Bulletin of the American Physical Society
2024 APS March Meeting
Monday–Friday, March 4–8, 2024; Minneapolis & Virtual
Session G20: Matter at Extreme Conditions: High-pressure Superconductivity II and Quantum PhenomenaFocus Session
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Sponsoring Units: GCCM DCOMP DMP Chair: Lewis Conway, Univ of Cambridge Room: M101ABC |
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Tuesday, March 5, 2024 11:30AM - 12:06PM |
G20.00001: Novel Hydride Superconductors Under High Pressure Invited Speaker: Xiaoli Huang Room-temperature superconductors have long been the ultimate goal of scientists. Superhydrides exhibit abundant crystal structures and electronic structures under high pressure. They are the forefront of physics, materials science and superconductivity. Recently, researchers have discovered binary H3S and LaH10 with Tc up to 203 K and 260 K, respectively. In this regard, these findings set a new record for superconductivity, a step closer to room-temperature superconductivity. |
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Tuesday, March 5, 2024 12:06PM - 12:18PM |
G20.00002: High-Pressure Structure, Equation of State, and superconductivity of Bi0.5Sb1.5Te3: Observation of a Novel Bi-Sb-Te Alloy Clayton P Halbert, Nilesh P Salke, Liangzi Deng, Shaowei Song, Xin Shi, Zhifeng Ren, Ching-Wu Chu, Russell J Hemley Post-transition metal and metalloid chalcogenides from A2B3 (A = Sb, Bi, B = S, Se, Te) is a unique family of materials known to show superconductivity and electronic topological transitions at high pressure. These materials are also of interest due to their thermoelectric properties. Bi0.5Sb1.5Te3 from the A2B3 family is found to show superconductivity with Tc of up to ~9 K under pressure. However, its structural and dynamical properties under pressure have not been fully explored. Here, we investigate the structural and dynamics properties of Bi0.5Sb1.5Te3 with x-ray diffraction, Raman spectroscopy, and infrared spectroscopy up to 50 GPa. Structural phase transitions observed by X-ray diffraction are consistent with spectroscopic results measured under pressure. An Electronic topological transition inferred at lower pressure can be correlated with Raman measurements. Notably, above ~25 GPa the Bi0.5Sb1.5Te3 forms a body-centered cubic Bi-Sb-Te alloy with a superconducting Tc near 9 K. Other compounds within the A2B3 family are reported to have high-pressure phases with different identified symmetries. These discrepancies are discussed using Raman and infrared measurements. |
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Tuesday, March 5, 2024 12:18PM - 12:30PM |
G20.00003: Pressure Induced Superconductivity; How it Relates to Structural Changes in Lithium Isotopes Willis Holle, Julia St. Andre, Mason S Burden, Audrey Glende, Stefano Racioppi, Irenka Saffarian-Deemyad, Eva D Zurek, Shanti Deemyad
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Tuesday, March 5, 2024 12:30PM - 12:42PM |
G20.00004: Phase Sensitive Detection Applied to Superconducting Transport Measurements Alexander C Mark, Nilesh P Salke, Muhtar Ahart, Russell J Hemley Measurements of superconducting transitions in materials under very high pressures (e.g., in diamond anvil cells) can be challenging due to the very small samples involved. Phase sensitive detection methods are used in both electrical resistance and magnetic susceptibility measurements in order to extract signatures of superconductivity (i.e., Tc) in such samples. The background signals in such measurements are often not well understood, leading to controversies in the literature. We present a method of extracting evidence for both zero-resistivity and the Meissner effect in a single electrical measurement for small samples within diamond-anvil cells, in particular, through the observation of a transient inductance at Tc . A framework for differentiating a superconducting transition from instrumental or environmental artifacts is developed and data from superconducting samples that have been well characterized using other techniques along with data for proposed near-ambient superconductivity in the Lu-N-H system. |
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Tuesday, March 5, 2024 12:42PM - 12:54PM |
