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Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes * , D.W. Chandler * , H.V. Linnartz and S. Stolte Department of Physical Chemistry, De Boelelaan 1083, 1081 HV Amsterdam vrije Universiteit amsterdam * Combustion Research Facility, Sandia National Laboratories, Livermore, California 94550
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Page 1: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Quantum Interference as the Source of

Stereo-Dynamic Effects in NO-Rare Gas Scattering

A. Gijsbertsen, C.A. Taatjes*, D.W. Chandler*, H.V. Linnartz and S. Stolte

Department of Physical Chemistry,

De Boelelaan 1083, 1081 HV Amsterdam

vrije Universiteit amsterdam

*Combustion Research Facility, Sandia National Laboratories, Livermore, California 94550

Page 2: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Outline

1. Introduction

2. Quasi-Quantum Treatment

3. Ion Imaging Experiments

4. Differential Cross Sections (DCSs)

5. Parity Effects

6. Conclusions and Outlook

Page 3: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Introduction

La se r b e a m

Prim a ry b e a m va lve (16 % N O /Ar)

Se c o nd a ry b e a m Va lve (Ar)He xa p o le sta te se le c to r

Le ns syste m a ndp ho to m ultip lie r

O rie nta tio n fie ldLig ht b a ffle s

oriented 21/2 NO ( j = ½, = -1) + R

21/2 NO ( j’, ’ ) + RWith R = Ar, He, D2,...

Page 4: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

The NO molecules are rotationally excited due to collisions with rare gas atoms.

Laser Induced Fluorescence (LIF) is used to measure the amount of molecules present in a particular rotational state after collision: it provides the total collision cross section .

The steric asymmetry S is given by:

Introduction

Page 5: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

NO-Ar, Etr 500 cm-1

NO-He, Etr 500 cm-1

Sif

Sif

Introduction

N-end j = odd dominatesO-end j = even dominates

Page 6: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Introduction

Page 7: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Introduction

A close coupling treatment reproduces experimental Sif:

- it showed that the oscillatory Sif is due to the anisotropy in the hard shell of R-NO potential*.

- it offers no explanation for undulative dependence upon j’ !

Our goal is to construct a quasi-quantum mechanical model to: obtain more information about the physical background of the steric asymmetry

*(Alexander, Stolte, J. Chem. Phys. 112 (2000) 437)

Page 8: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Introduction

Rainbow undulation for atom-atom scattering are caused by the pathway interference of 3 “rays” with different impact parameters:

H. Pauly et al. 1966

Page 9: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Quasi-Quantum treatment

The state selected wave function contains all NO orientations.

Assuming a hard shell the scattering angle is determined only by the angle between the surface normal and the incoming momentum ħk.

At fixed an infinite number of “rays” with different impact parameters b interfere, due to different path lengths.

Page 10: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Equipotential shell surface at Etr.

Quasi-Quantum treatment

Page 11: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Quasi-Quantum treatment

The kinematic apse n points perpendicularly to the hard shell. The projection of the rotational angular momentum (mj) is conserved along n.

The difference between the “hard shell” trajectory and the virtual pathway through the center of mass yields the phase shift .

^

^^

Page 12: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

k||

k

k

k’ (j = 0)

k’ (j = 1)

k’ (j = 2)

k’ (j = 3)

k’ (j = 4)

k’|| (= k||)

k’

Assuming a hard shell, only the momentum component perpendicular to the shell (k) can be transformed into rotation.The scattering angle depends on:1. Spacing between rotational states2. Angle between incoming momentum and apse.

Quasi-Quantum treatment

Page 13: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Quasi-Quantum treatment

Page 14: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Quasi-Quantum treatment

The phase shift for several rotational states, as function of n.

In this case cos()=-1.

O-end N-end

Page 15: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

The asymptotic solution of the Schrödinger equation at large distance, can be expressed as:

The differential cross section relates to the dimensionless scattering amplitude:

Remind, in the hard shell model, mj is conserved along the kinematic apse: mj’ =mj in the apse frame.

Vdiff is ignored, so ’=.

Quasi-Quantum treatment

Page 16: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

The scattering amplitude resulting from the hard shell model can be expressed as:

Where w takes care of the non-isotropic shape of the shell:

with:

The conservation of flux is taken care of by introducing C()

Note the elimination of the quantum numbers l and l’ !

Quasi Quantum treatment

Page 17: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Quasi Quantum treatment

Flux conservation correction C()2

Page 18: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Note that:

After some algebra one finds:

The distinguishes between the orientations.

