Lecture March18

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Molecular Modelling Lecture Notes

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  • Module-3

    Ab Initio Molecular Dynamics

    March 18

  • Molecular Dynamics (MD) Simulation

    Ab initio MD

    PLAN

  • R. Car and M. Parrinello Phys. Rev. Lett. 55, 2471, 1985

  • Molecular Dynamics

  • We like to move....atoms!How can I do it?

  • The Story of Newtons Apple...Equations of motion:

    Solving (integrating) D.E.

    F = md2x

    dt2

    We may use numerical or analytical integration

  • trusting truly on the

    classical equations of

    motion

    F=ma

    Mangalyaan Mission

  • also used to create your favorite characters!

  • gradient

    how to get forces?

    Fi = @U(x1, x2, , xn)@xi

    Born-Oppenheimer Molecular Dynamics

    U(RN ) = minD |Hel|

    E+ ENN

    {i}

    Ab Initio Molecular Dynamics

  • Demonstration: 1D-Harmonic Oscillator

    U(x) =1

    2kx2 ) md

    2x

    dt2= kx

    F = dUdx

    = kx Analytical solution obtainableReq. two initial conditions:

    x(0) x(0)&

  • Analytical integration of differential equation:

    ! =

    rk

    m

    x(t) = A cos(!t)

    v(t) = Aw sin(!t)

    x(0) = A v(0) = 0For the initial conditions:

  • time(t)

    x(t)

    ; v(t

    )

  • 2D-Harmonic OscillatorU(x, y) =

    1

    2kx2 +

    1

    2ky2

    U(x,y)

    x y

  • U(x,y)

    xy

    forces direct the system to the minimum PE

    Fx = @U@x

    = kx Fy = @U@y

    = ky

    F = Fxi+ Fyj

  • PE

    KE

  • How about atoms? Classical mechanics? or quantum mechanics? It is a good assumption to treat the atomic

    motions classically

    atom 2

    atom 3

    atom 1v1

    v2

    v3

    each degree of freedom of an atom will be having unique

    positions, velocities, and

    forces

    F = md2x

    dt2i ii i=1,3N

    N=number of particles

  • Each degree of freedom has an equation of motion (classical) as you have seen for a 2D-harmonic oscillator (before)

    For e.g. consider two atoms: 1 2

    x1

    y1

    z1

    x2

    y2

    z2

    Fx1 =M1d2x1dt2

    Fy1 =M1d2y1dt2

    Fz1 =M1d2z1dt2

    For atom 1 For atom 2

    Fx2 =M2d2x2dt2

    Fy2 =M2d2y2dt2

    Fz2 =M2d2z2dt2

    6 Eq. of motion to

    solve independently

  • The force acting on each degree of freedom of every atom has the information about the inter-atomic interactions

    Interatomic interactions are governed by the potential energy surface (as negative of the gradient of the potential energy is the force)

  • Lennard Jones Potential

    ULJ(R1, ,RN ) =XI

    XJ>I

    4

    "

    RIJ

    12

    RIJ

    6#

    FI = @ULJ(R1, ,RN )@RII = 1, , N

    RIJ = |RI RJ |

    LJ potential is an example of interatomic interaction

    Note: it is a 3D-vector(x,y,z components)

  • Numerical Integration

    VI(t) = VI(0) +

    Z t0dFI()

    MI

    RI(t) = RI(0) +

    Z t0

    dVI() atom 2 atom 3

    atom 1

    many body interactions within the

    force: numerical integration is required

    R

    tt

  • Velocity Verlet Algorithm

    RI(t +t) = RI(t) + RI(t)t +1

    2RI(t)t

    2 +O(t3)

    ULJ (R1(t), ,RN (t))

    RI(t +t) = RI(t) +t

    2

    hRI(t) + RI(t +t)

    i+O(t2)

    ULJ (R1(t+t), ,RN (t+t))

    derivat

    ive

    derivative

    deri

    vativ

    e

    Originally by Carl Stoermer (in 1907, particles in electric field)

  • tt

    tt

    RI RI

    velocity VerletnRI(0), RI(0)

    o nRI(t), RI(t)

    o nRI(2t), RI(2t)

    o

    Molecular Dynamics (MD)

    trajectory