Prof. Zheshen Zhang is a Professor in the Department of Electrical and Computer Engineering at the University of Michigan College of Engineering . He leads the Quantum Engineering Lab , focusing on harnessing quantum mechanical resources like entanglement to advance sensing, communication, and computing systems. Academic Rank: Professor Institution: University of Michigan School: College of Engineering Department: Electrical and Computer Engineering Research Interests: His work spans quantum engineering, emphasizing: Quantum computing architectures using continuous-variable cluster states Quantum communication via entanglement-assisted protocols Quantum sensing for precision metrology and dark matter detection Hybrid photonic circuits with Scandium Aluminum Nitride and Silicon Nitride Application of machine learning to quantum information processing Publications Trends: Recent articles highlight: Advances in integrated photonics for scalable quantum devices Development of entanglement-enhanced sensors for covert and precision applications Exploration of exceptional points in optical cavities for metrology Quantum network prototypes enabling open-access quantum computing Machine learning integration with quantum data acquisition
Prof. Dr. Michael Schramm serves as an Extraordinary Professor of Classical Philology at the University of Göttingen's Faculty of Humanities. His academic journey spans prestigious institutions including Heidelberg, Jena, Leipzig, and Bielefeld, with doctoral and habilitation degrees establishing his expertise in ancient philosophical traditions. Research interests center on Neoplatonism, Greek tragedy reception, and Late Antique political-religious dynamics, particularly focusing on Julian the Apostate's theological works and Euripides' influence in imperial philosophy. His publications demonstrate rigorous engagement with textual criticism, philosophical exegesis, and intercultural dialogue between pagan and early Christian thought. Current research includes DFG-funded projects on Julian's religious philosophy (2015-2019) and Euripidean tragedy's relationship to providence (2020-2021), alongside a Gerda Henkel Foundation research fellowship (2020-2021). His editorial leadership in volumes like Euripides-Rezeption in Kaiserzeit und Spätantike (2020) shapes contemporary scholarship in classical reception studies. Advisory roles include postdoctoral mentoring through DFG research groups, with institutional service comprising temporary professorships at Bamberg, Bonn, Tübingen, and Jena since 2012. His methodological approach integrates philological precision with philosophical analysis across monographs, critical editions, and interdisciplinary handbooks.
Wolfgang Lorenzon is a Professor of Physics at the University of Michigan, specializing in experimental particle physics, nuclear physics, and astrophysics. His research spans three major experimental programs: the LUX-ZEPLIN (LZ) dark matter experiment at SURF, the MUSE experiment at PSI for proton radius measurements, and the SpinQuest collaboration at Fermilab studying hadronic physics. He has held significant roles in major collaborations including SeaQuest and HERMES, where he served as Deputy Spokesman from 1997-1998. His educational background includes a Ph.D. (1988) and Diploma (1984), both from the University of Basel. Lorenzon has built a distinguished research career focusing on precision measurements in particle and nuclear physics, with particular expertise in detector development and experimental techniques. Lorenzon's research interests center on fundamental questions in particle physics. His work on the LZ experiment involves developing the in-line radon removal system for the central time-projection chamber, crucial for enhancing the detector's sensitivity to WIMPs. At PSI, he leads the development of liquid hydrogen targets for the MUSE experiment, which aims to resolve discrepancies in proton charge radius measurements. His hadronic physics work with SeaQuest and SpinQuest focuses on understanding nucleon structure through antiquark distributions and polarized Drell-Yan processes. His research bridges theoretical questions with cutting-edge experimental techniques, often requiring innovative detector solutions. Analysis of his recent publications (2023-2025) reveals a strong focus on dark matter detection using liquid xenon technology, precision measurements of nucleon structure, and development of next-generation detectors. His work spans theoretical interpretation of experimental results, detector development, and analysis of fundamental particle interactions. The research shows increasing collaboration across international boundaries, with significant contributions to multiple major experiments simultaneously. Scientific Awards: Fellow of the American Physical Society Lorenzon has mentored numerous graduate students through completion of their Ph.D. degrees, with recent graduates including Haley Reid (2024), Noah Wuerfel and Chami Amarasinghe (2023), Maris Arthurs (2022), Marshall Scott (2020), and Daniel Morton (2019). His current research group includes postdocs, graduate students, and undergraduate researchers. His research is supported by multiple grants from the National Science Foundation (Grant 2110229) and the Department of Energy (Grant SC0019193 and Subcontract 734299), as well as University of Michigan funding. Lorenzon leads a research group with active laboratories at both the Homer A. Neal Laboratory (3265 HANL) and West Hall (357 WH) at the University of Michigan. His team collaborates with international groups at Fermilab, SURF in South Dakota, and the Paul Scherrer Institute in Switzerland. The group maintains strong connections with the LZ collaboration, MUSE experiment, and SpinQuest collaboration, contributing both technical expertise and physics analysis capabilities to these major international efforts.