If positive Head collisionsIf negative Tail collisions

Quasi Quantum treatment

Page 19: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Quasi Quantum treatmentThe orientation dependent DCS can be written as:

Note that:

in which “+” denotes N-end and “–” O-end collision;

From which follows: !

Increasing j’ j’+1, switches the orientation preference!

Page 20: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Quasi Quantum treatment

Page 21: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Quasi Quantum treatment

max

cos(w)cos(w)

O-end preference

Page 22: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Quasi Quantum treatment

-

Page 23: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Quasi Quantum treatment

A non-oriented NO wave function has parity

the DCS follows as:

Note parity-pairs of similar DCSs, that can be observed:

etc.

:

Page 24: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

NO source chamber

He source

XeCl excimer laser

dye laser

308 nm, 5 mJ

226 nm, 1 mJ He

Hexapole

NO

collision chamber

Experiments

Hexapole state selected NO collides with He at Ecoll 500 cm-1:

Crossed 1+1’ REMPI detection

excitation 226 nmionization 308 nm

NO (j=½, =½, =-1) NO ( j’, ’, ’ )

Page 25: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

50

100

150

200

250

300

150 200 250 300 350

200

250

300

350

400

450

Experiments

To test our setup, some 2% NO was seeded in the He beam.

The NO beam consists of 16 % NO in Ar.

This image reflects the velocity distributions for both our pulsed beams.

vNO

vHe

Page 26: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

*

j’ = 1.5 j’ = 2.5 j’ = 3.5 j’ = 4.5 j’ = 5.5 j’ = 6.5

j’ = 7.5 j’ = 8.5 j’ = 9.5 j’ = 10.5 j’ = 11.5 j’ = 12.5

*

Parity conserving: p’ = p = - 1

Experiments

Marked images are from Q-branch transitions that are more sensitive to rotational alignment and show more asymmetry.These images were omitted for the extraction of the DCS.

Page 27: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

*****

j’ = 1.5 j’ = 2.5 j’ = 3.5 j’ = 4.5 j’ = 5.5 j’ = 6.5

j’ = 7.5 j’ = 8.5 j’ = 9.5 j’ = 10.5 j’ = 11.5 j’ = 12.5

Parity breaking: p’ = - p = 1

Experiments

Page 28: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Parity conserving: p’ = p = - 1, DCSs

j’=1.5 j’=2.5 j’=3.5

j’=4.5 j’=5.5 j’=6.5

[o] [o] [o]

[o] [o] [o]

[Å2]

[Å2][Å2] [Å2]

[Å2][Å2]

Page 29: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Parity conserving: p’ = p = - 1, DCSs

j’=7.5 j’=8.5 j’=9.5

j’=10.5 j’=11.5 j’=12.5

[o] [o] [o]

[o] [o] [o]

[Å2]

[Å2][Å2] [Å2]

[Å2][Å2]

Page 30: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

j’=1.5 j’=2.5 j’=3.5

j’=4.5 j’=5.5 j’=6.5

[o] [o] [o]

[o] [o] [o]

[Å2]

[Å2][Å2] [Å2]

[Å2][Å2]

Parity breaking: p’ = - p = 1, DCSs

Page 31: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

j’=7.5 j’=8.5 j’=9.5

j’=10.5 j’=11.5 j’=12.5

[o] [o] [o]

[o] [o] [o]

Parity breaking: p’ = - p = 1, DCSs

[Å2]

[Å2][Å2] [Å2]

[Å2][Å2]

Page 32: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Recall that the Quasi Quantum Treatment yields the following propensity rule depending on the parity

These parity-pairs of similar DCSs are seen in experimental results, the ratios within the pairs can be verified using HIBRIDON results.

Parity Effects

p’ = p = - 1

p’ = p = - 1

p’ = - p = 1

Page 33: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

The ratios between differential cross sections within parity pairs, is close to what the Quasi- Quantmum Treatment (QQT) predics.

For large j the agreement becomes worse.

Parity Effects

Page 34: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Conclusions and Outlook

1. Quasi quantum mechanical treatment that eliniminates l and l’ appears to be feasible for inelastic scattering.

2. The oscillatory dependence of S upon j’ can be explained as a quantum interference that invokes the repulsive part of the anisotropic potential.

3. An interference induced propensity rule of the DCS follows from our treatment and is seen experimentally. A physical interpretation of the DCSs emerges.

