum magnetic spin numberms.
    • If there are remaining electrons, put them in orbitals in the same order as before, but now assigningms = −12 to them.
  3. The overallS is calculated by adding thems values for each electron. The overallS is then12 times the number ofunpaired electrons.
  4. The overallL is calculated by adding them{\displaystyle m_{\ell }} values for each electron (so if there are two electrons in the same orbital, add twice that orbital'sm{\displaystyle m_{\ell }}).
  5. CalculateJ as
    • if less than half of the subshell is occupied, take the minimum valueJ = |LS|;
    • if more than half-filled, take the maximum valueJ =L +S;
    • if the subshell is half-filled, thenL will be 0, soJ =S.

As an example, in the case offluorine, the electronic configuration is 1s22s22p5.

  1. Discard the full subshells and keep the 2p5 part. So there are five electrons to place in subshell p (=1{\displaystyle \ell =1}).
  2. There are three orbitals (m=1,0,1{\displaystyle m_{\ell }=1,0,-1}) that can hold up to2(2+1)=6{\displaystyle 2(2\ell +1)=6} electrons. The first three electrons can takems =12 (↑) but the Pauli exclusion principle forces the next two to havems = −12 (↓) because they go to already occupied orbitals.
    m{\displaystyle m_{\ell }}
    +10−1
    ms{\displaystyle m_{s}}↑↓↑↓
  3. S =12 +12 +121212 =12;
  4. L = 1 + 0 − 1 + 1 + 0 = 1, which is "P" in spectroscopic notation.
  5. As fluorine 2p subshell is more than half filled,J =L +S =32. Its ground state term symbol is then2S+1LJ =2P32.

Atomic term symbols of the chemical elements

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In the periodic table, because atoms of elements in a column usually have the same outer electron structure, and always have the same electron structure in the "s-block" and "p-block" elements (seeblock (periodic table)), all elements may share the same ground state term symbol for the column. Thus, hydrogen and thealkali metals are all2S12, thealkaline earth metals are1S0, theboron group elements are2P12, thecarbon group elements are3P0, thepnictogens are4S32, thechalcogens are3P2, thehalogens are2P32, and theinert gases are1S0, per the rule for full shells and subshells stated above.

Term symbols for the ground states of most chemical elements[3] are given in the collapsed table below.[4] In the d-block and f-block, the term symbols are not always the same for elements in the same column of the periodic table, because open shells of several d or f electrons have several closely spaced terms whose energy ordering is often perturbed by the addition of an extra complete shell to form the next element in the column.

For example, the table shows that the first pair of vertically adjacent atoms with different ground-state term symbols are V and Nb. The6D12 ground state of Nb corresponds to an excited state of V 2112 cm−1 above the4F32 ground state of V, which in turn corresponds to an excited state of Nb 1143 cm−1 above the Nb ground state.[1] These energy differences are small compared to the 15158 cm−1 difference between the ground and first excited state of Ca,[1] which is the last element before V with no d electrons.

Term symbol of the chemical elements
Group →123456789101112131415161718
↓ Period
1H
2S1/2

