Towards surface experiments at HITRAP Erwin Bodewits , H. Bekker, - - PowerPoint PPT Presentation

towards surface experiments at hitrap
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Towards surface experiments at HITRAP Erwin Bodewits , H. Bekker, - - PowerPoint PPT Presentation

Towards surface experiments at HITRAP Erwin Bodewits , H. Bekker, A.J. de Nijs, D.Winklehner, B.Daniel, G. Kowarik, K. Dobes, F. Aumayr and Ronnie Hoekstra atom ic physics Introduction HITRAP - GSI Facility for slow highly charged ions


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SLIDE 1

Towards surface experiments at HITRAP

Erwin Bodewits, H. Bekker, A.J. de Nijs, D.Winklehner, B.Daniel,

  • G. Kowarik, K. Dobes, F. Aumayr and Ronnie Hoekstra

atom ic physics

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SLIDE 2

Introduction

HITRAP - GSI Facility for slow highly charged ions

(kinetic energy ~keV, potential energy up to 1MeV!)

Electron dynamics Metallic vs. insulating surfaces Electron capture according to the classical over the barrier model New IISIS set up First results on C60/Au system

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SLIDE 3

Artistic impression

Hollow atom formation

Tim e All processes happen on a femtosecond scale

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SLIDE 4

Some electronic processes

according to the classical over the barrier model

Burgdörfer et al, PRA 4 4 (1991) 5647

distance of first electron capture: D= (2q) 1/ 2 / Wφ into the shell n≈q High q – (very) large distance when first capture occurs

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SLIDE 5

IISIS: multi-user station for HITRAP

Inelastic Ion Surface Interactions Set-up

El.Stat.Det. X-ray det. surface analysis evaporator Target manipulator

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SLIDE 6

IISIS: electron statistics detection

Aumayr et al.

N3+ Xe12+

Intensity Number of electrons Number k probability

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SLIDE 7

IISIS: first electron yield data

Intensity Number of electrons

Xeq+ - Au

Meissl et al, J. Surf. Sci. Nanotech 6 (2008) 54

Charge state Electron yield O3+ Xe24+

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SLIDE 8

12xq keV Xeq+ - Au

γ/q vs q 4d shell 4p shell

Charge state Yield (electrons/ion charge)

γ vs Epot

Electron yield (electron/ion) Potential energy (eV) slope 140 ~70 eV/emitted electron

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SLIDE 9

First data on C60 films on Au Changing the electronic structure

Film production (Omicron evaporator) in situ calibration evaporation on quartz microbalance comparison to 1ML C60 produced via “heating recipe”

7xq keV Xeq+ - C60/ Au at different angles of incidence: 10o, 45o and 60o q= 10 q= 16 q= 23

Number of monolayers Number of monolayers Number of monolayers

Yield Yield Yield

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SLIDE 10

Relative electron yield versus C60 coverage

10+ 16+ 23+ 7xq keV Xeq+ - C60/ Au films

Number of monolayers

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SLIDE 11

Insulator versus metal

capture distance – states/ time resonant ionization secondary electrons escape depth

Metal C60 Wf

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SLIDE 12

conclusions

I I SI S

I nelastic I on Surface I nteractions Set-up

electron statistics detection at low energy first tests on C6 0 / Au succesfull rem aining issues: Further characterization of the film / surfaces full scale sim ulations at low energy

( inc. angle, position of beam ,...)

incorporation of X-ray detection

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SLIDE 13

Thank you for you attention!

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SLIDE 14

Maxwell et al, PRB 4 9 (1994) 10717

densities of states

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SLIDE 15

IISIS: deceleration and transport

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SLIDE 16

Experiments at HITRAP

TRAMPOLINE effect

  • n insulators

Surface lithography Exotic, spin-polarized hollow atoms Magnetized surfaces metals vs. insulators Thin films

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SLIDE 17

first generation of experiments

Not yet optimal HITRAP beams No hard constraints on beam energies

Surface lithography THIN FILMS: bridges between metals and insulators

electron statistics microscopy

(in collaboration with Aumayr et al (Vienna))

simultaneously look for X ray spectra

(in collaboration with Stöhlker et al (GSI))

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SLIDE 18

Some electron capture processes

according to the classical over the barrier model

Radiative transition electron resonant ionization/neutralization

Auger neutralization

distance of first electron capture: D= (2q) 1/ 2 / Wφ into n≈q

Auger deexcitation Auto ionization

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SLIDE 19

Eder et al, NIMB 1 5 4 (1999) 185

~ 0.3 keV/ amu kinetic emission threshold electronic KE eKE collisional KE cKE potential energy em ission PE

~4keV ~100keV

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SLIDE 20

First data on C60 films on Au

Film production (Omicron evaporator) in situ calibration evaporation on quartz microbalance comparison to 1ML C60 produced via “heating recipe”

168 keV Xe24+ - 1 ML C60/ Au kinetic electron emission: γ= γ0 + γθcos-1θ potential electron emission: γ= γ0 + γθcos−0.5θ