K.S. Babu, Ph.D. , is a Regents Professor in the Department of Physics at Oklahoma State University . His research focuses on theoretical physics beyond the Standard Model, particularly in neutrino mass models, grand unification, and baryon/lepton number violation. Email: kaladi.babu@okstate.edu Contact: 405-744-5810 | 232 Physical Sciences, OSU Dr. Babu's work spans several key areas: Grand Unified Theories (GUTs): Studies of SO(10), SU(5), and E6 unification frameworks. Neutrino Physics: Development of models like the Zee-Babu mechanism for neutrino masses and research on oscillations. Dark Matter & Cosmology: Proposals for dark matter candidates and connections to inflation and baryogenesis. CP Violation & Leptogenesis: Mechanisms for generating matter-antimatter asymmetry. His recent publications highlight advancements in: Spontaneous CP violation in SO(10) (2025) Left-right symmetric models for leptogenesis (2025) Ultraviolet-completed two-loop neutrino mass models (2025) Probing baryon number violation at IceCube and LHC (2024) Accidental Peccei-Quinn symmetry for axion models (2024) Dr. Babu actively collaborates on international initiatives such as the Center for Theoretical Underground Physics (CETUP) and contributed to the Snowmass 2013 Community Planning Study. His lab has mentored numerous graduate and postdoctoral researchers, including Kirtiman Ghosh, Sudip Jana, and Shaikh Saad.
Reed Essick is an Assistant Professor at the Canadian Institute for Theoretical Astrophysics (CITA), University of Toronto. His research focuses on experimental gravity, astrophysical signals, and nuclear physics, with particular emphasis on neutron stars, black holes, and gravitational waves. He develops advanced statistical methods like hierarchical Bayesian inference and nonparametric analysis for interpreting observational data from pulsars and gravitational wave detectors. Dr. Essick collaborates extensively with international observatories such as LIGO, Virgo, and KAGRA, contributing to cutting-edge projects like multimessenger astronomy and precision cosmology. His work bridges computational astrophysics with observational techniques, addressing fundamental questions about dense matter and strong-field gravity. Key contributions include studies on gravitational wave equation-of-state constraints, pulsar timing analysis, and the application of machine learning to detector data. His research leverages both ground-based interferometers and space-based observations to explore extreme astrophysical environments.
John E. Carlstrom is the Subrahmanyan Chandrasekhar Distinguished Service Professor and Chair of the Departments of Astronomy & Astrophysics and Physics at the University of Chicago. He leads the South Pole Telescope (SPT) project and co-chairs the CMB-S4 collaboration, focusing on observational cosmology and the cosmic microwave background (CMB). His work bridges the University of Chicago with Argonne National Laboratory, the Enrico Fermi Institute, and the Kavli Institute for Cosmological Physics. Education: PhD, University of California, Berkeley (1988) AB, Vassar College Carlstrom’s research centers on using the CMB to study the universe’s origin and evolution, including inflation, dark energy, and neutrino masses. His team employs advanced instruments like the SPTpol and SPT-3G cameras to map CMB polarization and detect galaxy clusters via the Sunyaev-Zeldovich effect. Recent projects include the Event Horizon Telescope’s black hole imaging and NSF-funded CMB-S4 development. Scientific Awards: MacArthur Fellowship (1998) Gruber Prize in Cosmology (2015) Breakthrough Prize in Fundamental Physics (2019) Dannie Heineman Prize for Astrophysics (2024) Arthur L. Kelly Faculty Prize (2024) Elected to AAAS (2000) and NAS (2002) He directs the SPT Group, which collaborates with Argonne National Laboratory on superconducting detector fabrication. His work has shaped major initiatives like the Dark Energy Survey and the Giant Magellan Telescope, influencing the Astro2020 decadal survey. Carlstrom mentors graduate students in physics and astrophysics, advancing precision cosmology through cutting-edge instrumentation.
