Calculation of Ionization Equilibrium for Dense Plasmas
نویسندگان
چکیده
منابع مشابه
Quantum-Mechanical Calculation of Ionization-Potential Lowering in Dense Plasmas
Sang-Kil Son (손상길), Robert Thiele, Zoltan Jurek, Beata Ziaja, and Robin Santra Center for Free-Electron Laser Science, DESY, Notkestrasse 85, 22607 Hamburg, Germany The Hamburg Centre for Ultrafast Imaging, Luruper Chaussee 149, 22761 Hamburg, Germany Institute of Nuclear Physics, Polish Academy of Sciences, Radzikowskiego 152, 31-342 Kraków, Poland Department of Physics, University of Hamburg,...
متن کاملIonization rate coefficients in warm dense plasmas.
We recast the atomic processes in a warm, dense plasma using Fermi-Dirac statistics and compare them to the rates of the usual Maxwell-Boltzmann approach of many collisional-radiative models. Population calculations show insignificant differences to calculations assuming nondegenerate free electrons of plasmas at solid density close to local thermodynamic equilibrium, but show departures in ave...
متن کاملAdiabatic Equation of State and Ionization Equilibrium of Dense Plasma
We consider the adiabatic equation of state for partially ionized non{ideal plasma. Plasma isentropes are calculated with the Pad e technique in the chemical picture. The interplay of ionization/dissociation equilibrium and non{ideality is investigated.
متن کاملOptimally Local Dense Conditions for the Existence of Solutions for Vector Equilibrium Problems
In this paper, by using C-sequentially sign property for bifunctions, we provide sufficient conditions that ensure the existence of solutions of some vector equilibrium problems in Hausdorff topological vector spaces which ordered by a cone. The conditions which we consider are not imposed on the whole domain of the operators involved, but just on a locally segment-dense subset of the domain.
متن کاملIonization Equilibrium and Equation of State of Hydrogen Plasmas in Strong Magnetic Fields
We study hydrogen plasmas at magnetic fields B ∼ 10 − 10 G, densities ρ ∼ 10 − 10 g cm and temperatures T ∼ 10−10 K, typical of photospheres of middle-aged cooling neutron stars. We construct an analytical free energy model of the partially ionized plasma, including into consideration the decentred atomic states, which arise due to the thermal motion across the strong field. We show that these ...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: International Astronomical Union Colloquium
سال: 1993
ISSN: 0252-9211
DOI: 10.1017/s0252921100017875