The High Pressure Science and Engineering Center meets every Wednesday in the BPB conference room at 11:30 AM. We typically have a scientific talk, reports on students’ attendance of conferences and workshops and general discussions. We welcome anyone interested in learning about high pressure science and about HiPSEC to attend our meetings. Please e-mail firstname.lastname@example.org if you wish to receive the seminar alert.
Wednesday, June 6, 11:30 am, BPB 217
Characterizing strain heterogeneities in polycrystalline quartz deformed under high PT conditions
Rheological studies of rocks and minerals allow researchers to study the grain-scale deformation mechanisms that govern large-scale geologic processes from mountain building to mantle mixing. Deforming rock samples with high pressure and temperature apparatuses similar to the Griggs piston cylinder apparatus allows us to simulate deformation at depth. However, many apparatuses are limited to “cook-and-look” analysis and require modeling techniques to determine the evolution of deformation patterns found in experimental samples. A previous study used two-dimensional (2D) plane strain finite element (FE) models to analyze the development of stress patterns in polycrystalline rocks. The study suggested rhythmic patterns in deformed rocks develop as a result of stress percolating through the elastically and plastically disordered system. 2D plane strain simulations are a convenient tool for modeling the long-range stress patterns of rocks because they do not require the processing power of a supercomputer. This study will assess the utility of the method by comparing the micro strain patterns of experimentally deformed samples with strain patterns in 2D FE models. Experimental micro strain will be measured using digital image correlation (DIC) of the sample before and after deformation. Electron channeling contrast imaging (ECCI) in conjunction with electron backscattered diffraction (EBSD) will be used to image and characterize plastic deformation in the sample using a field emission scanning electron microscope (FE-SEM). The 2D plane strain geometry of the FE models will be recreated experimentally by deforming slabs of polycrystalline quartz secured between two alumina half-cylinders in a Griggs apparatus. Optimal models with exact grain orientations and grain boundaries of the starting material will be generated using EBSD crystallographic orientation maps. This study can provide experimental evidence of stress percolation and help quantify the influence of grain-scale mechanisms and grain interaction on the bulk rheology of earth materials.
Wednesday, May 31, 11:30 am, BPB 217
Advanced synthesis of pHEMA-TiO2 hybrid materials by high-pressure induced polymerization methods and analysis of their optical properties
The specific functional properties of organic-inorganic hybrid materials depend on their microscopic structure as well as the nature of the interface between the organic and inorganic components. Many routes exist to fabricate hybrid materials. One of the most prominent is the incorporation of inorganic building blocks in organic polymers in order to combine the advantages of organic polymers with those of the inorganic component. The development of applications for these hybrid materials is often limited by their mechanical behavior. While an increase of the inorganic component concentration can improve the hybrid’s functional properties, it can simultaneously leads to a degradation of the mechanical properties by limiting the extent of the polymer network.
In this presentation I will discuss a new high pressure (HP) approach for the fabrication of nanoparticulate pHEMA-TiO2 (pHEMA = poly-(2-Hydroxyethyl)methacrylate) hybrid materials with high concentration of inorganic part and stable mechanical properties. First, I will present the spontaneous polymerization of HEMA under static pressure (up to 1.6 GPa). I will also show that HP-induced polymerization can be considerably accelerated if laser irradiation (488 or 355nm) is applied. Second, I will discuss a new high pressure rump (HPR) process originally developed for the super-fast polymerization of HEMA and later successfully applied for the fabrication of organic-inorganic hybrid materials. Finally, I will speak about optical properties of pHEMA-TiO2 hybrid materials synthesized by HPR process, studied by pump-probe photodarkening experiments.
Wednesday, May 24, 11:30 am, BPB 217
Molecular dynamics simulations of mechanical and dynamical properties of carbon nanomaterials
Molecular dynamics simulation is a classical computer simulation method that describes inter-atomic interactions via empirical potential functions. When applied appropriately, it can handle larger number of atoms than first-principles calculations and is much faster & efficient in providing valuable insights into some novel phenomena. In this presentation, I will briefly discuss some basics of molecular dynamics simulations including its pros and cons. I will then present some examples of using this method to study mechanical properties of nanomaterials and their dynamics. For example, using the famous AIREBO potential, molecular dynamics simulations can be used to predict the critical buckling behavior of carbon nanotubes. Using the same potential, we proposed a self-assembly approach to design an all-carbon core-shell nanostructure, which is the central component of a novel photovoltaic device, experiment results showed that such approach can notably improve the power conversion efficiency due to increased contact between carbon nanotubes and C60 molecues.
Wednesday, May 17, 11:30 am, BPB 217
Looking into the normal state of a High Critical Temperature Superconductor :
High pressure, high magnetic field Fermiology studies of YBCO
Our team’s expertise lies in the measurements of magnetization and Fermi surfaces of strongly correlated electronic systems, under the extreme conditions of high pressures , low temperatures and high magnetic fields . I will describe how those measurements are made, and how those extremes are reached. I will then discuss our most recent data on the archetypal High Temperature Superconductor YBCO.
