Continuum Lowering -- A New Perspective
arXiv:1309.1456 · doi:10.1016/j.hedp.2014.04.003
Abstract
What is meant by continuum lowering and ionization potential depression (IPD) in a Coulomb system depends upon precisely what question is being asked. It is shown that equilibrium (equation-of-state) phenomena and non-equilibrium dynamical processes like photoionization are characterised by different values of the IPD. In the former, the ionization potential of an atom embedded in matter is the difference in the free energy of the many-body system between states of thermodynamic equilibrium differing by the ionization state of just one atom. Typically, this energy is less than that required to ionize the same atom in vacuo. Probably, the best known example of such an IPD is that of Stewart and Pyatt (SP). However, it is a common misconception that this formula should apply directly to the energy of a photon causing photoionization, since this is a local adiabatic process that occurs in the absence of a response from the surrounding plasma. To achieve the prescribed final equilibrium state, additional energy, in the form of heat and work, is transferred between the atom and its surroundings. This additional relaxation energy is sufficient to explain the discrepancy between recent spectroscopic measurements of IPD in dense plasmas and the predictions of the SP formula. This paper provides a detailed account of an analytical approach to calculating thermodynamic and spectroscopic (adiabatic) IPDs in multicomponent Coulomb systems of arbitrary coupling strength. The ramifications are carefully examined in order to elucidate the roles of the various IPD forms. A formulation in terms of free energy leads to an analytical equation of state (EoS) that is thermodynamically self-consistent, provided that the bound and free electrons are dynamically separable. Of the various proposed formulae, the Spectroscopic (adiabatic) IPD gives the most consistent agreement with spectroscopic measurements.
80 pages 3 figures. S1. Expanded intro incl: summary of experiments; outline of ionization process & basis of local non-equilibrium hypothesis; revised para on connection with microfield. S2. New para on connection with self-energy; outline of basic continuum-lowering model used to illustrate the new ideas. S3. Rearranged text. S6. Revised & retitled. References: expanded. Minor changes throughout
Cited by in corpus (17)
- A New Generation of Cool White Dwarf Atmosphere Models. I. Theoretical Framework and Applications to DZ Stars
- Carbon ionization at Gbar pressures: an ab initio perspective on astrophysical high-density plasmas
- Ionization potential depression and dynamical structure factor in dense plasmas
- Ab-initio calculations on two-electron ions in strongly coupled plasma environment
- Ionization potential depression and Pauli blocking in degenerate plasmas at extreme densities
- Laboratory Measurements of White Dwarf Photospheric Spectral Lines: H
- Kinetic modeling of x-ray laser-driven solid Al plasmas via particle-in-cell simulation
- First-principles derivation and properties of density-functional average-atom models
- Classical molecular dynamics simulations of hydrogen plasmas and development of an analytical statistical model for computational validity assessment
- Transient ionization potential depression in nonthermal dense plasmas at high x-ray intensity
- Plasma-environment effects on K lines of astrophysical interest III. IPs, K thresholds, radiative rates, and Auger widths in Fe ix - Fe xvi
- Investigating Mechanisms of State Localization in Highly-Ionized Dense Plasmas
- Predicting Excitation Energies in Warm Dense Matter
- Plasma environment effects on K lines of astrophysical interest. V. Universal formulae for ionization potential and K-threshold shifts
- Decreasing ultrafast X-ray pulse durations with saturable absorption and resonant transitions
- Pauli Blocking in Degenerate Plasmas and the Separable Potential Approach
- Ionization potential depression in degenerate plasmas and Pauli blocking of multi-electron ions