Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present...

55
Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan. 3. The First Experiment. 4. Future Plan.

Transcript of Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present...

Page 1: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Background and Present Status from AMO Instrument Team

1. Team Organization.

2. Proposed Scientific Plan.

3. The First Experiment.

4. Future Plan.

Page 2: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Historical Facts• April 2004: LCLS puts out a call for Letters of Intent

(LOI)category A: science & end-station constructioncategory B: sciencecategory C: instrument design

• July 2004: LCLS SAC makes recommendation that two AMO proposals of the “category A LOI” collaborative teams merge

• October 2004: Ultra-fast science workshop

Page 3: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

October 2004: Ultra-fast science workshop►Workshop Objective:solicit input & participation from the AMOP community for the LCLS project- shape the scientific program: Scientists ideas- help define the critical XFEL machine parameters- help define the designs of an AMOP end-station(s)- interaction of the five collaborative teams

► Five LCLS collaborative teams:- Atomic, Molecular & Optical Science - Optical pump x-ray probe studies in chemistry,

biology & material science- Diffraction imaging of single objects approaching

atomic scale resolution- Coherent x-ray scattering for the study of dynamics- High-energy density science

Page 4: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

AMO Collaborative Team ( Original Merged LOIs A)Marriage of Synchrotrons + Ultrafast Communities

Lou DiMauro (OSU) & Nora Berrah (WMU) (co-T. Leaders)John Bozek (Instrument Scientist)

Pierre Agostini OSU Musahid Ahmed LBLJohn Bozek LBL Philip H. Bucksbaum SU/SLACRoy Clarke UM Todd Ditmire UT AustinPaul Fuoss ANL Ernie Glover LBLChris Greene U Colorado Elliot Kantor ANLBertold Kraessig ANL Steve Leone UC BerkeleyDan Neumark UC Berkeley Gerhard Paulus Texas A&MSteve Pratt ANL Alexei Sokolov Texas A&MJohn Reading Texas A&M David Reis UMSteve Southworth ANL Linn Van Woerkom OSULinda Young ANL

~ Twenty Additional Scientists Expressed Interest at the October 2004 Workshop

Page 5: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Update on AMO Organization/Activities

1. Instrument Scientist, John Bozek, Hired (Jan 2006)2. Regular Teleconference (Berrah, Bozek, DiMauro, Young)

3. N. Berrah on Sabbatical FY06 4. Periodic visits by DiMauro/Berrah5. Communication with Broader Team at Conferences

(Wisconsin W. 8/04; DOE M. 9/05; DAMOP 5/06)

6. E-mail Updates to Broader Team when Necessary (seek input, communicate news)

Discussions/communication led to determine the instrumentation needs for first experiments!

7. Conceptual Design and Instrument Budget was submitted and Accepted by LCLS.

Page 6: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Update on AMO Activities/ Organization (cont..)

8. Synergy between the PULSE Center and AMOS

9. Workshop to Stimulate Theory (ITAMP 06-06)

10. Met with:-----LCLS Optics Group------Pump-Probe Team to Explore Common

Interest and will Continue to Meet.

11. Plan to Meet with Imaging Group to Explore Shared Experimental System?

12. Held Ultrafast x-ray Summer School June 2007

Page 7: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Team Major Scientific Thrusts:

•Multiphoton and High-Field X-Ray Processes in Atoms, Molecules, Clusters,& Biological Molecules.

•Time-Resolved Phenomena in Atoms, Molecules (bio-molecules) and Clusters using Ultrafast X-Rays

Page 8: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

AMO LOIs Collaborative Team

Science:1. Multiple core excitation in atoms, molecules and clusters 2. Timing experiments: Inner-shell side band experiments

Photoionization of aligned moleculesTemporal evolution of state-prepared systems

3. Nonlinear physics4. Ion (positive/negative) studies5. Pump-probe, X-X or X-laser or X-e6. Raman processes7. Cluster dynamics (Diffraction of size-selected clusters)8. Photoionization dynamics of biomolecules

Page 9: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Ken Taylor (Ireland) Possibilities for few- and many-electron atoms & ions in XFEL pulses

David Reis (UM) Synchronization issues for pump-probe experiments at LCLS

Robin Santra (ITAMP) Cluster physics at high photon energiesAnders Nielsson (SSRL) Time resolved spectroscopy for studies in surface

chemistry and electron driven processes in aqueous systems

Chris Greene (UCB) Multiphoton ionization processes in free atoms and clusters

John Bozek (ALS, LBNL) Atoms, molecules, clusters and their ions studied with two or more Photons

Ali Belkacem (LBNL) Inner-shell ionization and de-excitation pathways of laser-dressed atoms and molecules

Keith Nelson (MIT) Give him 10 minutes max and then let's get back to reality

Ernie Glover (LBNL) X-ray/optical wave mixingElliott Kanter (ANL) Hollow neon atoms

Science discussed at 2004 October AMOS forum

Page 10: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

LCLS Characteristics• The LCLS beam intensity (~1013 x-rays/200 fs) is greater

than the current 3rd generation sources (104 x-rays/100 ps).