The pnictide, cuprate and molecular conductor families exhibit similar phase diagrams, leading to a great deal of interest in a common mechanism for a “universal phase diagram”. The typical ingredients for such phase diagrams include an antiferromagnetic phase, a superconducting dome, and possibly one, or several quantum critical points (QCP) [3,4]. The interplay between these various ingredients, in particular the origin of the superconducting dome, has been one of the hottest topics in condensed matter physics for the past 30 years, and is still heavily studied and debated. Chemical doping is one traditional way to look at such materials, however thermodynamic variables such as magnetic field or hydrostatic pressure have proven to be powerful tools to explore this phase diagram, with very strong magnetic fields being used to suppress the superconducting dome, allowing one to investigate the QCP.
Our group performed high pressure Fermi surface measurements (Shubnikov-de Haas effect) of YBCO6.5 (p=0.1) at He-3 temperatures in pulsed fields to 70 T and static fields of 45 T, and pressures of 25 GPa using plastic and metal diamond anvil cells (DACs), respectively. These cells are coupled with an LC tank circuit based on a tunnel diode oscillator. The small coil that makes up the inductor of this LC circuit and resides in the high pressure volume of the DAC senses changes in sample resistivity (or magnetism in insulators) due to variations in temperature, pressure or magnetic field. Our Fermiology studies clearly show a strongly diverging effective mass at 4.5 GPa that is associated with a local maximum in frequency and critical superconducting temperature. The high critical field Hc2 in this material limits our study in the low pressure range to pressures below 7 GPa in the 45 T hybrid magnet, but by increasing pressure to 25 GPa we are able to once again see quantum oscillations and find that the orbital frequency has increased from 550 T at ambient pressure to 690 T. Pulsed field high pressure studies are currently planned to shed light on the region between 7 and 25 GPa. This now allows us to use pressure to develop a B-P-T phase diagram that will permit a more complete picture of HTS to be pursued and answer how CDWs and the pseudogap play a role in superconductivity.
 D. Graf et al., High Pressure Research 31(4), 533 (2011)
 The National High Magnetic Field Laboratory’s website has a lot of tutorials and information about magnetism and magnets. A good introduction to high magnetic fields can be found at :
 S. Badoux, et al., Nature, 531, 210 (2016).
 B. Ramshaw, et al., Science, 348, 317 (2015).
Wednesday, Apr 26, 11:30 am, BPB 217
Calorimetry Study of the Phase Diagrams of EuNi2Ge2 and Eu2Ni3Ge5Under Pressure
Dr. S. Esakki Muthu
In this talk I will present the phase diagrams of EuNi2Ge2 and Eu2Ni3Ge5studied by ac calorimetry under pressure using a diamond anvil cell. In EuNi2Ge2 the antiferromagnetic transition exists up to 1.5 GPa. The sudden disappearance of magnetic order around 2 GPa is confirmed, consistent with the probable occurrence of a first order valence transition near that pressure. The ac calorimetry results on Eu2Ni3Ge5 clearly show 2 antiferromagnetic transitions, and suggest that magnetic order persists up to higher pressure than previously expected. At high pressure, where heavy fermion behavior has previously been reported, the Néel temperature is decreasing, and magnetic order is expected to disappear at an extrapolated pressure of 12-14 GPa. A semi-quantitative analysis of the pressure dependence of the specific heat does not show any large changes, but is compatible with a moderate enhancement of g. The similarities with the phase diagrams of Yb and Ce heavy fermion systems will be discussed.
Wednesday, Apr 19, 11:30 am, BPB 217
Laser annealing after a kinetically hindered phase transition in the pyrochlore La2Sn2O7
There is interest in identifying materials for use in radioactive waste applications and studying their structural properties. Studies has shown that pyrochlore (A2B2O7) compounds might be promising candidates for such purposes. In an attempt to obtain a broader understanding of the structural stability of these compounds, we have investigated the pyrochlore La2Sn2O7 under extreme conditions: high temperature isobaric and high-pressure isothermal study. Both quasi-hydrostatic and non-hydrostatic isothermal high pressure compression runs were undertaken to reveal alternative structural transformations and studied using synchrotron angle-dispersive X-ray diffraction and Raman scattering techniques, supported by ab-initio random structure searching (AIRSS). Compression using He as a quasi-hydrostatic pressure transmitting medium permitted the observation of a new high pressure phase via a kinetically hindered first-order phase transition that begins at 49 GPa and finally goes to completion at 61 GPa. Alternatively, the non-hydrostatic compression, using no pressure-transmitting medium, revealed the emergence of a phase transition at 46 GPa. However, it appears that this process occurs via a stress-induced pathway and in fact transforms into an amorphized phase by 67 GPa. Annealing the amorphized phase, through laser heating, at 70 GPa allows us to crystallize the high-pressure phase which is recoverable to ambient conditions. Our AIRSS calculations reveal three competing metastable structures, close in energy at 70 GPa.
