Dr. Paul Johns is a Distinguished Research Professor in the Department of Physics at Carleton University, affiliated with the Ottawa Medical Physics Institute (OMPI). His research focuses on innovative medical x-ray imaging techniques, including x-ray scatter imaging, dual-energy radiography, and focal spot mapping. He holds academic distinctions such as Fellowships from the Canadian College of Physicists in Medicine and the Canadian Organization of Medical Physicists, and received the Sylvia Fedoruk Prize in Medical Physics. Johns' career spans roles at AECL Power Projects, Ottawa Civic Hospital, and Carleton University since 1988. He previously chaired the Canadian Organization of Medical Physicists (1996-1998) and led Carleton's Physics Department as Chair (2005-2008). His research emphasizes leveraging x-ray wave behavior to enhance diagnostic capabilities while minimizing patient exposure. Key projects include developing scatter-based imaging systems and measuring x-ray scattering cross sections for tissues and materials. Publications highlight advancements in synchrotron-based scatter imaging, energy-dispersive form factor measurements, and multi-beam imaging systems. His work bridges fundamental physics and clinical applications, contributing to non-destructive testing and security screening beyond medicine. Active collaborations include the Canadian Light Source for synchrotron experiments.
Maria Chekhova is a Research Professor and Group Leader of the Quantum radiation research group at the Max Planck Institute for the Science of Light in Erlangen, Germany. Her position as an independent research group leader at one of the world's premier physics research institutions places her at the forefront of quantum optics research. Professor Chekhova's research spans three interconnected domains: Quantum Optics, focusing on nonclassical states of light including single-photon, two-photon, three-photon, and squeezed states; Quantum Metrology, investigating sub-shot-noise measurements, quantum sensing, and nonlinear interferometry; and Nonlinear Optics, exploring strongly pumped parametric down-conversion, four-wave mixing, and parametric amplification. Her work bridges fundamental quantum phenomena with practical applications in quantum information science. Analysis of Professor Chekhova's publication record reveals a consistent focus on quantum state generation and characterization, with recent work (2025) advancing photon pair generation in subwavelength films, entangled photon generation in resonant structures, and multimode squeezing measurement techniques. Her research demonstrates a progression from fundamental quantum phenomena toward increasingly sophisticated quantum technologies with practical applications. Professor Chekhova has made significant contributions to quantum optics through her leadership of the Chekhova Research Group at the Max Planck Institute. Her team operates at the intersection of quantum information, nanophotonics, and quantum metrology, developing novel approaches to generate and characterize nonclassical light states for applications in quantum communication, sensing, and computation.
Dr. Uwe Hommerich is a Professor of Physics at Hampton University's School of Science. His research focuses on luminescent materials development, laser spectroscopy, and crystal growth for applications in solid-state lasers, optical amplifiers, and photonic devices. He leads a research group advancing mid-infrared gain media using low-phonon energy halide crystals and infrared laser-induced breakdown spectroscopy (IR-LIBS) for environmental and security monitoring. Education: B.S. (1986) and M.S. (1990) from the University of Oldenburg, Germany; Ph.D. (1994) from the University of Hamburg, Germany (collaboration with University of Georgia, USA). Research emphasizes rare earth-doped materials, with recent work on IR-LIBS applications for energetic materials analysis and pharmaceutical monitoring. Collaborations include Brimrose Corporation of America and Edgewood Chemical Biological Center. Teaching philosophy integrates experimental physics with theoretical principles and project-based learning. Key research areas include mid-infrared emission optimization, crystal purification techniques, andLIBS-based chemical sensing. His publications span applied optics, spectroscopy, and materials science, advancing technologies for homeland security, environmental science, and industrial processes. No scientific awards explicitly listed, but active in interdisciplinary research and university-industry partnerships. Advising details not explicitly provided in text.
Hang Yu is an Assistant Professor of Physics at Montana State University affiliated with the College of Letters & Science. His research spans theoretical and experimental gravitational-wave astrophysics, focusing on tidal interactions in compact binaries, LIGO instrumentation, and machine learning applications. He holds a Ph.D. from MIT (2019) and B.S. from Johns Hopkins University (2014). Education: Ph.D. in Physics, MIT, 2019 B.S. in Physics (with Honor), Johns Hopkins University, 2014 Research Interests: Tidal interactions in neutron stars/black holes, LIGO commissioning, machine learning for gravitational wave analysis, hierarchical triple systems. Active in detector development (e.g., TianGO project). Awards & Grants: Recipient of grants from NASA and NSF supporting tidal dynamics research. Involved in detector sensitivity improvement projects like LIGO-LF concept. Service: Referee for journals including PRL, PRD, ApJ, and CQG. Contributed to LIGO commissioning activities at both Livingston and Hanford sites.
Partha Chowdhury is a Professor and Head of the Graduate School at the Kennedy College of Sciences, University of Massachusetts Lowell (UML). He holds a Ph.D. in Physics from the State University of New York, Stony Brook (1979), following an MA (1976) and BS from the Indian Institute of Technology, Kharagpur (1974). His research focuses on gamma-ray spectroscopy and nuclear structure, with contributions to neutron spectroscopy, scintillator development, and high-spin physics. Education: Ph.D. Physics, SUNY Stony Brook, 1979 MA Physics, SUNY Stony Brook, 1976 BS Physics, IIT Kharagpur, 1974 His work explores nuclear structure phenomena, including isomer decay mechanisms, collective excitations, and triaxial deformation in superheavy nuclei. Recent studies involve scintillator-based neutron detection and machine learning applications in spectroscopy. Chowdhury has led collaborations on fast neutron spectroscopy and gamma-ray tracking with detectors like GRETINA. Publications span gamma-ray instrumentation, decay spectroscopy of neutron-rich nuclei, and theoretical challenges in superheavy element stability. His research bridges experimental nuclear physics with advanced detector technologies. No scientific awards are explicitly listed, though his contributions to gamma-ray spectroscopy are widely recognized in the field. Advising and grants: No specific students or grants mentioned, but his role as a faculty member and graduate program head suggests extensive mentorship and leadership in research initiatives. Labs/Teams: Active in collaborations at facilities like CARIBU and with teams using Gammasphere and GRETINA detectors for nuclear structure studies.
Gabriela González is a Boyd Professor of Physics at Louisiana State University's Department of Physics & Astronomy. She holds a Ph.D. from Syracuse University (1995) and a Licenciada from the University of Córdoba (1988). Her research focuses on gravitational wave detection using LIGO interferometers, with expertise in instrument characterization, data calibration, and binary coalescence analysis. Her work involves reducing noise sources like seismic disturbances and scattered light to achieve unprecedented detector sensitivity. She served as spokesperson for the LIGO Scientific Collaboration (2011-2017), coordinating international research efforts that confirmed Einstein's predictions about spacetime ripples from cosmic events. Her research group develops calibration frameworks enabling landmark discoveries, including the first detection of black hole mergers and neutron star collisions. She maintains close collaboration with the LIGO Livingston Observatory located 30 miles from LSU campus.
Collin Capano is a Research Associate Professor in the Physics department at Syracuse University. He holds a Ph.D. and B.S. in Physics from Syracuse University (2011 and 2005 respectively). His research focuses on gravitational wave astronomy, black hole spectroscopy, and computational methods for analyzing astrophysical data. He has led projects involving black hole ringdown analysis, neutron star equation of state studies, and multimessenger astronomy. Dr. Capano has secured significant grants including a National Science Foundation award for developing black hole spectroscopy methods and desktop cluster infrastructure (2024-2026) and a Defense University Instrumentation Initiative grant (2022). He currently directs the Open Source Project Office at Syracuse University's Research Computing division. His work has been published in top journals like Physical Review D , Nature Astronomy , and The Astrophysical Journal . Notable contributions include testing general relativity with GW170817 observations and constraining neutron star radii through combined gravitational-wave and electromagnetic data analysis. Awarded the Max-Planck-Gesellschaft performance bonus (2020), he serves as a reviewer for leading journals including Physical Review Letters , Monthly Notices of the Royal Astronomical Society , and Classical and Quantum Gravity . He actively participates in international workshops and conferences, presenting on topics ranging from black hole spectroscopy to the future of gravitational wave astronomy.
