In condensed matter physics, magnetic anisotropy describes how an object's magnetic properties can be different depending on direction. In the simplest case, there is no preferential direction for an object's magnetic moment. It will respond to an applied magnetic field in the same way, regardless of which direction the field is applied. This is known as magnetic isotropy. In contrast, magnetically anisotropic materials will be easier or harder to magnetize depending on which way the object is rotated. For most magnetically anisotropic materials, there are two easiest directions to magnetize the material, which are a 180° rotation apart. The line parallel to these directions is called the easy axis. In other words, the easy axis is an energetically favorable direction of spontaneous magnetization. Because the two opposite directions along an easy axis are usually equivalently easy to magnetize along, and the actual direction of magnetization can just as easily settle into either direction, which is an example of spontaneous symmetry breaking. Magnetic anisotropy is a prerequisite for hysteresis in ferromagnets: without it, a ferromagnet is superparamagnetic. The observed magnetic anisotropy in an object can happen for several different reasons. Rather than having a single cause, the overall magnetic anisotropy of a given object is often explained by a combination of these different factors: The magnetic anisotropy of a benzene ring (A), alkene (B), carbonyl (C), alkyne (D), and a more complex molecule (E) are shown in the figure. Each of these unsaturated functional groups (A-D) create a tiny magnetic field and hence some local anisotropic regions (shown as cones) in which the shielding effects and the chemical shifts are unusual. The bisazo compound (E) shows that the designated proton {H} can appear at different chemical shifts depending on the photoisomerization state of the azo groups. The trans isomer holds proton {H} far from the cone of the benzene ring thus the magnetic anisotropy is not present. While the cis form holds proton {H} in the vicinity of the cone, shields it and decreases its chemical shift. This phenomenon enables a new set of nuclear Overhauser effect (NOE) interactions (shown in red) that come to existence in addition to the previously existing ones (show in blue). Suppose that a ferromagnet is single-domain in the strictest sense: the magnetization is uniform and rotates in unison. If the magnetic moment is μ {displaystyle scriptstyle {oldsymbol {mu }}} and the volume of the particle is V {displaystyle scriptstyle V} , the magnetization is M = μ / V = M s ( α , β , γ ) {displaystyle scriptstyle mathbf {M} ={oldsymbol {mu }}/V=M_{s}left(alpha ,eta ,gamma ight)} , where M s {displaystyle scriptstyle M_{s}} is the saturation magnetization and α , β , γ {displaystyle scriptstyle alpha ,eta ,gamma } are direction cosines (components of a unit vector) so α 2 + β 2 + γ 2 = 1 {displaystyle scriptstyle alpha ^{2}+eta ^{2}+gamma ^{2}=1} . The energy associated with magnetic anisotropy can depend on the direction cosines in various ways, the most common of which are discussed below. A magnetic particle with uniaxial anisotropy has one easy axis. If the easy axis is in the z {displaystyle z} direction, the anisotropy energy can be expressed as one of the forms: where V {displaystyle scriptstyle V} is the volume, K {displaystyle scriptstyle K} the anisotropy constant, and θ {displaystyle scriptstyle heta } the angle between the easy axis and the particle's magnetization. When shape anisotropy is explicitly considered, the symbol N {displaystyle scriptstyle {mathcal {N}}} is often used to indicate the anisotropy constant, instead of K {displaystyle scriptstyle K} . In the widely used Stoner–Wohlfarth model, the anisotropy is uniaxial. A magnetic particle with triaxial anisotropy still has a single easy axis, but it also has a hard axis (direction of maximum energy) and an intermediate axis (direction associated with a saddle point in the energy). The coordinates can be chosen so the energy has the form