We review theoretical progress and prospects for determining the nucleon's static dipole polarisabilities from Compton scattering on few-nucleon targets, including new values and an emphasis on what polarised targets and beams can contribute; see Refs. [1][2][3][4][5] for details and a more thorough bibliography.
I. WHY COMPTON SCATTERING?Let us start with an even simpler question: Why can you see any speaker at a conference? Light shines on matter, gets absorbed, and is re-emitted before it reaches your eyes. That is Compton scattering γX → γX. A white shirt and red jumper reflect light differently because they have different chemical compositions: one reemits radiation quite uniformly over the visible band, the other absorbs most non-red photons. The speaker's attire therefore not only shows their fashion sense (or lack thereof), but betrays information about the stuff of which they are made.Let's be a bit more scientific. In Compton scattering γX → γX, the electromagnetic field of a real photon induces radiation multipoles by displacing charged constituents and currents inside the target. The energyand angle-dependence of the emitted radiation carries information on the interactions of the constituents. In Hadronic Physics, it elucidates the distribution, symmetries and dynamics of the charges and currents which constitute the low-energy degrees of freedom inside the nucleon and nucleus, and -for nuclei -the interactions between nucleons, complementing information from onephoton data like form factors; see e.g. a recent review [1]. In contradistinction to many other electromagnetic processes, such structure effects have only recently been subjected to a multipole-analysis. The Fourier transforms of the corresponding temporal response functions are the proportionality constants between incident field and induced multipole. These energy-dependent polarisabilities parametrise the stiffness of the nucleon N (spin σ/2) against transitions Xl → Y l of given photon multipolarity at fixed frequency ω (l = l ± {0; 1}; X, Y = E, M ;. Up to about 400 MeV, the relevant terms are:The two spin-independent polarisabilities α E1 (ω) and β M 1 (ω) parametrise electric and magnetic dipole transitions. Of particular interest at present are now the four dipole spin-polarisabilities γ E1E1 (ω), γ M 1M 1 (ω), γ E1M 2 (ω) and γ M 1E2 (ω). They encode the response of the nucleon's spin structure, i.e. of the spin constituents, and complement JLab experiments at much higher energies. Intuitively interpreted, the electromagnetic field associated with the spin degrees causes birefringence in the nucleon (cf. classical Faraday-effect). Only the linear combinations γ 0 and γ π of scattering under (0 • and 180 • scattering) are somewhat constrained by data or * hgrie@gwu.edu; corresponding author. Invited Contribution to the 22nd International Spin Symposium (SPIN 2016), University of Illinois, Urbana (USA), 26-30 September 2016.phenomenology , with conflicting results for the proton (MAMI, LEGS) and large error-bars for the neutron.The sp...