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1 © copyright 2011 William A. Goddard III, all rights reserved Ch120a-Goddard-L03 Ch121a Atomic Level Simulations of Materials and Molecules William A. Goddard III, [email protected] Charles and Mary Ferkel Professor of Chemistry, Materials Science, and Applied Physics, California Institute of Technology BI 115 Hours: 2:30-3:30 Monday and Wednesday Lecture or Lab: Friday 2-3pm (+3-4pm) Teaching Assistants Wei-Guang Liu, Fan Lu, Jose Mendozq, Andrea Kirkpatrick Lecture 3, April 6, 2011 Force Fields – 1 valence, QEq, vdw
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Page 1: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

1© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Ch121a Atomic Level Simulations of Materials and Molecules

William A. Goddard III, [email protected] and Mary Ferkel Professor of Chemistry,

Materials Science, and Applied Physics, California Institute of Technology

BI 115Hours: 2:30-3:30 Monday and Wednesday

Lecture or Lab: Friday 2-3pm (+3-4pm)

Teaching Assistants Wei-Guang Liu, Fan Lu, Jose Mendozq, Andrea Kirkpatrick

Lecture 3, April 6, 2011Force Fields – 1 valence, QEq, vdw

Page 2: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

2© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

kj kj

k

ijijikl

lk

klki ik k r

eZ

r

e

R

eZZ

mMH

2222

22

2

22

Born-Oppenheimer approximation, fix nuclei (Rk=1..M), solve for Ψel(1..N)

The full Quantum Mechanics Hamiltonian: Htotal(1..Nel,1..Mnuc)

nuclei electrons nucleus-nucleus

electron-nucleus

electron-electron

Hel(1..Nel) =

NM M M,NN

Hel(1..Nel) Ψel(1..Nel) = Eel Ψel(1..Nel)

Ψel(1..Nel) and Eel(1..Mnuc) are functions of the nuclear coordinates.

Next solve the nuclear QM problem

+Eel(1..Mnuc)Hnuc(1..Mnuc) =

Hnuc(1..Mnuc) Ψnuc(1..Mnuc) = Enuc Ψnuc(1..Mnuc)

EPE(1..Mnuc)FF is analytic fit to this

Page 3: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

3© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Force Field

Involves covalent bonds and the coupling between them (2-body, 3-body, 4-body, cross terms)

= Eel(1..Mnuc)EPE(1..Mnuc)

The Force Field (FF) is an analytic fit to such expressions but formulated to be transferable so can use the same terms for various molecules and solids

General form:

Ecross-terms

E nonbond = Evdw + Eelectrostatic

Involves action at a distance, long range interactions

Page 4: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

4© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Re = 0.9 – 2.2 ÅKe = 700 (Kcal/mol)/Å 2

Units: multiply by 143.88 to convert mdynes/ Å to (Kcal/mol)/Å 2

Simple Harmonic

Bond Stretch Terms: Harmonic oscillator form

R

ignore

Taylor series expansion about the equilibrium, Re, = R-Re

E()=E(Re)+(dE/dR)e[]+½(d2E/dR2)e[]2+(1/6)(d3E/dR3)e[]3 + O(ignore zero ignore

Kb

Some force fields, CHARRM, Amber use k=2Ke to avoid multiplying by 2

Re

Problem: cannot break the bond, E ∞

Ground state wavefunction (Gaussian)mЋ) exp[- (m2Ћ)2]

eigenstates, E = + ½ , where =0,1,2,…

E(R) = (ke/2)(R-Re)2,

Page 5: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

5© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Note that E(Re) = 0, the usual convention for bond termsDe is the bond energy in kcal/molRe is the equilibrium bond distance is the Morse scaling parametercalculate from Ke and De

