Transcript Mesh

TRIGGERING EXCIMER LASERS BY
PHOTOIONIZATION FROM A CORONA
DISCHARGE*
Zhongmin Xiong and Mark J. Kushner
University of Michigan
Ann Arbor, MI 48105 USA
[email protected] [email protected]
Thomas Duffey and Daniel Brown
Cymer, Inc. San Diego, CA 92127
[email protected]
October 2009
* Work supported by Cymer, Inc.
AGENDA
 Excimer discharge excited lasers for photolithography
 Preionization schemes
 Description of Model
 Discharge triggering sequence
 Dependence on corona bar properties
 Concluding Remarks
ANDY_GEC2009
University of Michigan
Institute for Plasma Science & Engr.
EXCIMER LASERS FOR PHOTOLITHOGRAPHY
 Discharge excited excimer lasers operate in the UV on bound-free
transitions of rare-gas halogens
 Typical conditions: many atms, a few cm gap, pulsed 10s kV in 10s ns.
Ar+ + FAr* + F2
ArF*
E(R)
Laser
ArF
 e + Ar  Ar* + e
 e + Ar  Ar+ + 2e
 e + F2  F + FAr, F
R
 Coherent, short
wavelengths have
made ArF (193 nm) the
source of choice for
photolithography for
micro-electronics
fabrication.
(www.spie.org)
(Cymer Inc.)
ANDY_GEC2009
University of Michigan
Institute for Plasma Science & Engr.
PLASMA DISCHARGE and PRE-IONIZATION
 Gas mixtures contain highly attaching
halogens which places premium on high
preionization density for optimizing gain.
Frame 001  02 Oct 2009  CYMER_01E NE/AR/F2/XE (cymer_nlist_01b.nlist)
Insulator
e
 Preionization provided by UV illumination
from corona bar.
Frame 001  02 Oct 2009  CYMER_01E NE/AR/F2/XE (cymer_nlist_01b.nlist)
 Investigate preionization mechanisms.
Metal Corona
Bar (grounded)
0.25mm
Dielectric
Insulator
Cathode
5 cm
Ne/Ar/F2/Xe =
96.4/3.5/0.1/0.001
P = 2625 Torr
T = 338K
Anode
Insulator
12 cm
ANDY_GEC2009
University of Michigan
Institute for Plasma Science & Engr.
DESCRIPTION OF MODEL
 Discharge chamber and plasma kinetics modeled using nonPDPSIM
 Poisson’s Equation:
   e    N j q j  s
j
 Continuity equation for charged and neutral species:
N j
t

    j  S j

 s
   q j (   j  S j )    ( ())
 Surface charge balance
t
j
 nee   
5

 Bulk electron temperature:
 j  E  ne  Ni i     e  Te ,
t
2

i


j  qe
 Radiation transport for photons (more on this later)
 Secondary electron emission (ion and photons) from surfaces.
 Transport and rate coefficients obtained from solution of
Boltzmann’s equation for electron energy distribution.
ANDY_GEC2009
University of Michigan
Institute for Plasma Science & Engr.
REACTION MECHANISM
 Reaction mechanism contains 35 species, 12 charged species,
300+ reactions for Ne/Ar/F2/Xe mixtures.
 Operating pressures of  3 atm emphasize 3-body reactions
leading to rapid dimerization.
e + Ne  Ne+ + e + e
e + Ne  Ne* + e
Ne + Ne+ + M  Ne2+ + M
Ne + Ne* + M  Ne2* + M
e + Ar  Ar+ + e + e
e + Ar  Ar* + e
Ar + Ar+ + M  Ar2+ + M
Ar + Ar* + M  Ar2* + M
Ne2+ + Ar  Ar+ + Ne + Ne
Ne2* + Ar  Ar+ + Ne + Ne + e
e + F2  F- + F
 Ion-Ion neutralization
Ar2+ + F-  ArF* + Ar
ANDY_GEC2009
Ar+ + F- + M  ArF* + M
University of Michigan
Institute for Plasma Science & Engr.
PHOTOIONIZATION
 Excited stats generated by corona discharge produce VUV photons
which propagate to main discharge gap to photo-ionize low
ionization potential species for pre-ionization.
 Many species likely contribute to VUV flux – here we used Ne2* as
VUV source.
 Sufficient density and short enough lifetime to account for VUV
flux required to produce observed preionization densities –
radiation is not trapped.
 Xe has the lowest ionization potential in mixture and is the
photoionized atom.
 e + Ne  Ne* + e
 Ne* + 2Ne  Ne2* + Ne
 Ne2*  Ne + Ne + h
(15.5 eV, 800 A)
ANDY_GEC2009
 h + Xe  Xe+ + e
 Ionization potential: 12.13 eV
 [Xe] = 7.5 x 1014 cm-3
  = 10-16 cm2
University of Michigan
Institute for Plasma Science & Engr.
RADIATION TRANSPORT
Emission species j
 Radiation transport modeled using
propagator or Greens function
approach which relates photo flux at r
to density of excites states at r’.
Absobers k
 Includes view-factors.
 Rate of ionization



 
N (r )
3
   Ni (r ) N j (r ' ) Aj G j (r , r ' ) ij d r '
t
j

i
Ionized
Species i

r


 

exp    N k (r " ) kj dr "
 
k r '


