Alignment of Dust with Magnetic Inclusions: Radiative Torques and Superparamagnetic Barnett and Nuclear Relaxation
arXiv:0801.0265 · doi:10.1086/586706
Abstract
We consider grains with superparamagnetic inclusions and report two new condensed matter effects that can enhance the internal relaxation of the energy of a wobbling grain, namely, superparamagnetic Barnett relaxation, as well as, an increase of frequencies for which nuclear relaxation becomes important. This findings extends the range of grain sizes for which grains are thermally trapped, i.e. rotate thermally, in spite of the presence of uncompensated pinwheel torques. In addition, we show that the alignment of dust grains by radiative torques gets modified for superparamagnetic grains, with grains obtaining perfect alignment with respect to magnetic fields as soon as the grain gaseous randomization time gets larger than that of paramagnetic relaxation. The same conclusion is valid for the mechanical alignment of helical grains. If observations confirm that the degrees of alignment are higher than radiative torques can produce alone, this may be a proof of the presence of superparamagentic inclusions.
5 pages, emulated ApJ style, 2 figures, submitted to ApJL (earlier version was corrupted)
References in corpus (18)
- Radiative torques: Analytical Model and Basic Properties
- Tracing Magnetic Fields with Aligned Grains
- Radiative Torques on Interstellar Grains: I. Superthermal Spinup
- Radiative Torques on Interstellar Grains: II. Grain Alignment
- Magnetic Dipole Microwave Emission from Dust Grains
- The Efficiency of Grain Alignment in Dense Interstellar Clouds: A Reassessment of Constraints from Near Infrared Polarization
- Subsonic Mechanical Alignment of Irregular Grains
- Grain Alignment by Radiation in Dark Clouds and Cores
- Grain Alignment and Polarized Emission from Magnetized T Tauri Disks
- Nuclear Spin Relaxation within Interstellar Grains
- Polarization of Dust Emission in Clumpy Molecular Clouds and Cores
- Barnett Relaxation in Thermally-Rotating Grains
- Radiative Torques on Interstellar Grains. III. Dynamics with Thermal Relaxation
- Thermal Flipping and Thermal Trapping -- New Elements in Dust Grain Dynamics
- Circular polarization in comets: Observations of Comet C/1999 S4 (LINEAR) and tentative interpretation
- Davis-Greenstein alignment of non-spherical grains
- Simulations of polarized dust emission
- On the Disalignment of Interstellar Grains
Cited by in corpus (50)
- Radiative torque alignment: Essential Physical Processes
- A unified model of grain alignment: radiative alignment of interstellar grains with magnetic inclusions
- First results from BISTRO -- a SCUBA-2 polarimeter survey of the Gould Belt
- Radiative grain alignment in protoplanetary disks: Implications for polarimetric observations
- Grain Alignment by Radiative Torques in Special Conditions and Implications
- Velocity Gradients as a Tracer for Magnetic Fields
- Grain alignment induced by radiative torques: effects of internal relaxation of energy and complex radiation fields
- Cassiopeia A: dust factory revealed via submillimetre polarimetry
- Alignment of Irregular Grains by Mechanical Torques
- Radiative torques alignment in the presence of pinwheel torques
- Resolving the polarized dust emission of the disk around the massive star powering the HH~80-81 radio jet
- The Interstellar Magnetic Field Close to the Sun II
- Grain alignment and disruption by radiative torques in dense molecular clouds and implication for polarization holes
- Polarization of Magnetic Dipole Emission and Spinning Dust Emission from Magnetic Nanoparticles
- The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333
- Stringent Limits on the Polarized Submillimeter Emission from Protoplanetary Disks
- Physical Model of Dust Polarization by Radiative Torque Alignment and Disruption and Implications for Grain Internal Structures
- Constraint on the Polarization of Electric Dipole Emission from Spinning Dust
- Interstellar extinction and interstellar polarization: old and new models
- On Internal and External Alignment of Dust Grains in Protostellar Environments
- Magnetic Properties of Dust Grains, Effect of Precession and Radiative Torque Alignment
- Magnetic Fields in Massive Star-Forming Regions (MagMaR) I. Linear Polarized Imaging of the UCHII Region G5.89-0.39
- Paramagnetic alignment of small grains: a novel method for measuring interstellar magnetic fields
- Radiative torques of irregular grains: Describing the alignment of a grain ensemble
- Alignment and rotational disruption of dust
- Modeling Grain Alignment by Radiative Torques and Hydrogen Formation Torques in Reflection Nebula
- Interstellar polarization and grain alignment: the role of iron and silicon
- Properties and alignment of interstellar dust grains toward Type Ia Supernovae with anomalous polarization curves
- Alignment of irregular grains by radiative torques: efficiency study
- A systematic study of radiative torque grain alignment in the diffuse interstellar medium
- Tracing Magnetic Fields with Ground State Alignment
- ALMA reveals the magnetic field evolution in the high-mass star forming complex G9.62+0.19
- Physical Modeling of Dust Polarization from Magnetically Enhanced Radiative Torque (MRAT) Alignment in Protostellar Cores with POLARIS
- Correlation between Interstellar Polarization and Dust Temperature: Alignment of Grains by Radiative Torques is Ubiquitous?
- The Mechanical Alignment of Dust (MAD) I: On the spin-up process of fractal grains by a gas-dust drift
- Two modes of carbonaceous dust alignment
- Polarization measurement analysis III. Analysis of the polarization angle dispersion function with high precision polarization data
- Thermal Flipping of Interstellar Grains
- Electric dipole moments and disalignment of interstellar dust grains
- Gamma-ray Burst Afterglows: Time-Varying Extinction, Polarization, and Colors due to Rotational Disruption of Dust Grains
- Cross section alignment of polycyclic aromatic hydrocarbons by anisotropic radiation
- Physical conditions for dust grain alignment in Class 0 protostellar cores II. The role of the radiation field in models aligning/disrupting dust grains
- Evidence of Grain Alignment by Magnetically Enhanced Radiative Torques from Multiwavelength Dust Polarization Modeling of HL Tau
- ALMA reveals the coherence of the magnetic field geometry in OH 231.8+4.2
- Synthetic Modelling of Polarized Dust Emission in Intermediate-Mass YSOs: I: Constraining the Role of Iron Inclusions and Inelastic Relaxation on Grain Alignment with ALMA Polarization
- Spinning Dust Emission from Wobbling Grains: Important Physical Effects and Implications
- Alignment and Rotational Disruption of Dust Grains in the Galactic Centre Revealed by Polarized Dust Emission
- Grain Alignment: Role of Radiative Torques and Paramagnetic Relaxation
- The radiative torque spin-up efficiency of ballistic dust grain aggregates
- Grain alignment and dust evolution physics with polarisation (GRADE-POL). I. Dust polarisation modelling for isolated starless cores