Rayleigh scattering from hydrogen atoms including resonances and high photon energies
arXiv:2208.02111 · doi:10.1051/0004-6361/202243883
Abstract
The non-relativistic cross section from Rayleigh scattering by hydrogen atoms in the ground state is calculated over a wide range of photon energies ( keV). Evaluations are performed in terms of the real and imaginary components of the atomic polarizability. The sum over intermediate states that characterizes this second-order radiative process is performed using exact analytic expressions for oscillator strengths of bound and continuum states. Damping terms associated with the finite lifetimes of excited states and their splitting into two fine-structure levels ( and ) are taken into account in resonance cross sections. Fitting formulas required for cross-section evaluation are presented for incident photon energy i) redward of the first resonance (Lyman-), ii) in the spectral region corresponding to resonances (for an arbitrary number of them), and iii) above the ionization threshold.
arXiv comment8 pages, 7 figures. Accepted for publication in Astronomy & Astrophysics
References in corpus (17)
- Photodissociation and photoionisation of atoms and molecules of astrophysical interest
- Rayleigh scattering in the transit spectrum of HD 189733b
- HST hot-Jupiter transmission spectral survey: detection of potassium in WASP-31b along with a cloud deck and Rayleigh scattering
- A New Generation of Los Alamos Opacity Tables
- Low-temperature gas opacity - AESOPUS: a versatile and quick computational tool
- Radiative transfer with scattering for domain-decomposed 3D MHD simulations of cool stellar atmospheres
- The propagation of Lyman-alpha in evolving protoplanetary disks
- 3D LTE spectral line formation with scattering in red giant stars
- Rayleigh Scattering and Microwave Background Fluctuations
- Rayleigh Scattering Cross Section Redward of Ly by Atomic Hydrogen
- The Effects of Rayleigh Scattering on the CMB and Cosmic Structure
- Rayleigh scattering in dense fluid helium
- Relativistic dynamical polarizability of hydrogen-like atoms
- Optab: Public code for generating gas opacity tables for radiation hydrodynamics simulations
- Cosmology with Rayleigh Scattering of the Cosmic Microwave Background
- Rayleigh scattering in the atmospheres of hot stars
- Measuring the orbital inclination of Z Andromedae from Rayleigh scattering