4. Measurements of orientation dependence of the DCSs will be attempted.

5. Is it possible to invert oriented DCSs to PESs?

Page 35: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Questions?

j’ = 4.5, R21

Page 36: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

velocity mapping

ions

Extractor MCP's

+

Molecules in a certain rotational state (after collision) are ionized using 1+1’ REMPI and the ions are projected onto the detector, providing a 2D velocity distribution.

+

+

+

+repellor

Page 37: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

velocity mapping

The velocity distribution is recorded with a CCD camera. Ion images show the angular dependence of the inelastic collision cross sections of scattered NO (j’, ’, ’) molecules.

Page 38: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

Voltages: Vrepellor = 730 VVextractor = 500 V

Sensitivity: S = 7.7 m/s / pixel

NO beam velocity: vNO = 590 +/- 25 m/s He beam velocity: vHe = 1760 +/- 50 m/s

Images are: - 80 x 80 pixels- averaged over 2000 laser shots (@ 10 Hz)

Some parameters

Forward scattering ( = 0): Backward scattering ( = ):

vNO

vHe

Page 39: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

DCS extraction

Extraction of differential cross sections (dcs’s) fromimages:

1. Calculate the center(pixel) of the scattering circle2. use intensity on an outer ring of the image as trial dcs

3. Use the trial dcs to simulate an image4. Improve the dcs, minimizing the difference between

simulated and measured image

Step 3 and 4 are repeated until the simulated an measured images correspond well enough.

Page 40: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

NO-He, P11 (’=1/2, ’=1)

12-03-2004

j’ = 1.5 j’ = 2.5 j’ = 3.5 j’ = 4.5 j’ = 5.5 j’ = 6.5

j’ = 7.5 j’ = 8.5 j’ = 9.5 j’ = 10.5 j’ = 11.5 j’ = 12.5

Page 41: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

j’ = 1.5 j’ = 2.5 j’ = 3.5 j’ = 4.5 j’ = 5.5 j’ = 6.5

j’ = 7.5 j’ = 8.5 j’ = 9.5 j’ = 10.5 j’ = 11.5 j’ = 12.5

12-03-2004

NO-He R21 (’=1/2, ’=-1)

Page 42: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

NO-He R11 Q21 (’=1/2, ’=1)

15-03-2004

j’ = 1.5 j’ = 2.5 j’ = 3.5 j’ = 4.5 j’ = 5.5 j’ = 6.5

j’ = 7.5 j’ = 8.5 j’ = 9.5 j’ = 10.5 j’ = 11.5 j’ = 12.5

Page 43: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

NO-He Q11 P21 (’=1/2, ’=-1)

17-03-2004

j’ = 1.5 j’ = 2..5 j’ = 3.5 j’ = 4.5 j’ = 5.5 j’ = 6.5

j’ = 7.5 j’ = 8.5 j’ = 9.5 j’ = 10.5 j’ = 11.5 j’ = 12.5

Page 44: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

NO-He P12 (’=3/2, ’=1)

15-03-2004

j’ = 1.5 j’ = 2..5 j’ = 3.5 j’ = 4.5 j’ = 5.5 j’ = 6.5

j’ = 7.5 j’ = 8.5 j’ = 9.5 j’ = 10.5 j’ = 11.5 j’ = 12.5

Page 45: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

NO-He R22 (’=3/2, ’=-1)

15-03-2004

j’ = 1.5 j’ = 2..5 j’ = 3.5 j’ = 4.5 j’ = 5.5 j’ = 6.5

j’ = 7.5 j’ = 8.5 j’ = 9.5 j’ = 10.5 j’ = 11.5 j’ = 12.5

Page 46: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

NO-He P22 Q12 (’=3/2, ’=-1)

15-03-2004

j’ = 1.5 j’ = 2..5 j’ = 3.5 j’ = 4.5 j’ = 5.5 j’ = 6.5

j’ = 7.5 j’ = 8.5 j’ = 9.5 j’ = 10.5 j’ = 11.5 j’ = 12.5

Page 47: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

NO-He Q22 R12 (’=3/2, ’=1)

j’ = 1.5 j’ = 2..5 j’ = 3.5 j’ = 4.5 j’ = 5.5 j’ = 6.5

j’ = 7.5 j’ = 8.5 j’ = 9.5 j’ = 10.5 j’ = 11.5 j’ = 12.5

15-03-2004

Page 48: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

R21

Page 49: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

R21

Page 50: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

P11

Page 51: Quantum Interference as the Source of Stereo-Dynamic Effects in NO-Rare Gas Scattering A. Gijsbertsen, C.A. Taatjes *, D.W. Chandler *, H.V. Linnartz and.

P11


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