Graphite Revisited
arXiv:1608.02975 · doi:10.3847/0004-637X/831/1/109
Abstract
Laboratory measurements are used to constrain the dielectric tensor for graphite, from microwave to X-ray frequencies. The dielectric tensor is strongly anisotropic even at X-ray energies. The discrete dipole approximation is employed for accurate calculations of absorption and scattering by single-crystal graphite spheres and spheroids. For randomly-oriented single-crystal grains, the so-called 1/3 - 2/3 approximation for calculating absorption and scattering cross sections is exact in the limit a/lambda -> 0, provides better than ~10% accuracy in the optical and UV even when a/lambda is not small, but becomes increasingly inaccurate at infrared wavelengths, with errors as large as ~40% at lambda = 10 micron. For turbostratic graphite grains, the Bruggeman and Maxwell Garnett treatments yield similar cross sections in the optical and ultraviolet, but diverge in the infrared, with predicted cross sections differing by over an order of magnitude in the far-infrared. It is argued that the Maxwell Garnett estimate is likely to be more realistic, and is recommended. The out-of-plane lattice resonance of graphite near 11.5 micron may be observable in absorption with the MIRI spectrograph on JWST. Aligned graphite grains, if present in the ISM, could produce polarized X-ray absorption and polarized X-ray scattering near the carbon K edge.
To appear in ApJ
References in corpus (21)
- The chemical composition of the Sun
- Energy Band Gap Engineering of Graphene Nanoribbons
- Dust Grain Size Distributions and Extinction in the Milky Way, LMC, and SMC
- Infrared Emission from Interstellar Dust. IV. The Silicate-Graphite-PAH Model in the Post-Spitzer Era
- Universal dynamical conductance in graphite
- Present-day cosmic abundances. A comprehensive study of nearby early B-type stars and implications for stellar and Galactic evolution and interstellar dust models
- The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point
- On Ultrasmall Silicate Grains in the Diffuse Interstellar Medium
- Near-edge x-ray absorption fine structure investigation of graphene
- Identification of more interstellar C60+ bands
- Unidentified Infrared Emission bands: PAHs or MAONs?
- Variations on a theme - the evolution of hydrocarbon solids: I. Compositional and spectral modelling - the eRCN and DG models
- The Carriers of the Interstellar Unidentified Infrared Emission Features: Aromatic or Aliphatic?
- Variations on a theme - the evolution of hydrocarbon solids: II. Optical property modelling - the optEC(s) model
- Variations on a theme - the evolution of hydrocarbon solids: III. Size-dependent properties - the optEC(s)(a) model
- Discrete-dipole approximation with polarizabilities that account for both finite wavelength and target geometry
- The Carriers of the Interstellar Unidentified Infrared Emission Features: Constraints from the Interstellar C-H Stretching Features at 3.2-3.5 Micrometers
- Temperature evolution of infrared- and Raman-active phonons in graphite
- Some optical properties of graphite from IR to millimetric wavelengths
- A polycrystalline graphite model for the 2175 Angstrom interstellar extinction band
- Infrared phonon activity in pristine graphite
Cited by in corpus (20)
- Detection of the Aromatic Molecule Benzonitrile (-CHCN) in the Interstellar Medium
- The Astrodust+PAH Model: A Unified Description of the Extinction, Emission, and Polarization from Dust in the Diffuse Interstellar Medium
- Excitation of Polycyclic Aromatic Hydrocarbon (PAH) Emission: Dependence on Size Distribution, Ionization, and Starlight Spectrum and Intensity
- Observational Constraints on the Physical Properties of Interstellar Dust in the Post-Planck Era
- Detection of PAH Absorption and Determination of the Mid-Infrared Diffuse Interstellar Extinction Curve from the Sightline Toward Cyg OB2-12
- The first spectroscopic dust reverberation programme on active galactic nuclei: the torus in NGC 5548
- First-principles theory of infrared vibrational spectroscopy in metals and semimetals: application to graphite
- Radiative transfer of ionizing radiation through gas and dust: stellar source case
- Extended Dust Emission from Nearby Evolved Stars
- Benchmarking Dust Emission Models in M101
- How Much Graphene in Space?
- Probing the 9.7μm Interstellar Silicate Extinction Profile through the Spitzer/IRS Spectroscopy of OB Stars
- On Carbon Nanotubes in the Interstellar Medium
- A study in scarlet -- I. Photometric properties of a sample of Intermediate Luminosity Red Transients
- A complex dust morphology in the high-luminosity AGN Mrk 876
- The Nearby Evolved Stars Survey: I. JCMT/SCUBA-2 Sub-millimetre detection of the detached shell of U Antliae
- Ionization chemistry in the inner disc: a combined treatment of ionic and thermionic emission and arbitrary grain size distributions
- X-ray Spectroscopy of Interstellar Carbon: Evidence for Scattering by Carbon-Bearing Material in the Spectrum of 1ES 1553+113
- The first spectroscopic IR reverberation programme on Mrk 509
- The MATISSE view of the inner region of the RY Tau protoplanetary disk