Carlos Argüelles-Delgado is an Assistant Professor of Physics at Harvard University's Department of Physics within the Faculty of Arts and Sciences. His research focuses on neutrino physics and astroparticle physics, particularly using data from the IceCube Neutrino Observatory. He explores properties of neutrinos, including potential Beyond Standard Model effects, and contributes to the development of the IceCube-Gen2 upgrade. His work includes analyzing high-energy neutrinos, studying cosmic origins, and advancing detector capabilities. Education: Ph.D. in Physics from the University of Wisconsin at Madison (2015), M.Sc. in Physics from Pontificia Universidad Católica del Perú (2012), and B.Sc. in Physics from the same institution (2008). Research Interests: Neutrino oscillations, dark matter annihilation signatures, sterile neutrinos, and astrophysical neutrino flavor measurements. He develops novel analysis techniques, such as Bayesian methods and Monte Carlo simulations, and collaborates on global neutrino data projects. Awards: 2021 Sloan Research Fellow, 2021 IUPAP Young Scientist Prize, and 2020 IceCube Collaboration Impact Award. His contributions include advancing diversity initiatives and software tools for neutrino data analysis. Teaching: Taught Electricity and Magnetism at Harvard, and previously taught physics at the undergraduate and high school levels. Active in outreach, including mentoring students and organizing workshops like the IceDUNE Workshop (2021). Labs/Teams: Leads analyses in the IceCube Collaboration’s Beyond the Standard Model Working Group and participates in the IceCube-Gen2 project. Collaborates with Janet Conrad’s group at MIT and the Wisconsin IceCube Particle Astrophysics Center.
Robert J. Brunner is a Professor at the University of Illinois with primary appointments in the Gies College of Business (Department of Accountancy) and the School of Information Sciences. He holds affiliate roles across multiple departments including Astronomy, Computer Science, and Statistics, as well as research centers like the Beckman Institute and NCSA. His research focuses on applying statistical/machine learning to solve complex problems in astronomy, finance, and large-scale data science. Education: Ph.D. in Astrophysics from Johns Hopkins University (advisor: Alex Szalay). Postdoctoral work at Caltech on the Digital Sky project. Research Interests: Machine learning applications, computational techniques, data management/visualization, and observational cosmology. His work bridges astrophysical data analysis with modern data science methodologies. Recent work includes developing spatio-temporal neural networks for forecasting, evaluating AI-driven financial analysis tools, and planning for the Vera C. Rubin Observatory. He collaborates internationally on large-scale surveys like the Dark Energy Survey and SDSS. Labs/Teams: Leads data science initiatives at the University of Illinois Research Park. Active in interdisciplinary teams at NCSA and Beckman Institute focusing on algorithm optimization and data-intensive research.
Professor Ana Ferreira is a leading seismologist at University College London, focusing on deep Earth structure and earthquake source processes. Her research integrates seismic and geodetic data to understand planetary dynamics from the surface to the lowermost mantle. Her work includes pioneering seismic tomography, such as the SGLOBE-rani 3D anisotropy model, and earthquake source analysis using InSAR and normal mode data. She leads the Seismological Laboratory and teaches Seismology II and Field Geophysics. Recent projects include the UPFLOW experiment, which deployed 49 ocean bottom seismometers in the Atlantic, and studies on Greenland ice sheet evolution and Tonga volcanic eruptions. Her EU-funded research emphasizes multidisciplinary data integration and numerical modeling. Key article trends cover mantle anisotropy, global tomography, earthquake source inversion, cosmology-inspired machine learning, and ocean bottom seismology applications in geodynamics and cryospheric processes.
Prof. G. Scott Watson is a Professor in the Department of Physics at Syracuse University, affiliated with the College of Arts & Sciences. His research focuses on the interplay between fundamental particle physics and cosmology, particularly early universe cosmology, inflationary models, dark matter/energy, and string theory applications. He holds a Ph.D. in Physics from Brown University (2005) and B.S. degrees in Mathematics and Physics from the University of North Carolina at Wilmington (2000). Key research interests include string phenomenology as a quantum gravity framework, probing inflationary scenarios through cosmic microwave background (CMB) studies, and exploring dark matter origins. He leads major projects like CMB-S4 and contributes to the CMBPol mission concept. Watson has received the American Physical Society Outstanding Referee Award (2021) and serves on high-profile collaborations such as the Inflation Probe Study Analysis Group (IPSAG). Teaching responsibilities include advanced courses like Quantum Field Theory, Relativity and Cosmology, and Quantum Mechanics II. He actively mentors students through independent studies and advises on graduate admissions. Watson has secured significant grants, including a Department of Energy-funded project on theoretical particle physics and cosmology (2013–2025) and NSF support for cosmic acceleration research (2018–2023).
