Prof. Dr. Dominik Schwarz is a faculty member at the Faculty of Physics , Bielefeld University. His research focuses on Cosmology and Particle Physics , particularly in the areas of Dark Energy , Dark Matter , Cosmological Inflation , and Large-Scale Structure Formation . He contributes to projects like the International LOFAR Telescope Consortium and the SFB-TRR 211 on strongly interacting matter. APART Fellow of Austrian Academy of Sciences Humboldt Fellow CERN Fellow His recent work explores the cosmic dipole anisotropy , axion density perturbations , and multi-wavelength cosmic web mapping . He also advances data science infrastructure through the PUNCH4NFDI consortium.
Mark Trodden is the Dean of the School of Arts & Sciences and Thomas S. Gates Jr. Professor of Physics and Astronomy at the University of Pennsylvania. He previously served as the Fay R. and Eugene L. Langberg Professor of Physics, Department Chair, and Co-Director of the Center for Particle Cosmology. His career includes faculty roles at Syracuse University (2000–2009) and visiting positions at Case Western Reserve University and Cornell University. Ph.D. and M.Sc. in Physics, Brown University (1992–1995) Advanced Study in Mathematics, University of Cambridge (1990–1991) M.A. in Mathematics, University of Cambridge (1987–1990) Trodden’s research focuses on the intersection of cosmology and particle physics, addressing fundamental questions such as the nature of dark energy, dark matter, the baryon asymmetry of the universe, inflation, and modified gravity theories. His work explores how cosmological data can constrain physics beyond the Standard Model and general relativity. His publications span topics like dark energy models , inflationary spacetimes , topological defects , and BPS states in supersymmetric theories , reflecting his expertise in connecting high-energy physics to cosmological observations. At Penn, Trodden has held editorial roles for journals like Physics Letters B and Journal of Cosmology and Astroparticle Physics , and has contributed to collaborative workshops advancing cosmology and particle physics.
Matthew W. Kunz is an Associate Professor of Astrophysical Sciences at Princeton University, serving as Associate Chair of the Department of Astrophysical Sciences and Director of Graduate Studies for the Program in Plasma Physics. He holds a B.S. in Astronomy-Physics and B.A. in Music from the University of Virginia (2003), and a Ph.D. in Physics from the University of Illinois at Urbana-Champaign (2009). His research focuses on astrophysical plasma dynamics, including instability, turbulence, and transport in weakly collisional and poorly ionized plasmas, with applications to galaxy clusters, accretion disks, and the solar wind. Dr. Kunz's work employs analytical and numerical methods to study multi-scale plasma dynamics, aiming to understand angular momentum transport in accretion disks, kinetic turbulence cascades, and magnetic field evolution. His research has been recognized with several awards, including an NSF CAREER Award (2020-25), Alfred P. Sloan Research Fellowship (2017-20), and NASA Einstein Postdoctoral Fellowship (2011-14). He teaches courses on plasma astrophysics (AST 521), irreversible processes in plasmas (AST 554), and astrophysical research methods (AST 303). His publications demonstrate a consistent focus on plasma turbulence, magnetic reconnection, and cosmic ray propagation, with recent work emphasizing collisionless plasma dynamics and high-energy astrophysical phenomena.
