.. _magnetism: Polarisation/Magnetic Scattering ================================ Models which define a scattering length density parameter can be evaluated as magnetic models. In general, the scattering length density (SLD = $\beta$) in each region where the SLD is uniform, is a combination of the nuclear and magnetic SLDs and, for polarised neutrons, also depends on the spin states of the neutrons. For magnetic scattering, only the magnetization component $\mathbf{M_\perp}$ perpendicular to the scattering vector $\mathbf{Q}$ contributes to the magnetic scattering length. .. figure:: mag_img/mag_vector.png The magnetic scattering length density is then .. math:: \beta_M = \dfrac{\gamma r_0}{2\mu_B}\sigma \cdot \mathbf{M_\perp} = D_M\sigma \cdot \mathbf{M_\perp} where $\gamma = -1.913$ is the gyromagnetic ratio, $\mu_B$ is the Bohr magneton, $r_0$ is the classical radius of electron, and $\sigma$ is the Pauli spin. Assuming that incident neutrons are polarized parallel (+) and anti-parallel (-) to the $x'$ axis, the possible spin states after the sample are then Non spin-flip (+ +) and (- -) Spin-flip (+ -) and (- +) .. figure:: mag_img/M_angles_pic.png If the angles of the $Q$ vector and the spin-axis $x'$ to the $x$ - axis are $\phi$ and $\theta_{up}$, respectively, then, depending on the spin state of the neutrons, the scattering length densities, including the nuclear scattering length density $(\beta{_N})$ are .. math:: \beta_{\pm\pm} = \beta_N \mp D_M M_{\perp x'} \text{ for non spin-flip states} and .. math:: \beta_{\pm\mp} = -D_M (M_{\perp y'} \pm iM_{\perp z'}) \text{ for spin-flip states} where .. math:: M_{\perp x'} &= M_{0q_x}\cos(\theta_{up})+M_{0q_y}\sin(\theta_{up}) \\ M_{\perp y'} &= M_{0q_y}\cos(\theta_{up})-M_{0q_x}\sin(\theta_{up}) \\ M_{\perp z'} &= M_{0z} \\ M_{0q_x} &= (M_{0x}\cos\phi - M_{0y}\sin\phi)\cos\phi \\ M_{0q_y} &= (M_{0y}\sin\phi - M_{0x}\cos\phi)\sin\phi Here, $M_{0x}$, $M_{0x}$, $M_{0z}$ are the x, y and z components of the magnetization vector given in the laboratory xyz frame given by .. math:: M_{0x} &= M_0\cos\theta_M\cos\phi_M \\ M_{0y} &= M_0\sin\theta_M \\ M_{0z} &= -M_0\cos\theta_M\sin\phi_M and the magnetization angles $\theta_M$ and $\phi_M$ are defined in the figure above. The user input parameters are: =========== ================================================================ M0_sld = $D_M M_0$ Up_theta = $\theta_\mathrm{up}$ M_theta = $\theta_M$ M_phi = $\phi_M$ Up_frac_i = (spin up)/(spin up + spin down) neutrons *before* the sample Up_frac_f = (spin up)/(spin up + spin down) neutrons *after* the sample =========== ================================================================ .. note:: The values of the 'Up_frac_i' and 'Up_frac_f' must be in the range 0 to 1. *Document History* | 2015-05-02 Steve King | 2017-05-08 Paul Kienzle