He
1S0
2Li
2S1/2
Be
1S0

B
2P1/2
C
3P0
N
4S3/2
O
3P2
F
2P3/2
Ne
1S0
3Na
2S1/2
Mg
1S0

Al
2P1/2
Si
3P0
P
4S3/2
S
3P2
Cl
2P3/2
Ar
1S0
4K
2S1/2
Ca
1S0
Sc
2D3/2
Ti
3F2
V
4F3/2
Cr
7S3
Mn
6S5/2
Fe
5D4
Co
4F9/2
Ni
3F4
Cu
2S1/2
Zn
1S0
Ga
2P1/2
Ge
3P0
As
4S3/2
Se
3P2
Br
2P3/2
Kr
1S0
5Rb
2S1/2
Sr
1S0
Y
2D3/2
Zr
3F2
Nb
6D1/2
Mo
7S3
Tc
6S5/2
Ru
5F5
Rh
4F9/2
Pd
1S0
Ag
2S1/2
Cd
1S0
In
2P1/2
Sn
3P0
Sb
4S3/2
Te
3P2
I
2P3/2
Xe
1S0
6Cs
2S1/2
Ba
1S0
1 asteriskLu
2D3/2
Hf
3F2
Ta
4F3/2
W
5D0
Re
6S5/2
Os
5D4
Ir
4F9/2
Pt
3D3
Au
2S1/2
Hg
1S0
Tl
2P1/2
Pb
3P0
Bi
4S3/2
Po
3P2
At
2P3/2
Rn
1S0
7Fr
2S1/2
Ra
1S0
1 asteriskLr
2P1/2?
Rf
3F2
Db
4F3/2?
Sg
5D0?
Bh
6S5/2?
Hs
5D4?
Mt
4F9/2?
Ds
3F4?
Rg
2D5/2?
Cn
1S0?
Nh
2P1/2?
Fl
3P0?
Mc
4S3/2?
Lv
3P2?
Ts
2P3/2?
Og
1S0?

1 asteriskLa
2D3/2
Ce
1G4
Pr
4I9/2
Nd
5I4
Pm
6H5/2
Sm
7F0
Eu
8S7/2
Gd
9D2
Tb
6H15/2
Dy
5I8
Ho
4I15/2
Er
3H6
Tm
2F7/2
Yb
1S0
1 asteriskAc
2D3/2
Th
3F2
Pa
4K11/2
U
5L6
Np
6L11/2
Pu
7F0
Am
8S7/2
Cm
9D2
Bk
6H15/2
Cf
5I8
Es
4I15/2
Fm
3H6
Md
2F7/2
No
1S0

Term symbols for an electron configuration

[edit]

The process to calculate all possible term symbols for a givenelectron configuration is somewhat longer.

  • First, the total number of possible statesN is calculated for a given electron configuration. As before, the filled (sub)shells are discarded, and only the partially filled ones are kept. For a given orbital quantum number{\displaystyle \ell },t is the maximum allowed number of electrons,t=2(2+1){\displaystyle t=2(2\ell +1)}. If there aree electrons in a given subshell, the number of possible states is

    As an example, consider thecarbon electron structure: 1s22s22p2. After removing full subshells, there are 2 electrons in a p-level (=1{\displaystyle \ell =1}), so there are

    different states.

  • Second, all possible states are drawn.ML andMS for each state are calculated, withM=i=1emi{\displaystyle M=\sum _{i=1}^{e}m_{i}} wheremi is eitherm{\displaystyle m_{\ell }} orms{\displaystyle m_{s}} for thei-th electron, andM represents the resultingML orMS respectively:
     m{\displaystyle m_{\ell }} 
     +10−1MLMS
    all up11
    01
    −11
    all down1−1
    0−1
    −1−1
    one up
    one down
    ↑↓20
    10
    00
    10
    ↑↓00
    −10
    00
    −10
    ↑↓−20
  • Third, the number of states for each (ML,MS) possible combination is counted:
     MS
     +10−1
    ML+21
    +1121
    0131
    −1121
    −21
  • Fourth, smaller tables can be extracted representing each possible term. Each table will have the size (2L+1) by (2S+1), and will contain only "1"s as entries. The first table extracted corresponds toML ranging from −2 to +2 (soL = 2), with a single value forMS (implyingS = 0). This corresponds to a1D term. The remaining terms fit inside the middle 3×3 portion of the table above. Then a second table can be extracted, removing the entries forML andMS both ranging from −1 to +1 (and soS =L = 1, a3P term). The remaining table is a 1×1 table, withL =S = 0, i.e., a1S term.
    S = 0,L = 2,J = 2
    1D2
     MS
     0
    ML+21
    +11
    01
    −11
    −21
    S=1,L=1,J=2,1,0
    3P2,3P1,3P0
     MS
     +10−1
    ML+1111
    0111
    −1111
    S=0,L=0,J=0
    1S0
     MS
     0
    ML01
  • Fifth, applyingHund's rules, the ground state can be identified (or the lowest state for the configuration of interest). Hund's rules should not be used to predict the order of states other than the lowest for a given configuration. (See examples atHund's rules § Excited states.)
  • If only two equivalent electrons are involved, there is an "Even Rule" which states that, for two equivalent electrons, the only states that are allowed are those for which the sum (L + S) is even.

Case of three equivalent electrons

[edit]

Alternative method using group theory

[edit]

For configurations with at most two electrons (or holes) per subshell, an alternative and much quicker method of arriving at the same result can be obtained fromgroup theory. The configuration 2p2 has the symmetry of the following direct product in the full rotation group:

Γ(1) × Γ(1) = Γ(0) + [Γ(1)] + Γ(2),

which, using the familiar labelsΓ(0) = S,Γ(1) = P andΓ(2) = D, can be written as

P × P = S + [P] + D.

The square brackets enclose the anti-symmetric square. Hence the 2p2 configuration has components with the following symmetries:

S + D (from the symmetric square and hence having symmetric spatial wavefunctions);
P (from the anti-symmetric square and hence having an anti-symmetric spatial wavefunction).

The Pauli principle and the requirement for electrons to be described by anti-symmetric wavefunctions imply that only the following combinations of spatial and spin symmetry are allowed:

1S +1D (spatially symmetric, spin anti-symmetric)
3P (spatially anti-symmetric, spin symmetric).

Then one can move to step five in the procedure above, applying Hund's rules.

The group theory method can be carried out for other such configurations, like 3d2, using the general formula

Γ(j) × Γ(j) = Γ(2j) + Γ(2j−2) + ⋯ + Γ(0) + [Γ(2j−1) + ⋯ + Γ(1)].

The symmetric square will give rise to singlets (such as1S,1D, &1G), while the anti-symmetric square gives rise to triplets (such as3P &3F).

More generally, one can use

Γ(j) × Γ(k) = Γ(j+k) + Γ(j+k−1) + ⋯ + Γ(|jk|)

where, since the product is not a square, it is not split into symmetric and anti-symmetric parts. Where two electrons come from inequivalent orbitals, both a singlet and a triplet are allowed in each case.[6]

Summary of various coupling schemes and corresponding term symbols

[edit]

Basic concepts for all coupling schemes:

LS coupling (Russell–Saunders coupling)

[edit]

jj Coupling

[edit]

J1L2 coupling

[edit]

LS1 coupling

[edit]

Most famous coupling schemes are introduced here but these schemes can be mixed to express the energy state of an atom. This summary is based on[1].

Racah notation and Paschen notation

[edit]

These are notations for describing states of singly excited atoms, especiallynoble gas atoms. Racah notation is basically a combination ofLS or Russell–Saunders coupling andJ1L2 coupling.LS coupling is for a parent ion andJ1L2 coupling is for a coupling of the parent ion and the excited electron. The parent ion is an unexcited part of the atom. For example, in Ar atom excited from a ground state ...3p6 to an excited state ...3p54p in electronic configuration, 3p5 is for the parent ion while 4p is for the excited electron.[8]

In Racah notation, states of excited atoms are denoted as((2S1+1)L1J1)n[K]Jo{\displaystyle \left(^{\left(2{{S}_{1}}+1\right)}{{L}_{1}}_{{J}_{1}}\right)n\ell \left[K\right]_{J}^{o}}. Quantities with a subscript 1 are for the parent ion,n and are principal and orbital quantum numbers for the excited electron,K andJ are quantum numbers forK=J1+{\displaystyle \mathbf {K} =\mathbf {J} _{1}+{\boldsymbol {\ell }}} andJ=K+s{\displaystyle \mathbf {J} =\mathbf {K} +\mathbf {s} } where{\displaystyle {\boldsymbol {\ell }}} ands{\displaystyle \mathbf {s} } are orbital angular momentum and spin for the excited electron respectively. “o” represents a parity of excited atom. For an inert (noble) gas atom, usual excited states areNp5nℓ whereN = 2, 3, 4, 5, 6 for Ne, Ar, Kr, Xe, Rn, respectively in order. Since the parent ion can only be2P1/2 or2P3/2, the notation can be shortened ton[K]Jo{\displaystyle n\ell \left[K\right]_{J}^{o}} orn[K]Jo{\displaystyle n\ell '\left[K\right]_{J}^{o}}, wherenℓ means the parent ion is in2P3/2 whilenℓ′ is for the parent ion in2P1/2 state.