G j (r , r ' ) 
  2
4 | r  r ' |
ANDY_GEC2009
A
Einstein coefficient
 ij
Photo-ionization cross section
 kj
Photo-absorption cross section
University of Michigan
Institute for Plasma Science & Engr.
COMPUTATIONAL MESH
e 001  05 Oct 2009  CYMER_01E NE/AR/F2/XE (cymer_nlist_01b.nlist)
 Unstructured mesh used to resolve
chamber geometry and large
dynamic range in dimensions.
 Total number of nodes: 9,336
 Plasma nodes:
5,607
ANDY_GEC2009
University of Michigan
Institute for Plasma Science & Engr.
ELECTRICAL POTENTIAL
 Cathode pulsed to -40 kV
 Avalanche breakdown
collapsed potential in gap.
 Ne/Ar/F2/Xe = 96.4/3.5/0.1/0.001
 2625 Torr, 338K
 Time: 0-35ns :
ANDY_GEC2009
University of Michigan
Institute for Plasma Science & Engr.
CORONA POTENTIAL
 Probe from cathode to corona
dielectric surface initiates
surface discharge.
 Charging of surface occurs
around the circumference.
ANDY_GEC2009
 Ne/Ar/F2/Xe = 96.4/3.5/0.1/0.001
 2625 Torr, 338K
 Time: 0-35ns :
University of Michigan
Institute for Plasma Science & Engr.
CORONA E-FIELD
 Electric field in surface
avalanche propagates around
circumference.
 Remaining charge produces
radial fields in corona bar.
 Surface charges on insulator
produce large sheath fields.
Cathode
ANDY_GEC2009
Corona
Bar
 Ne/Ar/F2/Xe = 96.4/3.5/0.1/0.001
 2625 Torr, 338K
 Time: 0-35ns :
University of Michigan
Institute for Plasma Science & Engr.
CORONA [e]
 Small [e] seeded near probe from
cathode.
 Avalanche along surface to > 1015
cm-3 penetrates through gaps.
 Photoionization seeds electrons
in remote high field regimes,
initiating local avalanche.
ANDY_GEC2009
 Ne/Ar/F2/Xe = 96.4/3.5/0.1/0.001
 2625 Torr, 338K
 Time: 0-35ns :
University of Michigan
Institute for Plasma Science & Engr.
Ne2* - VUV SOURCE
 Electron impact from surface
avalanche produces Ne*  Ne2*.
 Densities in excess of 1012 cm-3
produce photon sources of 1018
cm-3s-1.
 Untrapped VUV is penetrates
through to discharge gap.
ANDY_GEC2009
 Ne/Ar/F2/Xe = 96.4/3.5/0.1/0.001
 2625 Torr, 338K
 Time: 0-35ns :
University of Michigan
Institute for Plasma Science & Engr.
PHOTOIONIZATION
 VUV from all sources seeds
electrons by photoionization.
 Preionization density in gap >109
cm-3 prior to avalanche.
 During avalanche, “internal” VUVaccounts for > 10% of ionization.
ANDY_GEC2009
 Ne/Ar/F2/Xe = 96.4/3.5/0.1/0.001
 2625 Torr, 338K
 Time: 0-35ns :
University of Michigan
Institute for Plasma Science & Engr.
ELECTRON DENSITY
 Electron density > 1015 cm-3 in mid
gap – spreading from narrow anode
to broad cathode.
 Photoelectrons seed avalanches in
all high field regions.
ANDY_GEC2009
 Ne/Ar/F2/Xe = 96.4/3.5/0.1/0.001
 2625 Torr, 338K
 Time: 0-35ns :
University of Michigan
Institute for Plasma Science & Engr.
ArF* DENSITY
 The density of the excimer ArF*
produced in the discharge exceeds
1014 /cm3.
 ArF*  Ar + F produces laser output
ANDY_GEC2009
 Ne/Ar/F2/Xe = 96.4/3.5/0.1/0.001
 2625 Torr, 338K
 Time: 0-35ns :
University of Michigan
Institute for Plasma Science & Engr.
CORONA BAR e
2.E+10
1.E+10
1.E+10
 The capacitance of the corona bar
increases with e.
 Longer charging time produces
more VUV, increasing [e] in gap.
1.E+10
8.E+09
6.E+09
4.E+09
2.E+09
0.E+00
0
 Pre-ionization electron density at t=25ns
e=5
ANDY_GEC2009
e = 20
20
40
60
80
Corona Bar e/e0
e = 60
University of Michigan
Institute for Plasma Science & Engr.
CONCLUDING REMARKS
 Preionization by VUV photons from a corona bar was
investigated in an ArF excimer discharge laser.
 Photons emitted by Ne2* are sufficient to produce
preionization densities > 109 cm-3 in mid gap.
 VUV produces photoionization electrons in all high field
regions, seeding avalanche there.
 Degree of photoionization is controllable by dielectric
constant of corona bar.
ANDY_GEC2009
University of Michigan
Institute for Plasma Science & Engr.
BACKUP V-I Curves
Peak voltage difference across the gap reaches
40KV. Avalanche starts and decreases the voltage
difference.
Peal current exceeds 40KA before starting to decay
due to the drop of voltage.
ANDY_GEC2009
University of Michigan
Institute for Plasma Science & Engr.