Dr. Alain Bonneville is a Lab Fellow and Geophysicist at Pacific Northwest National Laboratory (PNNL) and holds a Courtesy Professor appointment at Oregon State University's College of Earth, Ocean, and Atmospheric Sciences. With extensive experience in geological storage of CO2, geothermal energy, and geophysical monitoring techniques, Dr. Bonneville leads diverse research projects that bridge fundamental science and practical applications for energy and environmental challenges. Dr. Bonneville's educational background includes: PhD in Geophysics from the University of Montpellier, France MS in Petroleum Geophysics from IFP-School, Paris, France BS in Geology from the University of Lyon, France Dr. Bonneville's research spans several critical areas in Earth sciences and energy systems. His work on geothermal energy focuses on super-hot enhanced geothermal systems (EGS), site characterization, monitoring, and stimulation fluids. In geological CO2 storage, he investigates project management, site characterization, numerical modeling, and monitoring methods using potential fields and remote sensing. His expertise in geophysical methods includes heat flow measurements, gravity surveys, muon tomography development for borehole deployment, and remote sensing applications. Additional research areas encompass marine heat flow instrumentation development, thermal monitoring of active volcanoes, and intraplate volcanism studies in the Indian and Pacific Oceans. Dr. Bonneville has received significant recognition for his contributions to science, including: Membership in the Washington State Academy of Sciences Lab Fellow position at Pacific Northwest National Laboratory Executive Committee membership on the U.S. National Risk Assessment Partnership Scientific Committee membership at IFP-Energies Nouvelles, France He also holds two U.S. patents related to electrophilic acid gas-reactive fluids for enhanced fracturing and recovery of energy producing materials. Throughout his career, Dr. Bonneville has led significant research initiatives, including the PNNL Carbon Sequestration Initiative (2009-2013) and the European Marie Curie Research Training Network on Greenhouse Gas Removal (GRASP), which involved 14 academic and industrial institutions across 7 countries and supported 35 PhD students and post-docs. His work on the FutureGen 2.0 project demonstrates his leadership in large-scale carbon storage site characterization and monitoring program design. Dr. Bonneville maintains active collaborations with research teams at PNNL's Environmental Molecular Sciences Laboratory and works closely with Oregon State University's geoscience researchers. His laboratory work focuses on developing novel instrumentation for geophysical monitoring, particularly in the areas of muon tomography for subsurface characterization and thermal monitoring systems for geothermal and carbon storage applications.
Prof. Dr. Michael Klasen is a leading theoretical physicist at the Institute of Theoretical Physics at the University of Münster, where he heads his eponymous research group. His work bridges nuclear and particle physics, with significant contributions to quantum chromodynamics and physics beyond the Standard Model. His research focuses on Particle Physics , Quantum Chromodynamics , and Physics beyond the Standard Model , with particular emphasis on understanding the quark-gluon structure of atomic nuclei and dark matter phenomena. His innovative approach connects microscopic quark-gluon dynamics with nuclear binding phenomena, creating a crucial bridge between nuclear and particle physics. Prof. Klasen's recent work analyzing nucleon binding at the quark-gluon level was recognized as a "Breakthrough of the Year 2024" by Physics World. His research group's publication in Physical Review Letters demonstrated how quarks and gluons behave differently in nucleon pairs than in free nucleons, fundamentally advancing our understanding of nuclear binding. Breakthrough of the Year 2024 from Physics World Leadership of Research Training Group 2149 "Strong and weak interactions - from hadrons to dark matter" Supervision of award-winning doctoral research including the Infineon Dissertation Prize 2025 Prof. Klasen has successfully mentored numerous PhD students, with 20 of his group's graduates continuing their academic careers at prestigious institutions including CERN and Stanford University. His research has been supported by major funding bodies including the German Research Foundation (DFG), the Helmholtz Alliance for Astroparticle Physics, and BMBF collaborative research programs. The Klasen working group maintains active collaborations with international research networks including CTEQ, DM@NLO, and RESUMMINO.
Yakov Shlapentokh-Rothman is an Assistant Professor jointly appointed in the Department of Mathematics at the University of Toronto St. George and the Department of Mathematical and Computational Sciences at the University of Toronto Mississauga. His research focuses on the intersection of partial differential equations, general relativity, and geometric analysis, with particular emphasis on black hole physics and the Einstein field equations. Education: PhD: Massachusetts Institute of Technology (2015) BS with Honors: Stanford University (2010) Research Interests: Shlapentokh-Rothman's work explores fundamental problems in mathematical relativity, including black hole stability, singularity formation, wave propagation in curved spacetimes, and the asymptotic behavior of solutions to Einstein's equations. His research combines rigorous PDE analysis with deep geometric insights. Publications focus on: black hole dynamics, scattering theory in curved spacetimes, stability analysis of Kerr and Reissner-Nordström solutions, cosmic censorship conjectures, and self-similar solutions to Einstein's equations. Recent work examines the structure of naked singularities and decay properties of fields in black hole backgrounds. Awards and Recognition: Alfred P. Sloan Fellowship in Mathematics Advising and Grants: Currently advising PhD student: Avyay Venkat Viswanath Research supported by NSERC Discovery Grants (RGPIN-2021-02562, DGECR-2021-00093)
Professor August Evrard is a distinguished academic at the University of Michigan, holding the Arthur F. Thurnau Professorship in Physics and Astronomy. He is affiliated with the Department of Physics within the College of Literature, Science, and the Arts. Known for his contributions to cosmology and astrophysics, he pioneered the Problem Roulette tool, recognized with the Provost's Teaching Innovation Prize. His research focuses on galaxy clusters, dark matter, and cosmological surveys like the Dark Energy Survey (DES) and XXL Survey. He has been honored as an AAS Fellow (2025) and has contributed to advancements in physics education through innovative teaching methods and technologies. In research, Prof. Evrard explores topics such as dark matter halo dynamics, galaxy cluster properties, and weak lensing analyses. His work spans observational cosmology, computational modeling, and multi-wavelength astronomy. Notable projects include studies on galaxy cluster mass distributions, the relationship between X-ray emissions and velocity dispersions, and the application of machine learning to astrophysical data analysis. His contributions to education highlight the integration of AI-driven tools to enhance learning, as seen in initiatives like the Problem Roulette and course recommendation systems. Prof. Evrard's awards include the Provost's Teaching Innovation Prize for Problem Roulette and his AAS Fellowship. His academic leadership and innovative approaches to both research and education solidify his role as a pivotal figure in astrophysics and STEM pedagogy.
