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Neutron Scattering

Neutron Scattering - JuSER - Forschungszentrum Jülich

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fluctuate in space and time . A phase transition bas occurred at a critical temperature, called<br />

Curie temperature Tc for ferromagnets or Néel temperature TN for antiferromagnets, from a<br />

long range ordered state at low temperatures to a paramagnetic high temperature phase . The<br />

two phases are characterised by an order parameter, such as the magnetisation for<br />

fenomagnets or the sublattice magnetisation for antiferromagnets . In the paramagnetic phase<br />

this order parameter vanishes, while in the low temperature phase it increases towards a<br />

saturation value, when the temperature is lowered . Depending on whether the order<br />

parameter changes discontinuously or continuously at the critical temperature, the phase<br />

transition is offrst- or second- order, respectively . At least for local moment systems, the<br />

magnetic interactions and moments are still present in the paramagnetic phase . Therefore<br />

above the critical temperature, magnetic correlations persist. This magnetic short range order<br />

fluctuates in time and extends over regions with characteristic linear dimensions, called the<br />

correlation length . When we decrease the temperature in the paramagnetic phase towards the<br />

transition temperature, the correlation length increases . Larger and larger regions develop<br />

which show short range order characteristic for the low temperature phase . The larger these<br />

conelated regions, the slower the fluctuation-dynamics . At the critical temperature of a<br />

second order phase transition, the correlation length and the magnetic susceptibility diverges,<br />

while the dynamics exhibits a critical slowing down.<br />

Besides the magnetic phase transitions, there exist also structural phase transitions . However,<br />

experiments on magnetic model systems provided the bases for our modern understanding of<br />

this complex co-operative effect. Th reason is that magnetic model systems can offen be<br />

described by some veiy simple Hamiltonian, such as the Heisenberg (16 .12), the x-y (16 .13)<br />

or the Ising model (16 .14), depending whether the System is isotropie, has a strong planar- or<br />

a strong uniaxial anisotropy, respectively :<br />

Heisenberg : H = Y J;j S ; - S i (16 .12)<br />

x-y : H=1J~ (Si,Sj,+Si,,S j,, ) (16 .13)<br />

>,;<br />

Ising : H = ~JüS,zs~~ (16 .14)<br />

ï<br />

16- 1 3

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