Paschen notation is a somewhat odd notation; it is an old notation made to attempt to fit an emission spectrum of neon to a hydrogen-like theory. It has a rather simple structure to indicate energy levels of an excited atom. The energy levels are denoted asn′ℓ#. is just an orbital quantum number of the excited electron.n′ℓ is written in a way that 1s for(n =N + 1, = 0), 2p for(n =N + 1, = 1), 2s for(n =N + 2, = 0), 3p for(n =N + 2, = 1), 3s for(n =N + 3, = 0), etc. Rules of writingn′ℓ from the lowest electronic configuration of the excited electron are: (1) is written first, (2)n′ is consecutively written from 1 and the relation of =n′ − 1,n′ − 2, ... , 0 (like a relation betweenn and) is kept.n′ℓ is an attempt to describe electronic configuration of the excited electron in a way of describing electronic configuration of hydrogen atom.# is an additional number denoted to each energy level of givenn′ℓ (there can be multiple energy levels of given electronic configuration, denoted by the term symbol).# denotes each level in order, for example,# = 10 is for a lower energy level than# = 9 level and# = 1 is for the highest level in a givenn′ℓ. An example of Paschen notation is below.

Electronic configuration of Neonn′ℓElectronic configuration of Argonn′ℓ
1s22s22p6Ground state[Ne]3s23p6Ground state
1s22s22p53s11s[Ne]3s23p54s11s
1s22s22p53p12p[Ne]3s23p54p12p
1s22s22p54s12s[Ne]3s23p55s12s
1s22s22p54p13p[Ne]3s23p55p13p
1s22s22p55s13s[Ne]3s23p56s13s

See also

[edit]

Notes

[edit]
  1. ^There is no official convention for naming orbital angular momentum values greater than 20 (symbolZ) but they are rarely needed. Some authors use Greek letters (α, β, γ, ...) afterZ.

References

[edit]
  1. ^abcdNIST Atomic Spectrum Database For example, to display the levels for a neutral carbon atom, enter "C I" or "C 0" in the "Spectrum" box and click "Retrieve data".
  2. ^Russell, H. N.; Saunders, F. A. (1925) [January 1925]."New Regularities in the Spectra of the Alkaline Earths". SAO/NASA Astrophysics Data System (ADS).Astrophysical Journal.61. adsabs.harvard.edu/: 38.Bibcode:1925ApJ....61...38R.doi:10.1086/142872. RetrievedDecember 13, 2020 – via harvard.edu.
  3. ^"NIST Atomic Spectra Database Ionization Energies Form".NIST Physical Measurement Laboratory. National Institute of Standards and Technology (NIST). October 2018. Retrieved28 January 2019.This form provides access to NIST critically evaluated data on ground states and ionization energies of atoms and atomic ions.
  4. ^For the sources for these term symbols in the case of the heaviest elements, seeTemplate:Infobox element/symbol-to-electron-configuration/term-symbol.
  5. ^abXu, Renjun; Zhenwen, Dai (2006). "Alternative mathematical technique to determine LS spectral terms".Journal of Physics B: Atomic, Molecular and Optical Physics.39 (16):3221–3239.arXiv:physics/0510267.Bibcode:2006JPhB...39.3221X.doi:10.1088/0953-4075/39/16/007.S2CID 2422425.
  6. ^McDaniel, Darl H. (1977). "Spin factoring as an aid in the determination of spectroscopic terms".Journal of Chemical Education.54 (3): 147.Bibcode:1977JChEd..54..147M.doi:10.1021/ed054p147.
  7. ^"Atomic Spectroscopy - Different Coupling Scheme 9. Notations for Different Coupling Schemes".NIST. National Institute of Standards and Technology (NIST). 1 November 2017. Retrieved31 January 2019.
  8. ^"APPENDIX 1 - Coupling Schemes and Notation"(PDF). University of Toronto: Advanced Physics Laboratory - Course Homepage. Retrieved5 Nov 2017.
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