• Extreme focusing (KB pairs) leads to intensity ~1035

photons/s/cm2 (~ 1020 W/cm2 for 800 eV x- rays)

• Nonlinear and strong-field effects are expected when the LCLS beam is focused to a spot diameter of 1μm.

• BUT, electron’s ponderomotive (quiver motion) important at low frequencies IS negligible in the x-ray regime (λ2).

Page 11: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

AMOS AMOS Inst.TeamInst.Team ShortShort--Long Range Plans:Long Range Plans:

High Field: Using the extremely high brightness of the LCLS we propose to study:

→multiple ionization atoms & simple molecules with angle-resolved spectroscopy and ion imaging to understand basic phenomena in highly excited matter

→High-field photoionization in clusters (of various types)

→Low density ionic targets: atoms, molecules, fragments, clusters, biomolecules by photoelectron and ion imaging techniques

Time-Resolved: Temporal resolution will be used to perform:

→Inner-shell photoelectron spectroscopy of molecules (pump-probe using lasers) into specific states.

→Inner-shell photoelectron imaging of isolated biomolecules to follow their chemistry in natural time scale

Page 12: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Double K Vacancy in Gas-Phase Systems → Possible Consequences

• The decay of the KK-vacancy state will produce higher charge states

• This process → extensive fragmentation in molecules

• This process → damage consideration in experiments on Bio-molecules?

Page 13: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

LCLS High Field Beam will Probe:

Photodetachment(or Ionization)

Auger Decay

Sequential(or “Cascade”)

Multi-Auger DecayAuger Decay

SimultaneousDouble-Auger Decay(≈ 3-10% of single Auger)

Page 14: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

High Field Studies in Atoms

Some Examples

Page 15: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

X-Ray Strong Field Experimentx-ray multiphoton ionization

photoionization

Auger

2-photon, 2-electron

sequential

correlated ionization

Page 16: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Low-Frequency Physics → High Frequency

- Ip

1015 W/cm2

- Ip

1013 W/cm2

- Ip 10x20 W/cm2

• Keldysh parameter γ <<1• Tunnel / over the barrier

ionisation• Ponderomotive energy 10

– 100 eV

• Keldysh parameter γ >>1• Multi-photon ionisation• Ponderomotive energy

10 meV

IR:Low frequency regime

VUV FEL:Intense photon source

XFEL FEL:Highly ionizing source

• Angstrom wavelength• Direct multiphoton

ionisation• Secondary processes

γ ≡ Optical Frequency = (Ip/2Up)1/2 ∝ λ-1; Up=I/4ω2 (au)Tunneling Frequency

Page 17: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Intensity , Wavelength and PonderomotiveEnergy (Lambropoulos)

1.2 10-6

4.8 10-6

1. 10-5

7.7 10-5

3.1 10-4

1.2 10-3

4.9 10-3

1.9 10-2

7.9 10-2

0.31

1.27

Up (eV)

8.4 10 21

1.1 1021

1.3 1020

1.6 1019

2.1 1018

2.6 1017

3.2 1016

4.0 1015

5.0 1014

6.3 1013

7.8 1012

I (Up≈ ћω ) W/cm2

10241.2

5122.4

2564.9

1289.7

6419.4

3238.8

1677.6

8155.2

4310.5

2621

11242

ћω (eV)λ (nm)

Page 18: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Theory Available! Calculate the rate of production of highly charged Xei+ ions produced by direct multiphoton absorption, to compare with experiment.

PRL 94, 023001 (2005)

FLASH Experiments

Page 19: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

TOF Spectrum for Atomic Xenon Multiphoton Ionization (Wabnitz et al.’05 )

Page 20: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Wabnitz et al. ‘05

Page 21: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

First LCLS Experiment: K-Shell in Ne

1. Photoionization2. Auger Decay3. Sequential Multiphoton Ionization4. Direct Multiphoton Ionization

Theory:Double-K ionization in Ne due to absorption of 2-photons by 1 atom for hγ>932 eV is predicted to be 100%

LCLS

Page 22: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

The probability of two-photon absorption by 1s2 -shell accompanied by the creation of double 1s-vacancies predominatesover the probability of the process of two-photon one-electron excitation/ionization of the 1s2 shell in the range of x-ray photon energies ≥930 eV.

2 e-out

1e-out

Ne K-edge ~ 870 eV

Page 23: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Ne Charge State vs IntensityRohringer & Santra, PRA 76, 033416 (2007)

@1050 eV

Page 24: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Probable Ne Charge State with hv

Rohringer & Santra, PRA 76, 033416 (2007)

@1μm beamsize

Page 25: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Power of TOFs:Inner-Shell Resonances in Ar; 2 p Excitation to Rydberg States(ALS)

LCLS: K-Shell ArHow would the ratio of Doubly Ionized Ions (Auger decay) Compares to Singly Ionized Ions due to spectator Auger decay?

Resonant shake-off of two electrons.

