Symplectic integrators for classical spin systems

Klas Modin

Joint work with

Robert McLachlan

Massey University

Olivier Verdier

Western Norway University

Outline

  • Symplectic integrators on \(\mathbb{R}^{2n}\)
  • Slightly dissipative systems
  • Spherical midpoint method

Illustration

  • Non-linear pendulum \(H(q,p) = p^2/2 -\cos(q)\)
\dot q = p, \quad \dot p = - \sin(q)
q
p

Illustration

  • Non-linear pendulum \(H(q,p) = p^2/2 -\cos(q)\)
\dot q = p, \quad \dot p = - \sin(q)

Illustration

  • Non-linear pendulum \(H(q,p) = p^2/2 -\cos(q)\)
\dot q = p, \quad \dot p = - \sin(q)

Why?

Hamiltonian dynamics on co-tangent bundles

Phase space \(T^*Q\)

Simplest case \(T^*\mathbb{R}^n\simeq \mathbb{R}^{2n}\)

\displaystyle\dot q^i = \frac{\partial H}{\partial p_i}(q^1,\ldots,q^n,p_1,\ldots,p_n)
\displaystyle\dot p_i = -\frac{\partial H}{\partial q^i}(q^1,\ldots,q^n,p_1,\ldots,p_n)

Typical examples: celestial mechanics, molecular dynamics

\mathbf{z}=(q,p) \;\Rightarrow\; \dot \mathbf{z} = X_H(\mathbf{z})

Symplectic property of the flow

Symplectic 2-form:

\Omega = dq^i\wedge dp_i

On \(\mathbb{R}^{2n}\):

\displaystyle\Omega_z(U,V) = U^\top \begin{pmatrix} 0 & -I_{n\times n} \\ I_{n\times n} & 0 \end{pmatrix} V

Hamiltonian vector fields fulfill (defining property)

\Omega_z(X_H,\cdot) = d H
\Omega_z(X_H,X_G) = \{H,G \}(z)

Flow \(\varphi_t\) preserves the symplectic form:

 

 

\Omega_{\varphi_t(z)}(D\varphi_t(z)\cdot U,D\varphi_t(z)\cdot V) = \Omega_z(U,V)

Geometric interpretation: the "symplectic area" of 2D surfaces in phase space are preserved

Consequences of symplecticness

This explains why symplectic integrators are superior!

  • "Almost" conservation of tori for Hamiltonian perturbations of integrable systems (KAM theory)
     
  • Convergence towards correct macroscopic equilibrium (e.g. temperature in MD)

Common symplectic integrators on \(\mathbb{R}^{2n}\)

  • Verlet scheme (many names: Leap-frog, Störmer-Verlet, symmetric splitting, Strang splitting, etc) for \(H(q,p) = T(p) + V(q)\)
\displaystyle q^{(k+1)} = q^{(k)} + h \nabla T(p^{(k+1/2)})
\displaystyle p^{(k+1/2)} = p^{(k)} - \frac{h}{2} \nabla V(q^{(k)})
\displaystyle p^{(k+1)} = p^{(k+1/2)} - \frac{h}{2} \nabla V(q^{(k+1)})
  • Midpoint method
\displaystyle z^{(k+1)} = z^{(k)} + h X_H\left(\frac{z^{(k+1)}+z^{(k)}}{2} \right)

Slightly dissipative systems

  • Elastic 3D pendulum
\displaystyle\dot q = \frac{p}{m}, \quad \dot p = -k\left(1-\frac{\ell}{|q|} \right)q + mg
\displaystyle -\;\varepsilon \frac{qq^\top p}{|q|^2}

Slightly dissipative systems

  • Elastic 3D pendulum
\displaystyle\dot q = \frac{p}{m}, \quad \dot p = -k\left(1-\frac{\ell}{|q|} \right)q + mg
\displaystyle -\;\varepsilon \frac{qq^\top p}{|q|^2}

non-symplectic

symplectic

Slightly dissipative systems

  • Elastic 3D pendulum
\displaystyle\dot q = \frac{p}{m}, \quad \dot p = -k\left(1-\frac{\ell}{|q|} \right)q + mg
\displaystyle -\;\varepsilon \frac{qq^\top p}{|q|^2}

