WS2011/ Ionization - Electron impact ionization & Photo ionization -

WS2011/ Overview 1.Atomic processes in plasma 2.Rate equation 3.Electron impact ionization 4.Photo ionization 5. Summary Example EBIT, Charge Exchange, Radiative Recombination Ionization mechanism: Multistep ionization, Ionization factor, approximation for cross section (Lotz formula), Carlson correction, optimal electron energy, application (electron target) Basics, cross section, application (RILIS)

WS2011/ A Z+ : Atom of species A with charge state Z e’ : electron changed energy 2.1. Overview: Atomic processes in a plasma collisions with electrons collisions with photons Impact Ionization Three-Body-Recombination (TBR) Impact excitationImpact disexcitation Photo ionizationRadiative Recombination (RR) ExcitationSpontaneous emission Photo absorptionBremsstrahlung Non-radiative transition Line spectrum The electron changes from one free state to another free state with lower energy. Continuous spectrum In most ion sources, ions are produced in a plasma. The basic atomic processes (selection) in plasmas are:

WS2011/ From these multiple processes arise the dynamic balance quantities: Distribution of the abundance of all charge states Z (=0...Z max ), Ionization equilibrium Number of emitted and absorbed photons per time interval, Radiative equilibrium The density of the particle species are determined from so-called rate equations: Example: impact ionization: 2.2. Rate equation ß z+1, TBR : rate coefficient for Three-Body-Recombination (TBR) The rate coefficients often not be calculated with sufficient precision; experimental data are only available to a limited extent. Therefore one tries to obtain data from thermo dynamical equilibrium. With decreasing electron density the TBR drops, so that the impact ionization is not in equilibrium with the TBR anymore. The RR rate also decreases but not as strong. With decreasing n e also the photo ionization becomes unlikely. As result the impact ionization and the RR-process dominate. The photons leave the plasma without being re-absorbed.

WS2011/ : averaged thermal ion velocity : cross sections for impact ionization, RR and charge exchange by collisions with residual gas : collision rate for all Coulomb collisions of ions with charge state i : depth of the electrostatic potential (radial and axial), : thermal energy of the ions heated by Coulomb collisions : electron density and velocity : neutral particle density Example EBIT: The solutions of the linear system of equations provides the charge state distribution in dependence on the ionization factor TOP: Ionization of pulsed injected argon gas by an electron beam with an energy of 3.9 keV, which inhibits the ionization of the charge state Ar 17+ (EBIS-Mode with breeding at the shell closure). BOTTOM: Capture and ionization for the case of continuously injected argon atoms and 6 keV electron beam energy (EBIT-Mode without RR and charge exchange with residual gas).

WS2011/ For the approximation of the charge exchange cross section, commonly the equation by Müller and Salzborn is used: Therein i describes the charge state of the highly charged ion and E ion, gas is the ionization potential of the gas atoms interacting with the ion. Example: Reachable charge states depending on the current density and the pressure Charge exchange:

WS2011/ For the approximation of the RR cross sections the semi-classical expression by Kim und Pratt is used. Their formula bases on the first theoretical description of the Radiative Recombination by Kramers (1923): Radiative Recombination (RR): with Ry: Rydberg energy 13,6 eV  : fine structure constant  0 ratio between the numbers of occupied and unoccupied states Z: nuclear charge q: charge state n: main quantum number ( e ) r : reduced Compton-wavelength E: electron energy with: the effective nuclear charge to take into account the shielding of the nuclear potential by the bound electrons the effective main quantum number to include the capture into states with different angular momentums

WS2011/ Electron impact ionization The electron impact ionization is the most fundamental ionization process for the operation of ion sources. The cross section for the impact ionization is by orders of magnitudes higher than the cross section for the photo ionization. The cross section depends on the mass of the colliding particle. Since the energy transfer of a heavy particle is lower, a proton needs for an identical ionization probability an ionization energy three orders of magnitudes higher than an electron Why?

