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Secular Equation - Advanced Quantum Chemistry and Spectroscopy - Lecture Slides, Slides of Chemistry

Secular Equation, Long Form, Unit Matrix, Non Trivial Solution, Determinant of the Coefficients, Eigenvalues, Diagonal and Partition the Column, Three Eigenvalue Problems, Smaller Dimension to Solve and few other describes importance of this lecture in Advanced Quantum Chemistry and Spectroscopy course.

Typology: Slides

2011/2012

Uploaded on 11/21/2012

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Download Secular Equation - Advanced Quantum Chemistry and Spectroscopy - Lecture Slides and more Slides Chemistry in PDF only on Docsity! ⎟⎟ ⎟ ⎟ ⎟ ⎠ ⎞ ⎜⎜ ⎜ ⎜ ⎜ ⎝ ⎛ = ⎟⎟ ⎟ ⎟ ⎟ ⎠ ⎞ ⎜⎜ ⎜ ⎜ ⎜ ⎝ ⎛ ⎟⎟ ⎟ ⎟ ⎟ ⎠ ⎞ ⎜⎜ ⎜ ⎜ ⎜ ⎝ ⎛ ∴ NNNNNNN N N c c c m c c c MMMM MMMM MMMM MM K MMMMM K K 2 1 2 1 321 2232221 1131211 (3) written in long form: ( ) ( ) ( ) ( ) 0: 0:3 0:2 0:1 332211 3333232131 2323222121 1313212111 =−++++= =++−++= =+++−+= =++++−= NNNNNN NN NN NN cmMcMcMcMNk cMcmMcMcMk cMcMcmMcMk cMcMcMcmMk L M L L L docsity.com This can be written as: ( ) 0~~~ =− cImM I is an N x N unit matrix where Iij = δij 0 1000 0010 0001 2 1 321 2232221 1131211 = ⎟⎟ ⎟ ⎟ ⎟ ⎠ ⎞ ⎜⎜ ⎜ ⎜ ⎜ ⎝ ⎛ ⎥ ⎥ ⎥ ⎥ ⎥ ⎦ ⎤ ⎢ ⎢ ⎢ ⎢ ⎢ ⎣ ⎡ ⎟⎟ ⎟ ⎟ ⎟ ⎠ ⎞ ⎜⎜ ⎜ ⎜ ⎜ ⎝ ⎛ − ⎟⎟ ⎟ ⎟ ⎟ ⎠ ⎞ ⎜⎜ ⎜ ⎜ ⎜ ⎝ ⎛ ⇒ NNNNNN N N c c c m MMMM MMMM MMMM M K MKMMM K K K MMMMM K K Note: if m is known, can solve (3) for c1 , c2 ,…,cN . Get a non-trivial solution only if the determinant of the coefficients of the unknown {ci } is zero (4) In matrix form: 0~~ =− ImM ( ) ( ) 0 321 2232221 1131211 = − − NNNNN N N MMMM MMmMM MMMmM K MMMMM K K This is called a SECULAR EQUATION for the eigenvalues m; that is, it yields the m’s. docsity.com Procedure Given: 0~~ =− ImM = secular equation that yields mi 1.) Take one solution for m, say m1 and substitute into the set of equations given by: ( ) )1(0~~~ =− cImM Solve for cn1 , n = 1,2,…,N Since the solutions to (1) can only be solved within a constant; that is, for cn1 /c11 , the expansion coefficients can be completely specified by requiring Ψ1 =Σn=1,..,N cni Ωn to be normalized; that is, <Φi |Φi > = 1 = Σn=1,..,N |cn1 |2. Repeat steps above for next mj , solving for the {cnj }, and requiring Φj to be normal. The procedure is repeated for j = 1,2,…,N. docsity.com 2.4: Time-independent degenerate perturbation theory A. Getting the solution in principle: Procedure is effectively similar to non- degenerate case but needs modification for 2 reasons. 1.) Ek(0) – Eq(0) can not be zero when we want to calculate ak in the spectral expansion 2.) If there are 2 or more states with the same energy we don’t know which state will arise in the expansion Recall: .... .... )2(2)1()0( )2(2)1()0( +++= +++= qqqq qqqq EEEE ψλλψψψ λλ docsity.com As λ → 0, Eq →Eq(0) and Ψq → Ψq(0) But which state if there more than one with the same Eq(0)? In general therefore )0( 0 lim j j jq c ψψλ ∑=→ The sum is over the degenerate states, where the degeneracy is labeled g. To solve this problem, we need two pieces of information: a) superposition principle b) orthonormalization procedure docsity.com Thus, for the example above: 2121 22111 )0( 2 )0( 1 2121 2 2 2 1 121 * 2212 * 1222 * 211 * 11 22112211 )0( 2 )0( 2 1 )0( 1 | |0|but |2 |||| |1|ii) i) ψψ ψψψφφ ψψ ψψψψψψψψ ψψψψφφ ψφ bb bb bbbb bbbbbbbb bbbb += +== ++= +++= ++== = This is 2 equations in 2 unknowns (b1 and b2 ) since <Ψi |Ψj > can be calculated 0|;0|;1| useSimilarly,iii) )0( 3 )0( 2 )0( 3 )0( 1 )0( 3 )0( 3 === φφφφφφ to generate 3 equations in 3 unknowns to solve for (c1 , c2 , c3 ). These will be our starting wave functions! For state q, we will call these states {Φq,j(0)} docsity.com Now we can 1.) generate a complete orthonormal set of wave functions by linear combinations of the form )0( , 1 )0( , jq g j jjq cψφ ∑ = = for all degenerate eigenvalues; that is, generate g Φ’s with g sets of coefficients. 2. Use this new set of wave functions in a perturbation problem. For the following be careful of the meaning of super- and subscripts Will use: j for the degenerate level, j = 1,2,…,g q for the level of interest k for all levels, k=1,2,…,00, degenerate or not. docsity.com
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