Alexander Harvey Nitz is an Associate Professor and Director of Graduate Studies in the Department of Physics at Syracuse University's College of Arts and Sciences. His research focuses on gravitational-wave astronomy and the astrophysics of compact objects, including neutron stars, black holes, and dark matter. He develops high-performance data analysis techniques and contributes to next-generation gravitational-wave observatories. Education Ph.D. in Physics, Syracuse University (2015) B.S. in Physics, University of Michigan (2010) Research Interests Dr. Nitz's work centers on gravitational-wave astronomy , with emphasis on compact binary systems and astrophysical signatures . His research spans neutron stars , black holes , dark matter searches, and high-performance data analysis . He actively develops methods for third-generation detectors like Cosmic Explorer to probe the gravitational-wave universe with unprecedented sensitivity, focusing on eccentric systems, subsolar-mass binaries, and multi-messenger connections. Research Trends Recent publications (2023-2025) show Dr. Nitz's increasing focus on gravitational-wave searches for sub-solar mass binaries , eccentric compact binaries , and multi-messenger astronomy . His work addresses critical challenges for future observatories, including nonstationary noise mitigation, efficient template banking, and parameter estimation in low-SNR regimes. The trend demonstrates a strategic shift toward preparing analysis frameworks for Cosmic Explorer while maximizing science from current LIGO-Virgo-KAGRA data. Grants and Service Dr. Nitz co-leads major research initiatives as co-Principal Investigator on National Science Foundation grants supporting gravitational-wave astronomy and Cosmic Explorer development. He also directs open-source infrastructure through the Sloan Foundation-funded Syracuse University Open Source Program Office. NSF Grant (2024-2027) : "From Detector Hardware to Astrophysics: An Open Control and Analysis Architecture for Cosmic Explorer" NSF Grant (2023-2026) : "Gravitational-wave Astronomy and Astrophysics at Syracuse University" Sloan Foundation Grant (2023-2025) : "Syracuse University Open Source Program Office (SU-OSPO)" He serves as Physics Department's Director of Graduate Studies, chairs promotion committees, and is an active reviewer for leading journals including Physical Review D and Classical and Quantum Gravity. Dr. Nitz co-organized the 2024 Gravitational-wave Physics and Astronomy Workshop and mentors undergraduate researchers through the SUPER-Tech SHIP program. Labs and Teams As a key member of the LIGO Scientific Collaboration, Dr. Nitz leads development of the PyCBC gravitational-wave analysis software suite. His group collaborates internationally on detector characterization, data analysis pipelines, and multi-messenger follow-up. Current efforts focus on scalable algorithms for next-generation observatories and extracting novel astrophysical signatures from gravitational-wave data.
Roles & Affiliations: Dag Winkler is a Professor at Chalmers University of Technology, specializing in Quantum Component Physics. He has held academic roles including Head of the Department of Microtechnology and Nanoscience – MC2 (2007–2016) and previously served as a lecturer at the University of Gothenburg. His research focuses on superconductivity, quantum devices, and applications in bioassays and neuroimaging. Education: PhD in Physics from Chalmers (1987). Postdoctoral research at Yale University (1988–1990). Research Interests: Tunneling phenomena in superconductors, HTS SQUIDs for MEG/ULF-MRI, and 2D electronic properties at oxide interfaces. Key projects include multifunctional materials, Josephson junctions, and magnetic sensor systems. He has pioneered advancements in cryogenic electronics and superconducting quantum interference devices (SQUIDs). Publications: Over 100 peer-reviewed articles, including work on superconducting interfaces, SQUID magnetometers, and bioassay technologies. Recent research emphasizes nanoscale patterning and applications in neuroimaging systems. Advising & Grants: Extensive leadership in research projects funded by VR, SSF, and the EU. Contributions span nanotechnology, quantum sensing, and biomedical applications. Notable collaborations include ABB Corporate Research (cryogenic systems) and Acreo (microwave technology). Labs & Teams: Former head of the Quantum Device Physics Laboratory and MC2 Department. Active in developing cutting-edge SQUID-based systems and bioassay platforms for medical diagnostics.
Kerstin Borras is a Professor of Physics at RWTH Aachen University and a Leading Scientist at DESY, Germany's national research center for particle accelerators. She specializes in experimental particle physics, particularly in the analysis of the Standard Model and the strong interaction, with extensive experience in detector development for high-energy physics experiments. Affiliations: DESY (German Electron Synchrotron) RWTH Aachen University CMS Experiment Collaboration at CERN's LHC Her research focuses on CMS experiment operations at the LHC, including detector design, data analysis, and quench protection for superconducting magnets. She has led the DESY CMS group and serves as Deputy Spokesperson for the CMS collaboration. Borras' work bridges accelerator physics and detector technology, emphasizing superconducting RF cavities and material science for particle accelerators. Key contributions include advancing Nb3Sn magnet technologies, optimizing quench protection systems, and developing thin-film superconductors for next-generation accelerators. She actively participates in international committees like the Helmholtz Think Tank and the European Committee for Future Accelerators (ECFA). Research Themes: High-energy collider physics Superconducting magnet systems Detector development for particle physics experiments Material science for accelerator components
Edoardo Lopriore is a Researcher at the Laboratoire d'électronique et structures à l'échelle nanométrique (LANES) within the School of Engineering (STI) at École Polytechnique Fédérale de Lausanne (EPFL). His research focuses on nanoscale electronic systems, layered materials, and optoelectronic devices, particularly in van der Waals heterostructures. He has contributed to the development of ultrafast photodetectors, tunable exciton dynamics, and cryogenic ASICs for particle physics experiments. His work intersects semiconductor physics, quantum devices, and materials science, with applications in both fundamental research and advanced technology. Key themes in his publications include electrical characterization of layered materials, interlayer exciton interactions, and high-precision electronics for cryogenic environments. He collaborates on projects like the Deep Underground Neutrino Experiment (DUNE), emphasizing interdisciplinary innovation. Edoardo's research emphasizes experimental and theoretical analysis of nanomaterials' electronic and optoelectronic properties, with a focus on translating fundamental discoveries into functional devices. His lab website can be found at https://lanes.epfl.ch .