WS2011/ There are two different possibilities to produce multiple charged ions: in a collision where many electrons are removed from the ion (double-ionization, triple-ionization, …) multistep or successive ionization, where only one electron is removed per collision and high charge states are produced in different collisions For energetic reasons the ionization releasing only one electron from the atomic shell is the most probable process. To produce highly charged ions the kinetic energy of the projectile electrons has to be at least equivalent to the n-th ionization potential. Electron impact Single ionization Electron impact Double ionization Mechanism for the impact ionization Cross section electron energy

WS2011/ Ionization energies up to 100 keV (U 91+ → U 92+ ) → shell structure of the atomic shells is clearly visible

WS2011/ Successive ionization: The probability for removing one electron and changing the charge state of the ion from q  q+1 is determined by the cross section  q  q+1 [cm 2 ]. Are the cross sections for the successive ionization known, the average ionization time of the ions with charge state q can be approximated from the collision frequency: The time between to ionizing collisions is This applies to electrons with a defined kinetic energy. The average ionization time in the charge state q depends only on the cross section and the current density. This expression is called IONISATION FACTOR. (Sometimes it is defined as only the inverse cross section!) Principle of electron impact ionization

WS2011/ Approximation of the cross section and the ionization time for the production of bare ions from H-like ions using the Mosley’s law for X-ray frequencies emitted in transitions from the continuum to the K-shell:  wherein  Example on the right side: The ionization factor j e *  for different charge states of Xe depending on the electron energy. The average time necessary to reach the charge state q is therewith: Examples: Argon can be ionized by 10 keV electrons, ions of the heavy elements by up to 100 keV electrons and Uranium by 150 keV electrons. The resulting values for the ionization energy, cross section and ionization factor are summarized in the table on the left side.

WS2011/ Approximation of the cross section in quantum-mechanical calculations done by Bethe (1930) using the Born Approximation: Scattering of a matter wave at a central potential V(r) for E kin >> E ion (perturbation theory). All electrons in an atom or ion contribute with their individual  ei to the total cross section , as long as the kinetic energy E kin of the projectile is larger then the ionization energy P i of these electrons. All q i electrons of the subshell contribute to the  i of the shell. The cross section for the ionization of the (n, l) - shell results from integration of the transition probabilities over all states n’, l’  k und the integration over the collision vector with v before and v’ after the collision. One receives Bethe et al., Ann. Physik 5 (1930) 325 N = number of subshells Approximation of the cross section for the electron impact ionization

WS2011/ For practical reasons the semi-empirical formula developed by Lotz 1967 for the energy dependence of the cross sections for the elements from H to Ca and for energies < 10 keV is commonly used. The error is given by maximal 10%. The Lotz formula for the case of high ionization energies E kin >> P i is: For E  P i and with (x  0), and with for x << 1 This means the cross section goes linear with E  P i to zero. Examples for the dependence of the cross sections on the energy are shown for the case of He. The higher the initial charge state, the smaller is the cross section. Moreover the cross section is higher for atoms in an excited state. P i = E nl, N-subshells This expressions is mostly used in calculations of the charge state distribution. follows

WS2011/ Single-ionisation: He + e → He + + 2eMulti-ionisation: He + e → He e

WS2011/ Ionization of singly charged He Ionization of the excited state He (2s) + e → He + + 2eHe + + e → He e

WS2011/ E 0i : binding energy of an electron in the i-th shell of an atom E 0q : atomic binding energy of the electron, which is the weakest bound electron in the ion of the charge state q W i (q) : ionization energy of the ion (describes always the weakest bound electron) inner electron i, to be removed The ionization energies P q,i for ions with different charge states q, which does not describe the weakest bound electron are sometimes difficult to find in literature. They can be approximated with the Carlson- Correction. The ionization energy P q,i is calculated from the ionization energy W i (q) of the ion with charge state q and the atomic binding energies of the electrons as follows: Carlson-Correction for ionization energies: weakest bound electron q (ionization energy is known) Ion: A q+ E 0q -E 0i

WS2011/ Because  (E) has a maximum at a certain energy, the ionization factor j e *  has a minimum there. Basically the cross section for the last electron, which is removed, determines the ionisation time. The optimal energy is given by For the optimal energy of the last electron, which is removed, follows: Therewith the optimal energy is nearly e-times the ionization energy of the last electron that is removed from the ion with the charge state z. Optimal electron energy

WS2011/ Ionization factor and optimal electron energy electron energy ionization factor

WS2011/ Application of the electron impact ionization for the production of ions Plasma confinement by magnetic fields of different structure (cusp, magnetic mirror, …) (see next lectures) The efficiency of the electrons in the plasma and the charge state can be increased by using the electron several times, by: - reflection of the electrons, e.g. reflection discharge or penning discharge - magnetic confinement, e.g. by magnetic mirrors