Bond Stretch Terms: Morse oscillator form

-0.03

-0.02

-0.01

0

0.01

0.02

0.03

0.04

2 3 4 5 6

D0

R0

RWant the E to go to a constant as break bond, popular form is Morse function

E = 0

where X = exp[-(R-Re)] = exp[-(/2)(R/Re -1)]

Evdw (Rij) = De[X2-2X]

= sqrt(ke/2De), where ke = d2E/dR2 at R=Re (the force constant)

Page 6: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

6© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Morse Potential – get analytic solution for quantum vibrational levels

where X = exp[-(R-Re)] = exp[-(/2)(R/Re -1)]

Evdw (Rij) = De[X2-2X]

= sqrt(ke/2De), where ke = d2E/dR2 at R=Re (the force constant)

Ev = hv0( + 1/2 ) – [hv0( + ½)]2/4De

0 = (/2)sqrt(2De/m)

Level separations decrease linearly with level

E+1 – E = hv0 – (+1)(hv0)2/2De

Write

En/hc = e( + ½ ) - xee( + ½ )2

Page 7: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

7© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

The Bending potential surface for CH2

3B1

1A1

1B1

3g-

1g

9.3 kcal/mol

Page 8: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

8© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Angle Bend Terms: cosine harmonic

I K

J

E() = C0 + C1 cos() + C2 cos(2) + C3 cos(3) + ….

~ ½ Ch [cos - cos e]2 = 0 at = e

E”() = dE()/d = - Ch [cos - cos e] sin = 0 at = e

E”() = d2E()/d2 = - Ch [cos - cos e] cos + Ch (sin )2

= Ch (sin e)2 at = e

Thus k = Ch (sin e)2

Page 9: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

9© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

The energy barrier to “linearize” the molecule becomes

Ebarrier 1/2C 1 cos(o) 2 1/2K (1 cos(o)

sin(o))2

E( ) E( )By symmetry the angular energy satisfy

E( ) E()This is always satisfied for the cosine expansion but

Barriers for angle term

A second more popular form is the Harmonic theta expansionE() = ½ K + [ - e]2 However except for linear molecules this does NOT satisfy the symmetry relations, leading to undefined energies and forces for = 180° and 0°. This is used by CHARMM, Amber, ..

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10© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Angle Bend Terms for linear molecule,

I

K

J

If e = 180° then we write E() = K [1 + cos()]

since for = 180 – this becomes

E() = K [1 + (-1 + ½ K

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11© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

For an Octahedral complex The angle function should have the form E() = C [1 - cos4] which has minima for = 0, 90, 180, and 270°With a barrier of C for = 45, 135, 225, and 315°Here the force constant is K = 16C= CP2 where P=4 is the periodicity, so we can write C=K/P2

Simple Periodic Angle Bend Terms

Page 12: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

12© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

For an Octahedral complex The angle function should have the form E() = C [1 - cos4] which has minima for = 0, 90, 180, and 270°With a barrier of C for = 45, 135, 225, and 315°Here the force constant is K = 16C= CP2 where P=4 is the periodicity, so we can write C=K/P2

However if we wanted the minima to be at = 45, 135, 225, and 315° with maxima at = 0, 90, 180, and 270°then we want to use E() = ½ C [1 + cos4] Thus the general form is E() = (K/P2)[1 – (-1)Bcos4]Where B=1 for the case with a minimum at 0° and B=-1 for a maximum at 0°

Simple Periodic Angle Bend Terms

Page 13: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

13© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Rotational barriers

HOOH

1.19 kcal/mol Trans barrier

7.6 kcal/mol Cis barrier

HSSH:

5.02 kcal/mol trans barrier

7.54 kcal/mol cis barrier

Part of these barriers can be explained as due to vdw and electrostatic interactions between the H’s.

But part of it arises from covalent terms (the p lone pairs on each S or O

This part has the form E(φ) = ½ B [1+cos(2φ)]

Which is

E=0 for φ=90,270° and E=B for φ=0,180°

Page 14: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

14© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

dihedral or torsion terms

Where each kn is in kcal/mol, n = 1, is the periodicity of the potential and

d=+1 the cis conformation is a minimumd=-1 the cis conformation is thea maximumInput data is K and d for each n.