Energy behaviour

Classical spin systems

\displaystyle \dot w_i = w_i\times \frac{\partial H}{\partial w_i}

Phase space \((S^2)^n\)

 Symplectic structure on \(S^2\) \[\Omega_w(u,v)=\mathrm{det}(w,u,v)\]

+\cdots +

Motivation for spin systems

  • Abundance in physics
    (e.g. atomistic spin dynamics)
     

  • Simplest Kähler manifold
     

  • Simplest coadjoint orbit
     

  • Simplest inexact symplectic form

Some example spin systems

Free rigid body \[\dot w = w\times I^{-1}w \]

Heisenberg spin chain
(discrete Landau-Lifshitz) \[\dot w_i = w_i\times (w_{i-1}+w_{i+1}) \]

Fluid particle tracking on sphere \[\dot w = \xi(t,w), \quad \xi(t,\cdot)\in \mathfrak{X}_\mu(S^2) \]

Point vortex dynamics on spheres
(Jupiter's great red spot)

Known symplectic integrators

  • Splitting methods
     
  • \(S^2\) coadjoint orbit of reduced system on \(T^*SU(2) \)
    RATTLE \(\Rightarrow\) 9 variables
    Variational Lie \(\Rightarrow\) 8 variables
     
  • Collective symplectic integrator
    \(\Rightarrow\) 4 variables
T^*SU(2)
\mathfrak{su}(2)^*

Drawbacks: many auxiliary variables, complicated, large error constants

Minimum variables (=3)

and symplectic?

  • Classical midpoint method on \(\mathbb{R}^3\)
     
  • Riemannian midpoint method on \(S^2\)

\(\Rightarrow\) not symplectic

\(\Rightarrow\) not symplectic

Candidates:

Spherical midpoint method

\displaystyle\frac{W_i - w_i}{h} = \frac{W_i+w_i}{|W_i+w_i|}\times \frac{\partial H}{\partial w_i}\left(\frac{W_1+w_1}{|W_1+w_1|},\ldots,\frac{W_n+w_n}{|W_n+w_n|} \right)

Main result

  1. Second order
  2. Equivariant w.r.t. \(SO(3)^n\)
  3. Symplectic
  4. Preserves single-spin quadratic invariants
  5. Self-adjoint
S^3 \simeq

Hopf fibration

S^2
\pi

Extended Hopf fibration

\mathbb{R}^3_*
\pi
T^*\mathbb{R}^2_*
\pi

Classical
midpoint

Riemannian
midpoint

Simple interpretation

\displaystyle\frac{W - w}{h} = \frac{W+w}{|W+w|}\times \frac{\partial H}{\partial w}\left(\frac{W+w}{|W+w|} \right)
\displaystyle X_H(w) = w\times \frac{\partial H}{\partial w}(w)
\displaystyle \Rightarrow W-w = h X_H\left(\frac{W+w}{|W+w|}\right)
\displaystyle \bar X_H(w) = X_H\left(\frac{w}{|w|} \right)
\displaystyle \Rightarrow W-w = h \bar X_H\left(\frac{W+w}{2}\right)

Classical midpoint method applied to \(\bar X_H\)

Example 1: free rigid body

\dot w = w \times I^{-1}w

Example 2: irreversible rigid body

H(w)= \frac{1}{2} w\cdot I(w)^{-1}w

Example 3: development of chaos

H(w)= \frac{1}{2} w\cdot I^{-1}w + \varepsilon \sin(t)w^1

Example 4: Landau-Lifshitz PDE

\dot w = w\times w'', \qquad w\colon \mathbf{R}\times S^1 \to S^2

Example 5: atomistic spin dynamics ???

THANKS!

References:

Symplectic integrators for spin systems, Phys. Rev. E, 89:061301, 2014

arXiv:1402.4114

 

A minimal-variable symplectic integrator on spheres, Math. Comp., 86, 2325-2344, 2016

arXiv:1402.3334

 

Geometry of discrete-time spin systems, J. Nonlin. Sci., 26(5):1507-1523, 2016

arXiv:1505.04035

*slides at slides.com/kmodin

Symplectic integrators for classical spin systems

By Klas Modin

Symplectic integrators for classical spin systems

Presentation given 2017-12 to physicists in Uppsala.

  • 1,681