Alyson M. Brooks is an Associate Professor in the Department of Physics and Astronomy at Rutgers University, part of the School of Arts and Sciences. Her research focuses on galaxy formation and evolution, particularly using cosmological simulations to study dark matter dynamics, stellar abundances, and galactic structures. She holds a PhD in Astronomy from the University of Washington (2008) and has held prestigious fellowships, including the Sherman Fairchild Fellowship at Caltech and the Grainger Postdoctoral Fellowship at UW-Madison. Brooks has been recognized with awards such as the 2015 Alfred P. Sloan Research Fellowship and the 2019 Maria Goeppert Mayer Award from the American Physical Society. Her educational background includes a B.A. in Physics with Astronomy from Macalester College (2000) and an M.S. in Astronomy from the University of Washington (2004). Her research interests span topics like the interplay between baryonic processes and dark matter, chemical evolution in dwarf galaxies, and the role of feedback mechanisms in galaxy formation. Brooks is actively involved in outreach, including founding the RU-PREP program to support undergraduate research and mentoring initiatives. Brooks has authored over 100 refereed publications, with recent work exploring the resolved stellar populations of dwarf galaxies using the James Webb Space Telescope and analyzing dark matter halo properties through simulations. Her scientific contributions have advanced understanding of galaxy kinematics, dark matter interactions, and the evolution of galactic structures across cosmic time.
Michael G. Smith is a Professor of History at Purdue University's College of Liberal Arts, specializing in Russian History and Aerospace History. His office is located in BRNG 6170, where he holds office hours by appointment and before or after class. Dr. Smith teaches a diverse range of courses including History of Russia to 1861 (HIST 238), History of Russia from 1861 (HIST 239), History of Aviation (HIST 384), and History of the Space Age (HIST 387), along with numerous advanced seminars on Russian history, aerospace history, and global historical topics. Dr. Smith earned his Ph.D. from Georgetown University in 1991 and has established himself as a leading scholar in both Russian revolutionary history and aerospace history. His research demonstrates remarkable interdisciplinary breadth, connecting linguistic studies with political history in the Soviet context while simultaneously exploring the cultural dimensions of space exploration and aviation history. His scholarly output reveals two major research trajectories: deep investigations into the Russian Revolution with particular focus on language policy, nationalities issues, and revolutionary violence in Azerbaijan and the Caucasus region; and pioneering work on the history of aerospace, space exploration, and the cultural dimensions of the Space Age. These dual interests converge in his examination of how technological innovation intersects with political ideology and national identity formation. Dr. Smith has successfully mentored numerous undergraduate and graduate students whose research has resulted in publications in respected journals such as the Journal of Purdue Undergraduate Research, Quest: The History of Spaceflight Quarterly, and Astropolitics. His students have explored diverse topics including Purdue's aviation pioneers, NASA mission insignia, Shuttle-Mir program, and regional impacts of space programs. Working closely with the Purdue Archives, Dr. Smith has developed innovative archival-research seminars that have produced multiple student publications and special projects including Flight Paths: Purdue University's Aerospace Pioneers and Purdue Students Study Boilermaker Eugene Cernan's Remarkable Career. His commitment to connecting historical research with contemporary technological heritage has created unique opportunities for students to engage with primary sources related to aerospace history.