E() 1/2[kn (1 d cos(n)]n1

p

IJ K

LE(φ) = C0 + C1 cos(φ) + C2 cos(2 φ) + C3 cos(3 φ) + ….which we write as

I K

Jφ LGiven any two bonds IJ and KL attached

to a common bond JK, the dihedral angle φ is the angle of the JKL plane from the IJK plane, with cis being 0

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15© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Consider the central CC bond in Butane

There are nine possible dihedrals: 4 HCCH, 2 HCCC, 2 CCCH, and 1 CCCC.Each of these 9 could be written asE(φ) = ½ B [1 – cos(3 φ)], For which E=0 for φ = 60, 180 and 300°and E=B the rotation barrier for φ = 0, 120 and 240°.

IJ K

L

Page 16: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

16© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Consider the central CC bond in Butane

IJ K

L

For ethane get 9 HCCH terms.The total barrier in ethane is 3kcal/mol but standard vdw and charges of +0.15 on each H will account for ~1 kcal/mol.Thus only need explicit dihedral barrier of 2 kcal/mol.

There are nine possible dihedrals: 4 HCCH, 2 HCCC, 2 CCCH, and 1 CCCC.Each of these 9 could be written asE(φ) = ½ B [1 – cos(3 φ)], For which E=0 for φ = 60, 180 and 300°and E=B the rotation barrier for φ = 0, 120 and 240°.

Page 17: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

17© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Consider the central CC bond in Butane

IJ K

L

Can do two ways. Incremental: treat each HCCH as having a barrier of 2/9 and add the terms from each of the 9 to get a total of 2 (Amber, CHARRM)Or use a barrier of 2 kcal/mol for each of the 9, but normalize by the total number of 9 to get a net of 2 (Dreiding)

There are nine possible dihedrals: 4 HCCH, 2 HCCC, 2 CCCH, and 1 CCCC.Each of these 9 could be written asE(φ) = ½ B [1 – cos(3 φ)], For which E=0 for φ = 60, 180 and 300°and E=B the rotation barrier for φ = 0, 120 and 240°.For ethane get 9 HCCH terms.The total barrier in ethane is 3kcal/mol but standard vdw and charges of +0.15 on each H will account for ~1 kcal/mol.Thus only need explicit dihedral barrier of 2 kcal/mol.

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18© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Twisting potential surface for etheneThe ground state (N) of ethene prefers φ=0º to obtain the highest overlap with a rotational barrier of 65 kcal/mol for prefers φ =90º to obtain the lowest overlap.

We write this as E(φ) = ½ B [1-cos2 φ)]. Since there are 4 HCCH terms, we calculate each using the full B=65, but divide by 4.

φ = 0° φ = 90°φ = -90°

T

N

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19© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Inversions

When an atom I has exactly 3 distinct bonds IJ, IK, and IL, it is often necessary to include an exlicit term in the force field to adjust the energy for “planarizing” the center atom I.

E() 1/2C(cos() cos(o))2

I

K

LJ

K C sin2o

Where the force constant in kcal/mol is

LJ

I

K

Umbrella inversion:ω is the angle betweenThe IL axis and the JIK plane

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20© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Amber describes inversion using an improper torsion.

E() 1/2K cos[n( o)]

N=2 for planar angles (=180°) and n=3 for the tetrahedralAngles ( =120°).

Improper Torsion: is the angle between the JIL plane and the KIL planeL

J

I

K

AMBER Improper Torsion JILK

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21© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

CHARMM Improper Torsion IJKL

In the CHARMM force field, inversion is defined as if it were a torsion.