Wednesday, Mar 22, 11:30 am, BPB 217
Unexpected Structural and Electronic Behavior in Sn3N4
Group 14 nitrides have been a topic of recent scientific focus due to their interesting mechanical and electronic properties. My talk will describe our research into the behavior of the nitrogen-rich nitride Sn3N4 under high pressure-temperature conditions. Using in-house experimental optical techniques and in situ X-ray diffraction, coupled with laser heating in the diamond anvil cell we have observed exotic electronic behavior with pressure. The band gap in this optoelectronic material reveals an opening from 0.5 to 3 eV with pressure between 0 and 130 GPa, after which the band gap slowly closes. A component of this talk will be focused on the possible mechanisms for this phenomenon. The structure of Sn3N4 at these extreme pressures (measured up to 230 GPa) has not yet been solved, and I will discuss the methods and difficulties faced in identifying the new phases predicted by ab initio random structure searching (AIRSS).
Wednesday, Mar 15, 11:30 am, BPB 217
Quantum Critical Heavy Fermions
High pressure techniques can be used to tune heavy fermion materials to a quantum critical point. Presented here is the basic theory behind this. The Kondo effect, the Anderson model, the Kondo lattice and the RKKY interaction are discussed qualitatively. Selected publications from experimental work performed at HiPSEC that have demonstrated this as well as potential future work are also discussed.
Wednesday, Mar 1, 11:30 am, BPB 217
Shock Recovery of Bismuth
Between 0 and 10 GPa there are five different bismuth phases. High-pressure bismuth (Bi) phases have been examined in static compression experiments; however, none could be recovered to ambient conditions. Here we report Bi-III recovery (stable above 3 GPa) to ambient conditions from a shock compression experiment to 5.7 GPa. Bi-III was identified by synchrotron micro-diffraction and backscatter electron imaging. Our work shows shock-compression provides a tool for recovering high-pressure phases that otherwise elude decompression. DOE/NV/25946–3140
Wednesday, Feb 8, 11:30 am, BPB 217
Recreating planetary cores in the laboratory
Of the different planets in our solar system, our giant icy neighbors Neptune and Uranus are extremely fascinating, Uranus being the more peculiar of the two. Though Uranus is almost 2 billion kilometers closer to the sun than Neptune, its average surface temperature can dip as low as 50 K, actually making it colder than Neptune. The primary belief for this is that the core of Uranus, which is believed to be made of diamond, silicates, iron, and nickel, has shed most of its energy; cooling down to a point where it no longer radiates much heat. Despite having a cold core, Uranus has a very active and unique magnetic field. Unlike Earth, whose magnetic field is driven by a very hot active core, it is believed that Uranus’s unique magnetic field is actually driven by mixtures of super ionic and metallic molecular compounds. It has been measured that the primary components of its mantle are water, ammonia, and methane, which have all been predicted to show superionic properties at the conditions present within the mantle. There have recently been efforts in attempting to recreate the conditions necessary to verify these predicted phases, primarily in the area of shock compression. This is difficult as the region of P-T space that these superionic phases exist cannot be reached by traditional shock compression. In a traditional shock experiment the path the hugoniot takes overshoots the targeted region due to high amounts of entropy generated, so very high temperatures are reached along with very high pressures. One way around this is by compressing the sample to a specific density prior to shocking in order to take off hugoniot shock paths, reaching the pressures necessary at much lower temperatures. I will discuss some details of how these pre-compressed experiments are performed as well as how Velocity Interferometry for Any Reflector (VISAR) is used to interpret the results.
Wednesday, Jan 18, 11:30 am, BPB 217
Adventures with 5d orbitals at high pressure
Advanced Photon Source, Argonne National Laboratory
While first-row (3d) transition metal (TM) oxides continue to provide a rich playground for studies of electron correlations, recent focus has shifted to third-row (5d) TM oxides in the search for novel quantum states. The sizable spin-orbit interaction in heavy 5d ions, coupled with reduced on-site Coulomb interactions as a result of the large spatial extent of 5d orbitals, create unique experimental and theoretical opportunities for discovery of new electronic phases of matter.
We have studied some of the consequences of enhanced S-O coupling and spatial extent of 5d orbitals on the electronic structure and magnetic (exchange) interactions in a novel “iridate” magnetic insulator, Sr2IrO4. The high-brilliance, penetration power, and polarization/energy tunability of synchrotron radiation enable the use of x-ray absorption spectroscopy (including circular dichroism) and resonant magnetic scattering techniques in the diamond anvil cell providing exquisite sensitivity to the evolution of electronic correlations at high pressure. Among other findings, we discovered that pressure leads to frustration of exchange interactions in the square lattice of entangled spin-orbital Iridium moments and emergence of quantum paramagnetism, possibly a quantum spin liquid phase.
Higher brilliance, 4th generation synchrotron light sources now in development around the globe will bring unprecedented opportunities for studies of electronic/magnetic order at the limit of static high-pressure generation technologies.