Lecture 2: Few dimensional systems, Discrete variable representation, SOFT Flashcards

• Develop insight into a range of methods for solving the Schrodinger equation in few-dimensions, including discrete variable representation and split-operator Fourier transform. o Investigate two methods for solving the TDSE for few-dimensional systems on single PESs o Investigate how the DVR method can be used to determine eigenstates allowing direct wavefunction propagation

1
Q
  • Reminder from Lec 1
    • After making the …-… approximation, the time-dependent Schrodinger equation has the form below
    • This tells us how the wavefunction changes with time on a single
    • We want to use the TDSE to wavefunctions
A
  • Reminder from Lec 1
    • After making the Born-Oppenheimer approximation, the time-dependent Schrodinger equation has the form below
    • This equation of motion tells us how the nuclear wavefunction changes with time on a single electronic state
    • We want to use the TDSE to propagate wavefunctions
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2
Q
  • Reminder from Lec 1 part 2
    • Also saw last time that if we know the of the , wavefunction propagation is simplified
    • If the wavefuntion is one of the of the system, simply picks up an which changes with time
A
  • Reminder from Lec 1 part 2
    • Also saw last time that if we know the eigenstates of the PES, wavefunction propagation is simplified
    • If the wavefuntion is one of the eigenstates of the system, simply picks up an oscillating phase factor which changes with time
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3
Q

What if the wavefunction being propagated is not an eigenstate, but instead a combination of states is being populated?

A
  • Eigenstates of a Hamiltonian form a complete set
  • Any function can be written as a linear combination of eigenstates of this Hamiltonian
  • Time dependence now carried by expansion coefficients which contribute differently to each state
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4
Q
  • What are the two steps for propagating known eigenstates
A
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5
Q
  • How can eigenstates included in the nuclear SEQ be represented?
A
  • Want to find states that obey nuclear SEQ
  • Can expand each eigenstate in a fixed basis set of introduced functions ϕ
  • a indicates how much each basis function k contribute to eigenstate i
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6
Q

Our basis set is orthonormal, what does this mean?

A
  • Delta function is 0 if states i/j are not the same
  • Delta function is 1 if states i/j are the same
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7
Q
  • How is the set of equations of linear combinations of each eigenstate (linear combination of basis-functions) collected?
A
  • Set of equations collected together in a matrix, which is easy to compute
  • Where input is Hamiltonian matrix expressed in basis functions ϕ
  • Output is a diagonal matrix of eigenvalues (energies) and coefficients associated with them, a
  • MxM coefficient matrix, a indicates, for each eigenstate, how much each basis set contributes.
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8
Q
  • What is a good choice for basis-functions, ϕ?
A
  • Represent each basis function as a collection of complex waves (this is one example)
  • Each appear as delta functions centred at each grid-point
  • Increase in j moves line to left of graph (v.v)
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9
Q

Describe the differences and similarities between these two eigenstate representations

A
  • Sum of linear combination of functions of different contributions form different eigenstates
  • Same basis set in each but different set of contributions
  • Delta function on a uniform grid, height of which gives a (contribution) of basis function to eigenfunction
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10
Q
  • What contributes to the Hamiltonian matrix elements for our chosen basis functions?
A
  • Hij = Tij + Vij
  • T term depends on if i/j are the same or not, and can be calculated easily as know contributing components e.g. mass
  • Vij depends on delta function, works out as diagonal matrix where value at each grid point is just the V at that particular grid point
  • Now Hamiltonian matrix solved in Ha = Ea, (step 1) must find coefficients of M eigenstates.
    • –> step 2
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11
Q
  • What is an example of a process that can be used to find values of eigenstates?
A
  • Colbert-miller DVR used to find eigenstate numbers in matrix a
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12
Q
  • After eigenstates found one must move the calculated (time dependent) associated with in time
A

After eigenstates found one must move the calculated coefficients (time dependent) associated with wavefunction in time

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13
Q
  • What is the first step in calculating coefficients as they evolve in time?
A
  • Work out initial coefficients
  • Form a linear combination of eigenstates and coefficients i at t =0
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14
Q
  • What is the result of subbing in our linear combination of coefficients into the TDSEQ?
A
  • Once initial coefficients known, propagation becomes simple
  • Only thing changing with time is coefficients
  • Can now calculate any coefficient at any time t
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15
Q
  • What should be the result of calculated expansion coefficients for each eigenfunction relative to the initial wavefunction
A
  • Should get near exact agreement with initial wavefunction
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16
Q
  • Once TDSEQ solved can use at a certain time to calculate an expectation value e.g. (…/…)
A
  • Once TDSEQ solved can use wavefunction at a certain time to calculate an expectation value e.g. (momentum/position)
17
Q
  • Why can DVR not be used for more degrees of freedom?
A
  • For f degrees-of-freedom Nf grid-points are required
  • This quickly becomes computationally demanding
  • Large memory requirement for calculation of PE at each grid point
  • Restricted to 5 DOFs