Professor David Alexander is a distinguished academic at Durham University's Department of Physics, where he serves as Professor and Chair of Board of Examiners. His responsibilities include Head of Section for Astronomy and Director of Postgraduate Research, demonstrating his significant leadership role within the department. Alexander is also responsible for teaching the Stars Lecturer component of the Level 2 Stars and Galaxies course. His primary research interests focus on Active Galactic Nuclei, black holes, and galaxy formation and evolution, representing core areas in modern astrophysics. Alexander's work spans observational and theoretical aspects of high-energy astrophysics, with particular emphasis on understanding the connections between supermassive black holes and their host galaxies across cosmic time. His research leverages data from major international facilities including NuSTAR, ALMA, DESI, and XMM-Newton, conducting multi-wavelength studies that combine X-ray, infrared, optical, and radio observations. Analysis of his most recent publications reveals a strong focus on AGN demographics, obscuration mechanisms, quasar environments, and the role of AGN in galaxy evolution. His work frequently explores the connection between AGN activity and galaxy properties, with particular attention to the cosmic evolution of these relationships. Recent papers demonstrate increasing emphasis on large-scale surveys and statistical approaches to understanding AGN populations. Leverhulme Research Fellowship (2000-2012) Philip Leverhulme Prize (2000-2008) Royal Society University Research Fellowship (2000-2003) Thomson Reuters ESI highly cited researcher over 2002-2012 Professor Alexander has been instrumental in numerous major survey projects including the NuSTAR extragalactic surveys, DESI quasar studies, and the VST ATLAS Quasar Survey. His collaborative work spans international teams and leverages cutting-edge observational facilities across the electromagnetic spectrum. His research group focuses on understanding the physical processes that govern AGN activity and their connection to galaxy evolution, with particular emphasis on obscured AGN populations and their role in the cosmic black hole growth history.
Prof. Dr. Julia A. B. Hegewald is a Professor of Oriental Art History at the University of Bonn, Germany, affiliated with the Institute of Oriental and Asian Studies (IOA) and the Department of Asian and Islamic Art History (AIK). Her research focuses on artistic expressions of dependency in Asian art, particularly South Asian, using 're-use' theory to explore cultural integration and creativity under adversity. She holds a Ph.D. from SOAS, University of London, and a Habilitation from RWTH Aachen. Key academic roles include founding the Cam-Kar Research Institute in Mysore (since 2002) and serving on editorial boards for journals like the Journal of Global Archaeology and Veranda . She has led major projects, including the Emmy Noether Junior Research Group on Jainism in Karnataka (2005–2014). Awards include the DFG Emmy Noether extension (2011–2014) and the Prix en études indiennes (2010). Hegewald has authored over 3 books, edited 6 volumes, and published 77 academic articles. Her work bridges art history with cultural studies, addressing themes like Jaina temple architecture, Indo-Islamic syncretism, and modern Indian urban planning. She actively contributes to global academic networks, including the European Association for Asian Art and Archaeology (EAAA).
Professor Oscar Dias is a faculty member in the Department of Mathematical Sciences at the University of Southampton. His research focuses on Einstein's gravity, black holes, holographic dualities, and gravitational aspects of string theory. He actively supervises PhD students in mathematical sciences and holds grants from the Science and Technology Facilities Council (STFC), including projects like 'New Frontiers in Particle Physics, Cosmology and Gravity.' His work explores topics such as cosmic censorship, black hole dynamics, and numerical general relativity, with recent contributions published in journals like Physical Review Letters and Journal of High Energy Physics . Key research interests include the study of black hole binaries in de Sitter space, the stability of charged black holes, and the interplay between holographic dualities and quantum field theories. His projects often involve collaborations with leading institutions, addressing foundational questions in theoretical physics and cosmology. Professor Dias is a member of the Southampton Theory Astrophysics and Gravity (STAG) Research Centre and the String Theory and Holography group. His articles highlight advancements in understanding gravitational wave phenomena, quasinormal modes, and the behavior of black holes under various physical conditions. He currently accepts PhD applications and can be contacted via O.J.Campos-Dias@soton.ac.uk.
Pierre Baldi is a Distinguished Professor of Computer Science and Director of the Institute for Genomics and Bioinformatics at the University of California, Irvine (UCI). He is affiliated with the Donald Bren School of Information and Computer Sciences. His research spans artificial intelligence, machine learning, bioinformatics, and communication networks, with notable projects in protein structure prediction, gene expression modeling, and neutrino physics collaborations like DUNE. Baldi’s work bridges theoretical foundations (e.g., neural network theory) and applied domains, including medical imaging and fusion technology. Key research interests include AI-driven biomedical applications, neural network theory, and interdisciplinary projects such as the DUNE neutrino experiment. His contributions to neural network engineering were recognized with the 2023 INNS Dennis Gabor Award, highlighting his paradigm-changing impact on computational neuroscience and physics. Baldi’s academic leadership includes directing UCI’s Institute for Genomics and Bioinformatics, fostering collaborations in computational biology and AI. His recent work explores AI’s role in healthcare, climate modeling (e.g., ClimSim-Online), and fundamental physics challenges like neutrino oscillation studies.
Dr Christian Luczanits serves as the David L. Snellgrove Senior Lecturer in Tibetan and Buddhist Art at SOAS University of London, where he also acts as Department Recruitment, Admissions and Marketing Convenor. He previously held research positions at the University of Vienna, Austrian Academy of Sciences, and Lumbini International Research Institute, followed by visiting professorships at UC Berkeley , Free University Berlin, and Stanford University. Before academia, he was Senior Curator at the Rubin Museum of Art, New York. PhD in Tibetan and Buddhist Studies (University of Vienna) under the late Maurizio Taddei Specializes in early Buddhist art (1st-5th centuries) and early Tibetan Buddhist art (7th-15th centuries) Key research topics: Maitreya iconography , development of Mahāyāna and esoteric traditions, Tibetan artistic adaptation of Indian forms, and AHRC-funded monastery collections documentation in Mustang and Ladakh His recent publications analyze transcultural dynamics in Himalayan Buddhist heritage, including monastic collections, mandala symbolism, and artistic revival movements. He co-curated the Gandhara – The Buddhist Heritage of Pakistan exhibition at Bonn's Kunst- und Ausstellungshalle der Bundesrepublik Deutschland. PhD supervisees include: Udomluck Hoontrakul (Political Economy of Marginal Polities) Qianhui Lin (Bodhisattva Conceptualization in Gandhāra) Agneta Niklasson (Esoteric Buddhism in Swat-Gilgit-Kashmir sculpture) Dr Lesley S Pullen (Angkorian Divine Adornment) Kulamitra David Zukas (Rock-Cut Buddhist Monasteries)
Dan McCammon is a Professor in the Department of Physics at the University of Wisconsin-Madison, affiliated with the College of Letters & Science. His research focuses on X-ray astronomy, including studies of the diffuse X-ray background, interstellar and intergalactic media, and the development of advanced X-ray instrumentation. He is a key contributor to the XRISM (X-ray Imaging and Spectroscopy Mission) satellite, leading efforts in high-resolution X-ray spectroscopy and mission operations. McCammon's work emphasizes understanding cosmic plasma dynamics, galaxy cluster physics, and supernova remnant evolution through cutting-edge observational techniques and detector technology. His research interests span multiple subfields, including the thermodynamic properties of galactic clusters, charge-exchange processes in astrophysical plasmas, and the design of cryogenic microcalorimeters for space-based observatories. He has pioneered advancements in transition-edge sensors (TES) and superconducting detectors, enhancing the precision of X-ray spectral measurements. McCammon has contributed to numerous sounding rocket missions, such as Micro-X, and has been instrumental in the development of the Line Emission Mapper (LEM) probe concept, aimed at mapping the soft X-ray sky with unprecedented resolution. His work on the Hitomi (ASTRO-H) satellite demonstrated breakthroughs in resolving the thermal and dynamic properties of cosmic plasmas, such as the Perseus galaxy cluster and the Crab Nebula. His publications highlight a focus on high-resolution X-ray spectroscopy of cosmic sources, including galaxy clusters, active galactic nuclei, and supernova remnants. He has explored topics like non-thermal pressure contributions in cluster cores, ionized plasma diagnostics, and the role of charge-exchange emissions in interpreting diffuse X-ray backgrounds. McCammon's instrumentation innovations have enabled breakthroughs in measuring spectral features with sub-eV resolution, advancing our understanding of astrophysical processes. Despite the absence of explicitly listed awards or grants in the provided text, his leadership in major space missions and pioneering detector technologies underscores his contributions to the field. His research team collaborates on international projects, such as XRISM and LEM, reflecting a commitment to advancing observational astrophysics through interdisciplinary collaboration.
