Misplaced Pages

Classical Heisenberg model

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
(Redirected from Heisenberg model (classical))

In statistical physics, the classical Heisenberg model, developed by Werner Heisenberg, is the n = 3 {\displaystyle n=3} case of the n-vector model, one of the models used to model ferromagnetism and other phenomena.

Definition

The classical Heisenberg model can be formulated as follows: take a d-dimensional lattice, and place a set of spins of unit length,

s → i ∈ R 3 , | s → i | = 1 ( 1 ) {\displaystyle {\vec {s}}_{i}\in \mathbb {R} ^{3},|{\vec {s}}_{i}|=1\quad (1)} ,

on each lattice node.

The model is defined through the following Hamiltonian:

H = − ∑ i , j J i j s → i ⋅ s → j ( 2 ) {\displaystyle {\mathcal {H}}=-\sum _{i,j}{\mathcal {J}}_{ij}{\vec {s}}_{i}\cdot {\vec {s}}_{j}\quad (2)}

where

J i j = { J if  i , j  are neighbors 0 else. {\displaystyle {\mathcal {J}}_{ij}={\begin{cases}J&{\mbox{if }}i,j{\mbox{ are neighbors}}\\0&{\mbox{else.}}\end{cases}}}

is a coupling between spins.

Properties

  • The general mathematical formalism used to describe and solve the Heisenberg model and certain generalizations is developed in the article on the Potts model.
  • In the continuum limit the Heisenberg model (2) gives the following equation of motion
S → t = S → ∧ S → x x . {\displaystyle {\vec {S}}_{t}={\vec {S}}\wedge {\vec {S}}_{xx}.}
This equation is called the continuous classical Heisenberg ferromagnet equation or, more shortly, the Heisenberg model and is integrable in the sense of soliton theory. It admits several integrable and nonintegrable generalizations like the Landau-Lifshitz equation, the Ishimori equation, and so on.

One dimension

  • In the case of a long-range interaction, J x , y ∼ | x − y | − α {\displaystyle J_{x,y}\sim |x-y|^{-\alpha }} , the thermodynamic limit is well defined if α > 1 {\displaystyle \alpha >1} ; the magnetization remains zero if α ≥ 2 {\displaystyle \alpha \geq 2} ; but the magnetization is positive, at a low enough temperature, if 1 < α < 2 {\displaystyle 1<\alpha <2} (infrared bounds).
  • As in any 'nearest-neighbor' n-vector model with free boundary conditions, if the external field is zero, there exists a simple exact solution.

Two dimensions

  • In the case of a long-range interaction, J x , y ∼ | x − y | − α {\displaystyle J_{x,y}\sim |x-y|^{-\alpha }} , the thermodynamic limit is well defined if α > 2 {\displaystyle \alpha >2} ; the magnetization remains zero if α ≥ 4 {\displaystyle \alpha \geq 4} ; but the magnetization is positive at a low enough temperature if 2 < α < 4 {\displaystyle 2<\alpha <4} (infrared bounds).
  • Polyakov has conjectured that, as opposed to the classical XY model, there is no dipole phase for any T > 0 {\displaystyle T>0} ; namely, at non-zero temperatures the correlations cluster exponentially fast.

Three and higher dimensions

Independently of the range of the interaction, at a low enough temperature the magnetization is positive.

Conjecturally, in each of the low temperature extremal states the truncated correlations decay algebraically.

See also

References

  1. Polyakov, A.M. (1975). "Interaction of goldstone particles in two dimensions. Applications to ferromagnets and massive Yang-Mills fields". Phys. Lett. B 59 (1): 79–81. Bibcode:1975PhLB...59...79P. doi:10.1016/0370-2693(75)90161-6.

External links

Categories: