DAC Center at NSLS Q. Z. Guo (X17B3) Jingzhu Hu (X17C) Z. X. Liu (U2A) R. J. Hemley (IR...
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Transcript of DAC Center at NSLS Q. Z. Guo (X17B3) Jingzhu Hu (X17C) Z. X. Liu (U2A) R. J. Hemley (IR...
![Page 1: DAC Center at NSLS Q. Z. Guo (X17B3) Jingzhu Hu (X17C) Z. X. Liu (U2A) R. J. Hemley (IR spokesperson) H. K. Mao (Xray spokesperson) Geophysical Laboratory,](https://reader034.fdocuments.us/reader034/viewer/2022051216/5697bfba1a28abf838ca065f/html5/thumbnails/1.jpg)
DAC Center at NSLS
Q. Z. Guo (X17B3)Jingzhu Hu (X17C)
Z. X. Liu (U2A)R. J. Hemley (IR spokesperson)H. K. Mao (Xray spokesperson)
Geophysical Laboratory, Carnegie Institution of Washington
COnsortium for Materials Properties Research in Earth Sciences
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IR
X-RAY
U2A
X17BX17C
DAC Center at NSLS
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X17B3 beam line•On-line laser-heating•Cryogenic conditions•EDXD•ADXD•Microbeam < 10 microns•100 days/year beam time
X17C beam line•EDXD•ADXD•<10 microns white beam•Sagittal Laue focusing mono •200 days/year beam time
U2A beam line•Cryogenic conditions•Diffraction limited IR microscopy•On-line Raman•200 days/year beam time
On-site laboratory•Ruby P-calibration•Portable on-line Raman•Sample prep•Cryogenic gas loading•Supporting all HP beamlines
Capabilities
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X17 Superconducting Wiggler White Beam Flux
10000 1000 100 10 1108
109
1010
1011
1012
1013
1014
1015
1016
1017
1018
1019
2000K Black Body
U4IR
NSLS U2B Mk.2 40 mrads hor40 mrads vert.
NSLS U2B 12 mrads hor8 mrads vert.
Phot
ons/s
ec/0
.1%
bw/m
m2 sr
Wavelength (microns)
ALS Superbend
NSLS X17
HPCAT BM 2002
HPCAT BM 2005
HPCAT ID 2002
HPCAT ID 2005IR Brilliance
X-RayBrilliance
Xray Spectroscopy
Time Resolved XRD
Xray Diffraction Amorphous
Single-crystal XRD
NSLS has a very bright
future in the next decade
![Page 5: DAC Center at NSLS Q. Z. Guo (X17B3) Jingzhu Hu (X17C) Z. X. Liu (U2A) R. J. Hemley (IR spokesperson) H. K. Mao (Xray spokesperson) Geophysical Laboratory,](https://reader034.fdocuments.us/reader034/viewer/2022051216/5697bfba1a28abf838ca065f/html5/thumbnails/5.jpg)
•Dedicated high-pressure XRD beamline•Dedicated high-pressure IR beamline•Integration of XRD and laser-heating high P-T •Double-sided laser heating•Resistive heating and XRD above 100 GPa-1000 K•Integration of HP XRD, IR, on-line Raman at cryogenic T•Side diffraction for HP elasticity tensor and rheology•Single crystal diffraction above 20 GPa (to 60 GPa)•XRD of nanometer-size single crystal•XRD of amorphous structure at high P•Pressure calibration based on volume and elasticity
Firsts
![Page 6: DAC Center at NSLS Q. Z. Guo (X17B3) Jingzhu Hu (X17C) Z. X. Liu (U2A) R. J. Hemley (IR spokesperson) H. K. Mao (Xray spokesperson) Geophysical Laboratory,](https://reader034.fdocuments.us/reader034/viewer/2022051216/5697bfba1a28abf838ca065f/html5/thumbnails/6.jpg)
•Dedicated high-pressure XRD beamlines•Dedicated high-pressure IR beamline•Integration of XRD, IR, on-line Raman at HP, Hi-Lo T•Axial XRD for EOS and phase transition studies•Radial XRD for HP elasticity tensor and rheology•Micrometer to nanometer mineralogy with single-xl XRD•Brightest high-energy white x-ray in the U.S.•500 day/yr beam time for COMPRES •Lowest cost (needs $1200/day b.t.), 1/4 of other facilities•Most productive HP geoscience facility in the world
Unique & Routine Operations
But unsustainable at the current funding of $660/day b.t.
![Page 7: DAC Center at NSLS Q. Z. Guo (X17B3) Jingzhu Hu (X17C) Z. X. Liu (U2A) R. J. Hemley (IR spokesperson) H. K. Mao (Xray spokesperson) Geophysical Laboratory,](https://reader034.fdocuments.us/reader034/viewer/2022051216/5697bfba1a28abf838ca065f/html5/thumbnails/7.jpg)
Xie et al, GCA 2002
Chen et al, PNAS 2003
New mineral, Tuite, in shocked meteoriteTwo new minerals, HP forms of chromite, discovered in shocked meteorite & synthesized in DAC
Thin chromite (presumed) precipitates in olivine from garnet peridotite.
Green, PNAS 2003
Ultrahigh-pressure metamorphism and meteorite impact metamorphism
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New Lunar Mineral, HapkiteAnand et al, PNAS 2004
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Rapid growth of superhard single-crystal Diamond by Homoepitaxial CVD method[Yan, et al, 2004]
1 6 .2 m m
CVD homoepitaxial growth
1 .6 m m
seed
1 0 .7 m m
9 °
B
G
B
2 .8 m mA
1 2 .1 m mH
XRD, IR, Raman, and laser heating with 10 carat moissanite anivl cell[Xu, et al, 2004]
CVD diamond anvils reaching 230 GPa[Mao, et al, 2004]
Big MAC and CVD DAC
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- ANOMALOUS TRANSITIONS
IN ICE VIII
100 200 300 400 500
6.51
4.71
2.08
0.14
1.48
2.83
4.12
6.18
7.98 GPa
D2O 85 K
Abso
rban
ce (a
rb. u
nit)
Wavenumber (cm-1) 0 2 4 6 8150
200
250
300
350
400
450D
2O 85K
decompression
compression
Wav
enum
ber (
cm-1
)
Pressure (GPa)
Pressure dependence of IR translational and rotational mode frequencies in D2O No transition
[Klug et al., Phys. Rev. Lett., 2004 submitted]
A WEALTH OF FINDINGS:A WEALTH OF FINDINGS: HP IR studies
?
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HP IR study of Amphibole
Group from Dip. Scienze della Terra, Università di Chieti, Chieti Scalo (2004)
3600 3700 3800 3900
Na(Li0.8
Na0.2
Mg)Mg5Si
8O
22(OH)
2
20.8 GPa
18.315.613.512.310.89.48
7.946.665.813.942.931.671.000.33
1 atm
0.2
Ab
sorb
ance
Wavenumber (cm-1)
Unpublished work, do not circulate
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HP hydrogen bond symmetrization in methane clathrate
0 5 10 15 20 25 30 35
2700
2800
2900
3000
3100
3200
3300
3400
3500
3600
3700
3800
solid symbols 10 Kopen symbols 300 K
Methane-III Clathrate Hydrate (98.3% D
2O + 1.7 % H
2O)
Wav
enu
mb
er (
cm-1)
Pressure (GPa)
2500 3000 3500 4000
10 K
3.59
5.73
8.58
13.2
16.3
19.2
22.124.6
29.5 GPa
Methane-III Clathrate Hydrate (98.3% D
2O + 1.7 % H
2O)
0.5
Ab
sorb
ance
Wavenumber (cm-1)
Klug et al June 2004; unpublished work, do not circulate
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Original PRT MembersEarl Skelton- -- NRL
Dave Schiferl -- LANLJagan Akella -- LLNLPaul McMillan -- ASU
Funding SourcesNSF-EARNSF-DMRDOE-DPDOE-BES
NASANavy
Carnegie
Beamline DevelopmentTom Duffy
Guoyin ShenYanzhang Ma
Maddury SomayazuluMichael Hanfland
Ming Li
Technical HelpLarry CarrPeter Eng
Larry FingerAlexander Goncharov
Gwyn Williams Yan Wu
Mark RiversUsers
Acknowledgments