E() 1/2K [ o]2

Improper Torsion: φ is the angle between the IJK plane and the LJK plane

L

J

IK

For a tetrahedral carbon atom with equal bonds this angles is φ=35.264°.

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22© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Bond Stretch

Angle bend

Torsion

Inversion

Typical ExpressionsDescription Illustration

2

00)]cos())][cos(sin(2/[ kEHarmonic-cosine

Dreiding dihedral

2

00)]cos())][cos(sin(/2/1[ kE

Umbrella inversion

2

2)( o

b RRK

RE Harmonic Stretch

E() 1/2[kn (1 dcos(n)]n1

p

Summary: Valence Force Field Terms

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23© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Coulomb (Electrostatic) Interactions

Most force fields use fixed partial charges on each nucleus, leading to electrostatic or Coulomb interactions between each pair of charged particles. The electrostatic energy between point charges Qi and Qk is described by Coulomb's Law as

EQ(Rik) = C0 Qi Qk /(Rik)

where Qi and Qk are atomic partial charges in electron units

C0 converts units: if E is in eV and R in A, then C0 = 14.403If E is in kcal/mol and R in A, then C0 = 332.0637= 1 in a vacuum (dielectric constant)

TA check numbers

Page 24: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

24© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

How estimate charges?

Even for a material as ionic as NaCl diatomic, the dipole moment a net charge of +0.8 e on the Na and -0.8 e on the Cl.

We need a method to estimate such charges in order to calculate properties of materials.

First a bit more about units.

In QM calculations the unit of charge is the magnitude of the charge on an electron and the unit of length is the bohr (a0)

Thus QM calculations of dipole moment are in units of ea0 which we refer to as au. However the international standard for quoting dipole moment is the Debye = 10-10 esu A

Where (D) = 2.5418 (au)

Page 25: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

25GODDARD - MSC/CaltechGODDARD - MSC/Caltech Berlin 3/22/04Berlin 3/22/04

ReaxFF Electrostatics energy – Critical element

Three universal parameters for each element:1991: used experimental IP, EA, Ri;

ReaxFF get all parameters from fitting QM

ci

si

ci

oi

oi qRRJ &,,,

Keeping: i

i Qq

•Self-consistent Charge Equilibration (QEq)•Describe charges as distributed (Gaussian)•Thus charges on adjacent atoms shielded (interactions constant as R0) and include interactions over ALL atoms, even if bonded (no exclusions)•Allow charge transfer (QEq method)

ji iiiiiijjiiji qJqrqqJqE

2

1),,(}{

Electronegativity (IP+EA)/2

Hardness (IP-EA)

interactions atomic

lk

kir

rErflj

kiij QQQQrE

ij

ijklij

klij

,,int

Jij

rij

1/rij

ri0

+ rj0

I

2

Page 26: © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03 1 Ch121a Atomic Level Simulations of Materials and Molecules William A.

26© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Charge Equilibration

Charge Equilibration for Molecular Dynamics Simulations;

A. K. Rappé and W. A. Goddard III; J. Phys. Chem. 95, 3358 (1991)

First consider how the energy of an atom depends on the net charge on the atom, E(Q)

Including terms through 2nd order leads to

(2) (3)

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27© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Charge dependence of the energy (eV) of an atom

E=0

E=-3.615

E=12.967

Cl Cl-Cl+

Q=0 Q=-1Q=+1

Harmonic fit

= 8.291 = 9.352

Get minimum at Q=-0.887Emin = -3.676

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28© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

QEq parameters

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29© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Interpretation of J, the hardness

Define an atomic radius as

H 0.84 0.74C 1.42 1.23N 1.22 1.10O 1.08 1.21Si 2.20 2.35S 1.60 1.63Li 3.01 3.08

RA0 Re(A2) Bond distance of

homonuclear diatomic

Thus J is related to the coulomb energy of a charge the size of the atom

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30© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

The total energy of a molecular complex

Consider now a distribution of charges over the atoms of a complex: QA, QB, etc

Letting JAB(R) = the Coulomb potential of unit charges on the atoms, we can write

or

Taking the derivative with respect to charge leads to the chemical potential, which is a function of the charges

The definition of equilibrium is for all chemical potentials to be equal. This leads to

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31© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

The QEq equations Adding to the N-1 conditions

The condition that the total charged is fixed (say at 0) leads to the condition

Leads to a set of N linear equations for the N variables QA.

