(Sub)millimeter Disk Polarization: a Brand New Window to Study Protoplanetary Disks
Title: (Sub)millimeter Disk Polarization: a Brand New Window to Study Protoplanetary Disks
Speaker: Dr. Haifeng Yang (Institute for Advance Study, Tsinghua University)
Time: 10:00am, July 12, 2021
Location: 5-516, PMO Xianlin Campus
Abstract: (Sub)millimeter disk polarization is an exciting new field that is being revolutionized by Atacama Large Millimeter/submillimeter Array (ALMA). Traditionally, (sub)millimeter polarization thermal emission from dusts were believed to trace the magnetic field structures, based on the assumption that grains are aligned with the background magnetic fields. Using polarization to trace magnetic field structure on the disk scale, however, has been a failure. Most systems show uniform polarization patterns, which can be well-explained with the scattering off dust grains themselves, the so-called “self-scattering” or “scattering-induced” mechanism. This opens up a brand new window to study the grain properties in protoplanetary disks (PPDs). Most notably, we have shown that the dust grains have grown to 100 micron in sizes in PPDs. These large dust grains are the building blocks of planetesimals and planets. Aside from probing grain sizes, it is also potentially capable to probe the settling of dust grains, among others.
Not all data can be explained with the self-scattering mechanism. The HL Tau Band 3 polarized image, for example, shows an azimuthal pattern which is beyond the scattering-induced mechanism. Aside from scattering, other mechanisms to produce disk polarization all rely on the dust grains being aligned with some underlying fields. Theoretically, the traditional magnetic alignment mechanism is expected to fail due to the disalignment by the frequent random bombardment from the gas particles. The favored grain alignment theory predicts the alignment of dust grains by the radiation flux. This mechanism, however, failed to explain the HL Tau Band 3 data, which can be explained by an old theory proposed by Gold in 1950s. This Gold mechanism is not favored in theory, because it is known to work only under (super) thermal conditions, but the differential motion in disks can hardly achieve thermal speed. The exact origin of complicated polarization patterns is still an open question. If we can settle on their origin, we will be able to harness the full power of ALMA polarization observation to study various properties of PPDs.