WS2011/ Further application of electron impact ionization Example: electron target Investigation of electron-ion-collisions: Investigation of electron impact ionization Investigation of recombination processes Investigation of excitation processes Measurement of rate coefficients R and therewith cross sections: A n+ Important is the overlap of ion and electron beam  : cross section n e : electron density n i : ion density v r : collision velocity / relative velocity f(v r ): distribution function of the relative velocity

WS2011/ “crossed beams technique” better energy resolution then gas target cm long interaction region spectroscopic access is possible electrostatic focusing BUT: lower interaction rate as longitudinal electron target or gas target Transversal electron targetLongitudinal electron target „Merged beams“. also used as cooler for ion beams 2-2.5m long interaction region BUT: limited access for spectroscopy 0.061A/cm, R=8.19 mesh units, J=0.2 A/cm 2

WS2011/ Atoms of a gas can be ionized by an intensive beam of photons with the adequate energy (photo ionization). Therefore the photon energy has to be. The energy of a photo electron is: The reaction is: 2.4. Photo ionization For a given atomic shell the cross section  p is the largest close to threshold, meaning where the photon energy reaches the ionization energy I (resonance/ threshold behavior): Cross section  p :  p has a strong dependence on the photon energy and the nuclear charge Z: Description of  p as time-inverse effect to the radiative recombination by the Milne-formula: For high photon energies the ionization of the s-orbital is most probable and the K-shell ionization delivers the dominant contribution: with g: statistical weights →  pn : cross section for RR into the K-shell n: main quantum number

WS2011/ RILIS (Resonant ionization laser ion source) Ionization via resonant excitation with three laser beams of frequencies f 1 – f 3, as shown in the following scheme. Application of photo ionization for the production of ions 1 eV  l = 1.24 mm (IR-radiation),5 eV  l = 248 nm (close UV) For direct ionization photons from the UV – x-ray region are necessary.

WS2011/ In reality there a many more effects to be takeen into account: Excitation schemes used for resonant laser ionization Excitation into auto-ionizing state (AIS) with typical lifetimes of – s Excitation in Rydberg-states n = n* Lifetime Binding energy Radius of Rydberg atoms R = Rydberg constant Orders of magnitudes for the cross sections: non-resonant (direct ionization):  = – cm 2 AIS:  = 1.6 x cm 2 Rydberg states:  ~ cm 2

WS2011/ A prominent example for a RILIS is at ISOLDE/CERN (see picture). Advantages of a RILIS: high selectivity separation of surface-ionizing contaminations by adjusting the temperature of the cavity high efficiency

WS2011/ Processes increasing the charge state Processes decreasing the charge state 2.5. Summary: Ion production Ionization - single-ionization - double-ionization The production of higher charge states is a successive process The ionization has energy threshold → higher charge states need higher projectile energies (electron energies) Charge exchange (for low charge states) Recombination - radiative recombination The cross section is larger for lower electron temperatures - dielectronic recombination (resonant process) Charge exchange (for high charge states) depending on the neutral particle density (residual gas) cross section are larger for higher charge states

WS2011/ Spouses never need to worry about what their ion source physicist husband or wife is up to when they still aren’t home by midnight...they know with great confidence that they’re just at the lab changing a source! 9. Between –the International Conference on Ion Sources, –the Workshop on Ion Source Issues Relevant to a Pulsed Spallation Neutron Source, –the ECR Ion Source Workshop, –The International Conference on Negative Ions, Beams and Sources, –the International Symposium on the Production and Neutralization of Negative Ions and Beams, –the Workshop on Negative Ion Formation and Beam Handling, –the International Conference on Sources of Highly Charged Ions, the ion source community has the greatest number of conferences and workshops of any scientific discipline measured per linear inch of subject matter 8. Endless hours can be devoted to the important philosophical meaning of “pi” as in “the output emittance is 0.2 pi-mm-mrad” 7. Believe it or not, sometimes the SNS ion source antenna picks up free Satellite Television! 6. High-voltage, hydrogen gas, antennas and power supplies: it’s every little kids dream! 5. In what other field can you acquire a Ph.D., and then spend your professional life practicing the occult? 4. When the phone rings during dinner time, you always know who it is: no its not a tele-marketer, it just the lab...the ion source went down! 3. In what other field could you advertise a workshop on “RF-driven, multicusp, Cesium-enhanced H-sources for the SNS”, and have 50 people actually show up? 2. Job security...when was the last time you heard a manager say, “the ion source is running so well, we’re going to let the entire group go.” 1. It’s a subject in which anyone can make a contribution, and everyone has an opinion! Courtesy of Stuart Henderson/ORNL