G20.00005: Pressure Driven Competition between Superconductivity and Charge Density Wave States in BaSbTe2.1S0.9 Mason S Burden, George V Wintriss, Tushar Bhowmick, Zhong-Zhen Luo, Shanti Deemyad, Mercouri G Kanatzidis, Weizhao Cai BaSbTe2.1S0.9 (BSTS) is a newly discovered 2D layered material which exhibits charge density wave (CDW) order under ambient conditions. CDW is a correlated electronic phenomenon in a periodic modulation of charge density of a material. Both CDW and superconductivity are correlated states and often observed in the materials under different conditions. Currently, however, the correlation between the two states is not well understood. Here we present the pressure studies of the magnetic resistivity and XRD analysis of BSTS up to 30 GPa under quasi-hydrostaitc conditions where we show that CDW is suppressed under high pressure and leads to the emergence of superconductivity at around 10 Gpa. Our results support that CDW and superconductivity are competitive electronic states in BSTS. |
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Tuesday, March 5, 2024 12:54PM - 1:06PM |
G20.00006: Electrical Resistance and Magnetic Susceptibility Evidence for Near Ambient Superconductivity in Nitrogen-Doped Lutetium Hydride NILESH P SALKE, Alexander C Mark, Muhtar Ahart, Russell J Hemley The discovery of superconductivity in nitrogen-doped lutetium hydride at near-ambient conditions has attracted significant attention1 but also controversy as many experimental groups report no superconductivity at these conditions in Lu-N-H samples they have synthesized (e.g., Refs. 2-5). We present the electrical resistance6 and magnetic susceptibility measurements on nitrogen-doped lutetium hydride samples that are in very good agreement with both previously reported Tc and its pressure dependence for nitrogen-doped lutetium hydride. We also find that the observation of these very high Tc is highly variable and that some samples, including those that have degraded over time, show no evidence for superconductivity |
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Tuesday, March 5, 2024 1:06PM - 1:18PM |
G20.00007: Structural Phase Transitions in KC8 under High Pressure Husam Farraj, Russell J Hemley, Jordi Cabana, Muhetaer Aihaiti, Hanns-Peter Liermann, Konstantin Glazyrin, Yue Meng KC8 displays intriguing phase transitions under varying pressures, making it an ideal candidate for investigation for possible a novel superconductor under pressure with hydrogen. Our findings provide a robust foundation for a broader exploration of carbon-rich compounds featuring sp3 networks. At ambient conditions, KC8 displays a 2x2 phase. As pressure increases from 2.3 GPa to 21 GPa, phase transitions occur along the a and b axes. At 2.3 GPa, a transition to a square root 3 x square root 3 phase is observed, in line with previous data. At 3.0 GPa, the 2x2 phase disappears, while the square root 3 phase persists until 6 GPa. Between 6 GPa and 21 GPa, new phases emerge, but their identification is pending. At 21 GPa, we observe evidence of changes not only in the a and b axes but also in the c axis. Importantly, the compressibility of the c axis, from ambient conditions up to the point just before these transitions, aligns with previously reported data. We have utilized Raman and IR spectroscopy to investigate the incorporation of hydrogen into KC8. |
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Tuesday, March 5, 2024 1:18PM - 1:30PM |
G20.00008: Pressure-dependence of the Colossal Magnetoresistance of Europium Cadmium Phosphate (EuCd2P2) ANUKRITI GHIMIRE, Shaun McKeller, Audrey Glende, Mason S Burden, Shanti Deemyad
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Tuesday, March 5, 2024 1:30PM - 1:42PM |
G20.00009: Exploring Novel Material Properties of Colossal Magnetoresistant Material EuCd2P2 through Transport Measurements at Extreme Conditions Audrey Glende, Tushar Bhowmick, Zoey Brookbanks, Mason S Burden, ANUKRITI GHIMIRE, Willis Holle, Sree Sai Ogeti, Shanti Deemyad Exotic compounds that display novel quantum phenomena are the foundations of technological innovation. EuCd2P2 is a newly discovered strongly correlated electron system which displays colossal magnetoresistance (CMR) as an as-grown crystal despite failing to satisfy the accepted paradigm of archetypal CMR materials (i.e. La0.75Ca0.25MnO3, La0.67Ca0.33MnO3 and other mixed-valence perovskite manganites). Colossal Magnetoresistance is the tendency of a material to experience a dramatic change in electrical resistance as a response to the presence of a magnetic field. This quantum phenomena lends itself to a robust increase in hard disk drive data density. |
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Tuesday, March 5, 2024 1:42PM - 1:54PM |