Page 26: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

High Field Studies in Molecules

Page 27: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Resonant Auger Electron Spectroscopy

• Interesting in molecules too – CO resonant Auger:

Page 28: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Probe Auger(2+)/Spectator Auger(1+) Decay & Fragmentation Pathways

Spectator Auger

Page 29: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

LCLS: HBr, Br2 2p & 2s Ionization

HBr 3d (ALS) Excitation/Ionization2D Map; Angle-Resolved;e- TOFs

Page 30: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Ion Imaging : Fragmentation Decay Channels of CO22+ Subsequent to K-

Shell Photoionization and Auger Decay of CO2.

Identify different fragmentation mechanisms

Page 31: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Fragment Momentum Correlation Plots: Fragmentation Decay Channels of CO2

2+ Subsequent to K-shell Photoionization and Auger Decay of CO2.

Page 32: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

High Field Studies in Clusters

Page 33: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Cluster Studies at FLASH in Hamburg

Page 34: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Cluster Studies, FLASH

200 400 600 800

2*1010

Xe+

8*1010

Inte

nsity

(arb

. uni

ts)

T im e of flight (ns)

6*1011

Xe2+

6*1012

3

54

PFEL=2.5*1013

W /cm 2

876

Tpuls=50 fsλFEL=98 nm

Unusually high energy absorption in clusterFragmentation starting at 1011 W/cm2

Wabnitz et al, Nature 420, 482 (2002)

Xenon Cluster size 2500 atoms

Page 35: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Molecular dynamics simulations indicatethat standard collisional heating cannot fully account for the strong energy absorption.

Page 36: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

hν=37.8 eV, <N>~100, I=3x1013W/cm2 @25 fs

In contrast with earlier studies in IR and VUV spectral regime, we find NO evidence for electron emission from plasma heating processes; Multistepionization process is dominant

Page 37: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Proposed at LCLS: Ion, e-, and Scattering Experiments on Clusters

• Study the Dynamics of Cluster Explosion as a Function of Cluster Size, Wavelengths, Intensity:

Is it a Coulomb Explosion Picture (as in intense optical or near IR ultrafast laser pulses) OR

Explosion due to Hot Nanoplasma (multiple scattering from the cluster atoms can confine electrons yielding a nanoplasma); Explosion Time can be Different

OR, New mechanisms??

• Will Collective Electron Effects be important as in the dynamics of IR irradiated large clusters?

Page 38: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

4d Photoelectron Spectrum of Xe Clusters at hν=135 eVn1

Page 39: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Slide 38

n1 berrah, 6/3/2008

Page 40: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Velocity Map Imaging Coincidence System (PEPIPICO) @ ALS

Electron Detection Ion Detection

80 mm position-sensitive multi-hit hex-anode detector (Roentdek)

Rolles et al. Nucl. Instr. and Meth. B 261, 170 (2007).

Page 41: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Fragmentation of Rare Gas Clusters @ ALS

Page 42: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

PEPIPICO coincidence map for photoionizationat hv=216 eV

n2

Page 43: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Slide 41

n2 berrah, 6/3/2008

Page 44: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

High Field Studies in Ions

Page 45: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Movable Ion-Photon Beamline for ions & size-selected clusters

Size Selected Production Size and Charge Selected Detection

Absolute cross sections: measurements of overlaps, photon & ion fluxes and detector efficiencies.

Page 46: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

High Charge State Formation Following 2p Photodetachment of S- (ALS)

Li3+/Li2+<1%LCLS: S K-shell

S2+/S+∼ 60%

Th, Sim-Auger Int, K-Out H, S-Off; S-Up+Seq-Aug

PR A 72, 050701(R), 05

Page 47: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Ion StudiesIon Studies: : Measure electron spectra of ionic species–

Si-→S+

•Si+

•Si2+

Si3+

Page 48: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Photoionization Dynamics of Clusters or Biomolecules

Biomolecules injected via electrospray

Page 49: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Time-Resolved Studies of Molecules

Pump-probe experiments of molecules (state-selected):- Launch a molecule on a particular potentially energy surface- Watch temporal evolution with angle-resolved inner-shell PES

Page 50: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Photodissociation Dynamics of I2-: Pump-Probe Experiments

•Short delay times photodetachmentaccesses bound vibrational levelsof I2 states

•Longer times,dissociation to I- + I

•Complete dissociation≡ photodetaching free I-

LCLS, Probe with >800 eVphotons

I2

I2-

Page 51: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Photodissociation Dynamics of I2-

I- photoelectron spectrum

2P1/2 and 2P3/2 spin-orbit states of I.

Neumark et al. Chem. Phys. Lett, 258 (1996) 523.

Page 52: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Photodissociation Dynamics of I2-

Dissociation Time scale: Rise time of electron signal reaches 50% of its maximum value by 100 fs.

I 2P3/2

I 2P1/2

Page 53: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

END

Page 54: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Molecular Fragmentation: Ion Momentum Imaging of Molecules (ALS)

Page 55: Background and Present Status from AMO Instrument Team · 2010. 3. 2. · Background and Present Status from AMO Instrument Team 1. Team Organization. 2. Proposed Scientific Plan.

Photodissociation Dynamics of I2-

Kolsoff et al.