AQ=X, where the NxN matrix A and the N dimensional vector A are known. This is solved for the N unknowns, Q.

We place some conditions on this. The harmonic fit of charge to the energy of an atom is assumed to be valid only for filling the valence shell.

Thus we restrict Q(Cl) to lie between +7 and -1 and

Q(C) to be between +4 and -4

Similarly Q(H) is between +1 and -1

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32© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

The QEq Coulomb potential lawWe need now to choose a form for JAB(R) A plausible form is JAB(R) = 14.4/R, which is valid when the charge distributions for atom A and B do not overlapClearly this form as the problem that JAB(R) ∞ as R 0In fact the overlap of the orbitals leads to shielding The plot shows the shielding for C atoms using various Slater orbitals

And = 0.5 Using RC=0.759a0

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33© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

QEq results for alkali halides

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34© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

QEq for Ala-His-Ala

Amber charges in

parentheses

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35© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

QEq for deoxy adenosine

Amber charges in

parentheses

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36© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

QEq for polymers

Nylon 66

PEEK

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37GODDARD - MSC/CaltechGODDARD - MSC/Caltech Berlin 3/22/04Berlin 3/22/04

Four universal parameters for each element:Get from QM

Polarizable QEq

)||exp()()(

)||exp()()(

2

2

23

23

si

si

si

si

ci

ci

ci

ci

rrQr

rrQrsi

ci

Allow each atom to have two charges:A fixed core charge (+4 for Si) with a Gaussian shapeA variable shell charge with a Gaussian shape but subject to displacement and charge transferElectrostatic interactions between all charges, including the core and shell on same atomAllow Shell to move with respect to core, to describe atomic polarizabilitySelf-consistent charge equilibration (QEq)

ci

si

ci

oi

oi qRRJ &,,,

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38© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Noble gas dimers

Ar2

Re

De

Most popular form: LJ 12-6E=A/R12 –B/R6

= De[12 – 26] where = R/ReDe[12 – 6] where R/Here = Re(1/2)1/6 =0.89 Re

All nonbonded atoms and molecules exhibit a very repulsive interaction at short distances due to overlap of electron pairs (Pauli Repulsion) and a weak attractive interaction scaling like 1/R6 at long R (London Dispersion. Together these are called van der Waals (vdW) interactions

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39© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

van der Waals interaction

6, 8, 10,

6 8 10( ...)ij ij ij

dispi j ij ij ij

C C CE

R R R

What vdW interactions account for?

Short range repulsion Overlap of orbitals and the Pauli Principle

Dipole-dipole Dipole-quadrupole Quadruole-quadrupole

We often neglect higher order (>R6) terms.

(where 0)

1or (where 9)

ijCR

repi j

rep Ni j ij

E e C

E NR

Long range attraction Instantaneous multipolar interaction (London dispersion)

Pauli repulsion:

Born repulsion:

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40© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Popular vdW Nonbond Terms: LJ12-6NonBond

RLennard-Jones 12-6

E(R)=A/R12 – B/R6

=Dvdw{1/12 – 2/6} where = R/Rvdw

= 4Dvdw{[vdw/R)12]- [vdw/R)6]}

Dvdw=well depth,

Rvdw = Equilibrium distance for vdw dimer

= point at which E=0 (inner wall, ~ 0.89 Rvdw)

Dimensionless force constant = {[d2E/d2]=1}/Dvdw = 72

The choice of 1/R6 is due to London Dispersion (vdw Attraction)

However there is no special reason for the 1/R12 short range form (other that it saved computation time for 1950’s computers)

LJ 9-6 would lead to a more accurate inner wall.