Kyle Dawson is a Professor of Physics and Astronomy at the University of Utah, where he has been employed since 2009. He currently serves as both a full Professor and Director of Graduate Studies in the Department of Physics and Astronomy, having progressed from Assistant Professor (2008-2015) to Associate Professor (2015-2019) before achieving his current position in 2019. His institutional affiliation places him within the College of Science at the University of Utah, a major research university in the western United States. Dawson earned his BA in Physics from Cornell University in 1998, followed by a PhD in Physics from the University of California, Berkeley in 2004. After completing his doctoral studies, he served as a postdoctoral researcher at the Lawrence Berkeley National Laboratory before joining the University of Utah faculty. His educational background in physics provided the foundation for his transition into observational cosmology, where he has made significant contributions through large-scale spectroscopic surveys. Professor Dawson's research focuses on observational cosmology through large spectroscopic surveys designed to measure the fundamental properties of the universe. He is currently the co-Spokesperson for the Dark Energy Spectroscopic Instrument (DESI), a major cosmological survey that has produced numerous high-impact publications in 2024-2025. Previously, he served as Principal Investigator for the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), which concluded in 2020 with final cosmological measurements. His work centers on measuring baryon acoustic oscillations to constrain cosmic expansion history, dark energy properties, neutrino masses, and to test General Relativity. His research group employs techniques including galaxy clustering analysis, quasar astrophysics, and large-scale structure mapping to address fundamental questions in cosmology. The analysis of Dawson's recent publications reveals a strong focus on extracting cosmological constraints from the DESI survey data. His work spans multiple aspects of cosmological analysis, including baryon acoustic oscillation measurements, full-shape power spectrum analysis, imaging systematics mitigation, and cross-correlation studies with cosmic microwave background data. The publications demonstrate collaborative work with large international teams and contribute to increasingly precise measurements of cosmological parameters, with particular attention to dark energy equation of state, neutrino masses, and potential deviations from General Relativity. Professor Dawson has secured significant research funding throughout his career, including multiple grants from the Department of Energy (DOE), NASA, and the National Science Foundation. His grant portfolio includes leadership roles in major cosmological surveys like DESI and eBOSS, as well as support for postdoctoral researchers and graduate students. His research group has mentored numerous students who have gone on to successful careers in academia, industry, and data science fields. Dawson leads a vibrant research group at the University of Utah focused on cosmological data analysis from large spectroscopic surveys. His current team includes two postdoctoral researchers (Angela Berti and Sarah Eftekharzadeh) and a graduate student (Allyson Brodzeller). The group specializes in galaxy clustering analysis, quasar astrophysics, and machine learning applications to spectroscopic data. The research environment fosters collaboration with international teams working on DESI and related cosmological surveys, providing students with opportunities to engage with cutting-edge cosmological research and large-scale data analysis techniques.
Dr. Alan Jamison is an Assistant Professor at the University of Waterloo's Institute for Quantum Computing (IQC), located in the Quantum-Nano Centre. His research focuses on ultracold atoms and molecules to study quantum many-body physics and quantum chemistry, enabling precise control of quantum states for applications in quantum computing, sensors, and simulation. He teaches courses such as PHYS 359 (Statistical Mechanics) and PHYS 363 (Intermediate Classical Mechanics), having taught them since 2021. Jamison holds a PhD and MSc from the University of Washington (2014, 2008), and a BS in Mathematics from the University of Central Florida (2007). His accolades include the Henderson Thesis Prize (2015) and the Hans G. Dehmelt Prize (2013). He leads the Jamison Lab, a multidisciplinary team exploring quantum systems' fundamental properties and applications, with current and former students contributing to cutting-edge projects. The lab collaborates across disciplines, including economics, to apply quantum mechanics to diverse fields. Education: PhD Physics, University of Washington, 2014 MSc Physics, University of Washington, 2008 BS Mathematics, University of Central Florida, 2007 Research Interests: Jamison's work spans ultracold chemistry, quantum simulation, and quantum computing. His group uses lasers to cool atoms to near-absolute zero, creating systems to study quantum phenomena like supersolid phases and quantum interference-driven reactions. Recent projects include collisional cooling of molecules and probing spin-orbit coupling in Bose-Einstein condensates. Awards: Henderson Thesis Prize, University of Washington (2015) Hans G. Dehmelt Prize, University of Washington (2013) Mellam Teaching Fellowship, University of Washington (2008) Lab & Team: The Jamison Lab at IQC fosters collaboration across physics, mathematics, and economics. Current graduate students include Omar Hussein and Megan Byres, with undergraduates like Nabeel Rasheed. Former members have pursued roles at institutions like Harvard University and Pratt & Whitney. Labs/Teams: Jamison Lab is part of IQC, a hub for quantum research with faculty from diverse departments. Projects include exploring economic systems through quantum many-body techniques and advancing precision interferometry for quantum sensors.
