Martini purdue universityhigh level course outline
Short Course on Molecular Dynamics Simulation
Lecture 2:
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Move All Atoms
to New
Positions
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Interaction Models
Coulomb | EAM | Inter- atomic |
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Torsion |
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Reaction | Bond |
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Pair Potentials
Attractive
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– Lennard-Jones (n=12, m=6)
U LJr () | = | ⎛ 4 ε⎜⎜⎝ |
⎛⎜ |
σ⎞ ⎟ |
6 | ⎟
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FLJr () | = | − | dU r ( ) | = | 24 | 2⎛ ⎜ |
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ε
� Truncation
– The Lennard-Jones force (and similar models) decays rapidly with distance– Significant computation time can be saved by neglecting pair interactions beyond a cut-off
U | LJ | , | t | ( | r | ) | = | ⎛ 4 ε⎜⎜⎝ |
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6 | r | ≤ |
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0 | r | > |
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U |
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( | r | ) | = | ⎧U |
LJ | ( ) | − | U | LJ | r | ≤ | ||
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r | > |
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Pair Potentials
1. | ε = ij | σ = ij |
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2. | σ ij | = | σ i | + | |||||||||||||
3. | ε ij | = | 2 σ σ i 33 j |
σ ij | = | σ i 6 | + | ||||||||||
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σ i 6 |
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� Coulombic interactions
– Included if electrostatics between atoms are significant
– Atomic charges qi and qj
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Coulombic Interactions
� Coulombic force decays slower than r-3
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– Electrostatic potential due to i is exclusively due to the fraction of qi that is not screened by the cloud– This fraction rapidly decays to zero
– But we want to evaluate the contribution from point charges, not screened charges
– So we correct for the screening clouds by
introducing a smooth, compensating charge density
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( | r | ) | = | − | q i | ( α π ) | 3 2 | exp | (− | α r | |||||||||||||
U | Coulomb | = | 1 | ∑k≠0 | 4 π |
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(− | k | 2 |
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2 V | k |
Embedded Atom Model
Pair Potential | A. Martini | |
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Last Updated 8/2009 |
Embedded Atom Model
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