G20.00010: A simple and accurate extension to the quasiharmonic approximation for the calculation of thermodynamic properties of solids. Alberto Otero de la Roza, Ernesto Blancas, Álvaro Lobato Fernández, Fernando Izquierdo Ruiz, Antonio Marcial Márquez Cruz, José Manuel Recio Muñiz, José Javier Plata Ramos The quasiharmonic approximation (QHA) is the main computational method for the prediction of structural and thermodynamic properties of periodic solids, including their phase stability, at arbitrary temperatures and pressures. In a QHA calculation, the static energy and the harmonic phonon density of states are calculated on a volume grid spanning the region of interest. QHA has had great success in the prediction of material properties which are difficult to measure or inaccessible to experiment. The most important drawback of QHA is that, at temperatures higher than a material- and pressure-dependent validity limit, there is a complete breakdown of the theory with spurious thermodynamic predictions across the board. This is caused by the incorrect description of anharmonicity by QHA via the volume dependence of the harmonic vibrational frequencies. In the past, computationally intensive approaches such as ab initio molecular dynamics (AIMD) have been used to calculate thermodynamic properties beyond the QHA limit. To circumvent the use of complex methods like AIMD, we present in this work a simple and efficient way of extending the validity range of QHA. Our method is based on the combination of three ingredients: i) the calculation of force constants to nth order and the subsequent calculation of effective temperature-dependent second-order force constants using the hiphive method (Eriksson et al., Adv. Theory Simul. 2 (2019) 1800184), ii) Allen's quasiparticle theory (Phys. Rev. B 92 (2015) 064106) that posits the calculation of the anharmonic entropy from temperature-dependent frequencies, and iii) a simple fitting method based on the Debye model to obtain the system's free energy as well as the rest of the thermodynamic properties. The proposed method is conceptually and computationally very simple, with a cost similar to that of plain QHA, and reproduces the QHA results below its validity limit by construction. Therefore, our method retains the accuracy of QHA at low temperature while providing a physically grounded and accurate extension to QHA in the high-temperature limit. The implementation of our new method in the gibbs2 program is described, as well as illustrative examples. |
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Tuesday, March 5, 2024 1:54PM - 2:06PM |
G20.00011: A model-free uncertainty-aware equation of state for gold Lin H Yang, Jim A Gaffney, Philip A Sterne This study introduces an advanced Uncertainty-Aware Equation of State (UEOS) toolkit rooted in the error-in-variables Gaussian process. Our approach deviates from traditional methods by generating a gold EOS table (U790) directly from quantum simulation data, bypassing the need for fitting into conventional EOS models like the Mie-Grüneisen equation. The toolkit meticulously accounts for systematic and model-derived uncertainties originating from quantum simulations and experimental data. These uncertainties are seamlessly integrated using Gaussian operations, including additions and derivatives, to obtain the final free energies, specifically the Gibbs free energy. |
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Tuesday, March 5, 2024 2:06PM - 2:18PM |
G20.00012: Gravitational Wave Signatures of Particle Physics Models with Extended Gauge Symmetries Bartosz Fornal The Standard Model of elementary particles describes remarkably well the physics at the most fundamental scale, but it leaves several questions unanswered: What is the nature of dark matter? What is the origin of the matter-antimatter asymmetry of the Universe? How do neutrinos become massive? Finding answers to those questions requires an understanding of what happened when high energy physics effects were prevalent in the Universe, i.e., a small fraction of a second after the Big Bang. Diving this far back into the Universe's history has become possible thanks to the recent first detection of gravitational waves. A primordial stochastic gravitational wave background, although not yet discovered, is expected to carry information precisely about the very early stages of the evolution of the Universe. Those gravitational waves could have been generated through a variety of processes, including first order phase transitions, cosmic strings, and domain walls. Their expected spectrum is within the reach of upcoming gravitational wave experiments, such as LISA, DECIGO, Big Bang Observer, Cosmic Explorer and Einstein Telescope. I will discuss how to use such signals to probe particle physics theories with extended gauge symmetries broken at high energy scales, otherwise completely inaccessible in conventional particle physics experiments. |
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