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41© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Popular vdW Nonbond Terms- Exponential-6

Buckingham or exponential-6E(R)= A e-CR - B/R6 which we write as

NonBond

R

whereR0 = Equilibrium bond distance; = R/R0 is the scaled distanceDo=well depth = dimensionless parameter related to force constant at R0

We define a dimensionless force constant as = {(d2E/d2)=1}/D0 = 72 for LJ12-6= 12 leads to –D0/6 at long R, just as for LJ12-6= 13.772 leads to = 72 just as for LJ12-6A problem with exp-6 is that E- ∞ as R 0. To avoid this BioGraf, LinGraf, CeriusII calculate the inner maximum and reflect E about this point for smaller R so that E and E’ are continuous. When >10 this point is well up the inner wall and not important

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42© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Converting between X-6 and LJ12-6

Usual convention: use the same R0 and D0 and set = 12.

I recall that this leads to small systematic errors.

Second choice: require that the long range form of exp-6 be the same as for LJ12-6 (ie -2D0/6) and require that the inner crossing point be the same. This leads to

This was published in the Dreiding paper but I do not know if it has ever been used

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43© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

Popular vdW Nonbond Terms: MorseNonBond

RE(R) = D0 {exp[-R-R0)] - 2 exp[(-(R-R0)]}At R=R0, E(R0) = -D0

At R=∞, E(R0) = 0D0 is the bond energy in Kcal/molR0 is the equilibrium bond distance is the Morse scaling parameter

-0.03

-0.02

-0.01

0

0.01

0.02

0.03

0.04

2 3 4 5 6

D0R0

I prefer to write this asE(R) = D0 [X2 - 2X] where X = exp[(/2)(1-)]At R=R0, = 1 X = 1 E(R0) = -D0

At R=∞, X = 0 E(R0) = 0 = {(d2E/d2)=1}/D0 = 2/2Thus = 12 = 72 just as for LJ12-6Few theorists believe that Morse makes sense for vdw parameters since it does not behave as 1/R6 as R∞ However, the vdw curve matches 1/R6 only for R>6A, and for our systems there will be other atoms in between. So Morse is ok.

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44© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

vdW combination rules

Generally the vdw parameters are provided for HH, CC, NN etc (diagonal cases) and the off-diagonal terms are obtain using combination rules

D0IJ = Sqrt(D0II D0JJ)

R0IJ = Sqrt(R0II R0JJ)

IJ = (IJ + IJ)/2

Sometimes an arithmetic combination rule is used for vdw radii

R0IJ = (R0II + R0JJ)/2 but this complicates vdw calculations

(the amber paper claims to do this but the code uses geometric combinations of the radii)

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45© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

1-2 and 1-3 Nonbond exclusions

For valence force fields, it is assumed that the bond and angle quantities include already the Pauli Repulsion and electrostatic contributions included in the nonbond interactions.

Thus normally we exclude from the vdw and coulomb sums the contributions from bonds (1-2) and next nearest neighbor (1-3) interactions

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46© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L03

1-4 Nonbond exclusions

There is disagreement about 1-4 interactions. In fact the original of the rotational barrier in ethane is probably all due to Pauli repulsion orthogonality effects.

Thus a proper description of the vdW interactions between 1-4 atoms should account for the barrier.

In fact it accounts only for 1/3 of the barrier.

I believe that this is because the CH bond pairs are centered at the bond midpoint not on the H atoms.

Thus using atom centered vdw accounts for only part of the barrier necessitating an explicit dihedral term.

Thus I believe that the1-4 vdw and electrostatic terms should be included. However some FF, such as Amber, CHARRM reduce the 1-4 interactions by a factor of 2. I do not know of a justification for this.


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