Emmanuel Fonseca is an Assistant Professor in the Department of Physics and Astronomy at West Virginia University (WVU), joining in Fall 2021. Previously, he was a postdoctoral researcher at McGill University (2016–2021) and completed his Ph.D. in Astronomy at the University of British Columbia (2016). His research focuses on radio astronomy, particularly pulsars and fast radio bursts (FRBs), leveraging facilities like CHIME, the Green Bank Telescope, and NANOGrav. He specializes in using pulsars as laboratories for testing fundamental physics and detecting gravitational waves via pulsar timing arrays. Education: Ph.D. in Astronomy, University of British Columbia (2016) M.Sc. in Astronomy, University of British Columbia (2012) B.Sc. in Physics and Astronomy, Pennsylvania State University (2010) Research Interests: Emmanuel’s work spans three key areas: Compact Objects: Investigating neutron stars and extreme environments using pulsar binaries and relativistic dynamics. CHIME Pulsar/FRB Science: Developing instrumentation and analyzing data from the Canadian Hydrogen Intensity Mapping Experiment to study FRBs and pulsars. Gravitational Waves: Contributing to NANOGrav’s efforts to detect nanohertz gravitational waves via millisecond pulsar timing arrays. Collaborations: He is a core member of NANOGrav and instrumental in maintaining CHIME’s pulsar and FRB backend systems. His work bridges hardware/software development with observational astronomy. Labs/Teams: Involved with the CHIME/FRB Collaboration and the NANOGrav Collaboration, advancing both observational infrastructure and theoretical astrophysics.
Dr. Andreas Kopmann serves as Deputy Director of the Institute for Process Data Processing and Electronics (IPE) at Karlsruhe Institute of Technology (KIT) and leads the Process Data Processing group. With over two decades of experience in experimental physics and data systems, he plays a pivotal role in major international research collaborations including the KATRIN neutrino experiment and PANDA detector project. PhD in Electrical Engineering, University of Hannover (2000) Diploma in Electrical Engineering, University of Hannover (1994) Dr. Kopmann's research focuses on data acquisition systems, trigger systems, real-time monitoring, GPU computing, and data management for large-scale physics experiments. His work bridges experimental physics requirements with advanced computing technologies, particularly in high-data-rate applications for particle physics and synchrotron radiation facilities. He has pioneered novel detector technologies and data processing frameworks that enable cutting-edge scientific discoveries in neutrino physics and accelerator science. Analysis of Dr. Kopmann's recent publications reveals a strong trajectory toward higher data rates, sophisticated real-time processing, and integration of machine learning techniques. His work spans neutrino physics through KATRIN, detector development for PANDA and other experiments, and innovative data acquisition systems like KALYPSO and UFO. The interdisciplinary nature of his research combines particle physics, computing science, and electronics engineering to solve complex experimental challenges. KIT Program Lead for "Matter and Technologies" (2021-present) Coordinator of Helmholtz Program Topic "Detector Technologies and Systems" Principal Investigator in Karlsruhe School for Elementary Particle Physics (KSETA) Project Leader for Data Acquisition in KATRIN experiment As Deputy Director of IPE, Dr. Kopmann oversees research groups developing critical technologies for experiments at KIT, DESY, CERN, and other international facilities. His team's work on high-speed data acquisition, detector electronics, and computing infrastructure supports groundbreaking research in particle physics, neutrino physics, and materials science.
David E. Kaplan is a Professor of Physics and Astronomy at Johns Hopkins University, where he has been a faculty member since 2002. He holds a PhD from the University of Washington (1999) and completed postdoctoral research at the University of Chicago/Argonne National Lab and SLAC. His research focuses on theoretical extensions of the Standard Model of particle physics and cosmology, with emphasis on dark matter, axions, quantum gravity, and experimental probes of fundamental physics. Notably, he created and produced Particle Fever , a documentary film awarded the DuPont Journalism Award. Key research interests include exploring new physics beyond the Standard Model, such as models addressing the strong CP problem, probing dark matter interactions via atom interferometry and spin precession, and studying cosmological implications of gravitational theories. He is a Fellow of the American Physical Society (APS), a DOE Outstanding Junior Investigator, Kavli Frontiers Fellow, and Alfred P. Sloan Fellow. His work integrates theoretical frameworks with experimental efforts, such as collaborations at SQMS (Quantum Sensing) and proposals for next-generation experiments like GALILEO (Galactic axion laser interferometer). His recent articles address topics ranging from nonlinear quantum mechanics to gravitational wave detection and cosmological constant relaxation.