Prof. Corsin Battaglia is a Lecturer at the Department of Information Technology and Electrical Engineering at EMPA, Switzerland. His work focuses on electromagnetic compatibility (EMC), shielding effectiveness, and reverberation chamber applications. He has contributed to IEEE standards such as P2715 and P2716, addressing board-level and planar material shielding characterization. His research explores topics like stochastic electromagnetic field coupling, absorption cross-section analysis, and the impact of internal loading on shielding performance. Collaborations include studies on high-voltage antennas for IEMI testing and thermal noise effects in reverberation environments. His publications span experimental validations, theoretical models, and novel measurement techniques in EMC. Research interests include electromagnetic field modeling, shield design optimization, and EMC standardization. His recent work emphasizes practical applications of EMC principles in automotive and high-frequency electronics contexts. No specific grants or awards are listed, though his involvement in international conferences and standards indicates significant professional recognition. His lab focuses on advancing EMC methodologies through experimental and theoretical approaches.
Lydie GIOT is an Associate Professor at IMT Atlantique's SUBATECH Laboratory since 2006, specializing in reactor physics and nuclear safety. She holds a PhD in Nuclear Physics (2003) with a European Doctorate label from the Universities of Caen and Surrey. Her research focuses on decay heat calculations, nuclear data uncertainty propagation, and molten salt reactor modeling. She has led projects like ENDURANCE (2024–2028) and APRENDE (2024–2028), addressing Generation IV reactor challenges. She advises on EU nuclear safety initiatives and chairs the Nuclear Technology course for engineering students. Key roles include representing IMT Atlantique in the European Industrial Alliance for Small Modular Reactors and co-chairing the CNRS steering committee for MSR systems. Education: PhD in Nuclear Physics (2003), Marie Curie Fellowships (2002–2006) Teaching: Responsible for reactor physics courses and STAR engineering program (2009–2017) Recognition: Knight of the French Academic Palms (2022), SAMPO Fellowship (2015) Her work bridges fundamental physics (antineutrino oscillations in Double Chooz/SoLid experiments) with applied nuclear engineering, emphasizing decay heat safety for reactor design and waste management. Collaborations span CEA, IRSN, and international organizations like OECD/NEA.
Cora Salm is a Lecturer in the Department of Integrated Devices and Systems at the University of Twente, affiliated with the MESA+ Institute for Nanotechnology. Her research focuses on semiconductor device reliability, hot-carrier effects, and microelectromechanical systems (MEMS). She has contributed to studies on device degradation mechanisms, environmental impact on materials, and advanced fabrication techniques for high-performance electronics. Key research areas include hot-carrier degradation in MOSFETs, environmental recovery phenomena, and reliability of RFID tags under thermal stress. Her work spans semiconductor materials, plasma processing, and the integration of MEMS with CMOS technologies. Notable collaborations involve investigations into LHC dipole circuit transients and radiation detector development using wafer post-processing. Recent publications highlight advancements in understanding charge trapping dynamics, humidity effects on ferroelectric capacitors, and RF MEMS switch characterization. She has presented at multiple international conferences and contributed to proceedings on microelectronics education and semiconductor reliability.
Dr. A.J. Noble is a Professor in the Department of Physics, Engineering Physics and Astronomy at Queen's University, and the inaugural Scientific Director of the McDonald Institute. He holds cross-appointments in the Arthur B. McDonald Canadian Astroparticle Physics Institute and the Canadian Particle Astrophysics Research Centre. His research focuses on dark matter detection through experiments at SNOLAB, including DEAP-3600 (liquid argon) and PICO (superheated fluids). He has also contributed to accelerator experiments at TRIUMF, CERN, and the ANTARES neutrino telescope. Noble earned his PhD in Elementary Particle Physics from the University of British Columbia (1990). Education: PhD (1990) - Elementary Particle Physics, University of British Columbia MSc - Elementary Particle Physics, University of British Columbia Research Interests: Dr. Noble's work centers on astroparticle physics, particularly direct detection of dark matter using advanced underground experiments. He investigates cosmogenic neutrons, neutrino interactions, and novel detector technologies like bubble chambers and liquid argon scintillation. His contributions span both experimental design (e.g., DEAP-3600's position reconstruction) and interdisciplinary projects like the Mechanical Ventilator Milano during the COVID-19 pandemic. Affiliations & Leadership: Director of the Canadian Particle Astrophysics Research Centre (2016–present) and SNOLAB (2009–2013). He advises postdoctoral researchers such as Serge Nahornyi and collaborates internationally on projects like IceCube and PICO. Labs/Teams: Leads the DEAP collaboration and contributes to PICO, leveraging SNOLAB's deep underground facilities to minimize cosmic background interference.
