Find Academic Supervisors

• Accelerator Physics
• Beam Dynamics
• Radio-Frequency Photoinjectors
• +5 more

Thorsten Kamps is a Professor of Physics at Humboldt University of Berlin and Head of the Department of High-Brilliance Electron Beams at Helmholtz-Zentrum Berlin . He is also Deputy Project Manager for the Superconducting RF Electron Accelerator Laboratory SEALAB . Education: Graduate Physicist (Dipl.-Phys.) from TU Dortmund (formerly University of Dortmund), Doctor rerum naturalium (Dr. rer. nat.) from Humboldt University of Berlin Research Interests: Particle accelerator beam dynamics, diagnostics, superconducting radio-frequency photoinjectors (SRF photoinjectors), photocathode growth, instrumentation for bright electron beams, free-electron lasers, ultrafast scattering sources, and future trends of accelerator-driven light sources Expertise: Accelerator physics, beam physics of electron beams, photoinjectors, storage rings, electron beam diagnostics, free-electron lasers, and project management of large-scale accelerator projects Labs/Teams: Involved with SEALAB (Superconducting RF Electron Accelerator Laboratory), BERLinPro (Berlin Energy Recovery Linac Project), and collaborations with institutions like Royal Holloway University of London, DESY, and DELTA/University of Dortmund Publications Trends: Thorsten Kamps’ recent works focus on SRF photoinjectors, beam diagnostics, photocathode development, and thermal load studies. His research spans applications in ultrafast electron diffraction, laser-driven acceleration, and energy-recovery linacs, with collaborations across Europe and the US. Topics include interferometric beam monitoring, multi-alkali antimonide materials, and solenoid alignment for beam control. Teaching: Promotes education in accelerator physics through BSc and MSc courses, and supervises BSc, MSc, and PhD students. Develops practical experiments for internships in accelerator physics.

Ben MargalitView profile

Assistant Professor

• Theoretical Astrophysics
• Time-domain Astronomy
• Neutron Star Mergers
• +7 more

Ben Margalit is an active Assistant Professor in the School of Physics and Astronomy at the University of Minnesota, specializing in theoretical astrophysics with a focus on high-energy transient phenomena. His research centers on time-domain astronomy, particularly neutron star mergers, gravitational-wave events, fast radio bursts, gamma-ray bursts, and supernovae. His research interests span theoretical astrophysics with emphasis on radiative processes , compact objects , neutron star equation-of-state , circumstellar interaction , non-thermal emission , accretion , nuclear astrophysics , and various types of shocks in astrophysical environments. His work integrates theoretical modeling with observational data to understand extreme cosmic events. Analysis of his recent publications reveals a strong focus on fast radio bursts (FRBs) and their host environments, with significant work on neutron star physics, shock dynamics, and multi-wavelength observations of transients. His research shows increasing emphasis on connecting theoretical models with observational constraints from facilities like CHIME. Dr. Margalit currently leads two major research projects: Accurately Modeling Emission from Fast, Mildly-Relativistic Transients funded by the National Science Foundation (2025-2028) and Not so heavy metal: an enhanced rate of SLSNe at Cosmic Noon funded by Research Corporation (2025-2026), demonstrating substantial grant acquisition capability. He is affiliated with the Minnesota Institute for Astrophysics and collaborates extensively with researchers globally, particularly in the fast radio burst community. His work contributes significantly to understanding high-energy transient phenomena and their underlying physical mechanisms in the universe.

• Mechanical Engineering
• Artificial Intelligence
• Tribology
• +3 more

Hassan Shirvani is a Professor of Engineering Design and Simulation at the School of Engineering and the Built Environment, Anglia Ruskin University. He serves as Director of the Engineering Analysis Simulation and Tribology (EAST) Research Group, focusing on industry collaborations to solve engineering challenges. PhD in Mechanical Engineering, University of Bath MSc in Mechanical Engineering, University of Birmingham Member, Institute of Mechanical Engineers (IMechE) His research spans mechanical engineering, artificial intelligence, and biomedical applications, including: Thermal system optimization Machine learning in clinical decision-making Composite metal foil manufacturing Virtual reality medical training systems Flow dynamics in heat exchangers and nozzles AI-assisted diagnostics Hybrid manufacturing processes Hassan's publications reflect expertise in computational modeling, multi-physics simulations, and industrial applications. Notable areas include deep learning for suicide prediction, thermodynamic analysis of sustainable energy systems, and tribology in mechanical components.

Kuver SinhaView profile

Associate Professor

• Early Universe Cosmology
• High Energy Particle Physics
• String Phenomenology
• +4 more

Kuver Sinha holds the Carl T. Bush Professorship of Theoretical Physics and is an Associate Professor in the Homer L. Dodge Department of Physics and Astronomy at the University of Oklahoma. His work bridges particle physics, cosmology, and string theory, focusing on the early Universe's first moments. He earned his Ph.D. from Rutgers University in 2008, advised by Emanuel Diaconescu, and has held postdoctoral positions at Texas A&M and shifted to cosmology/astroparticle physics. His research explores early Universe cosmology, axion searches, dark matter in extreme environments, and the string landscape's implications for SUSY. Recent work emphasizes gravitational waves from phase transitions, primordial black holes, and axion detection via neutron stars. He leads a vibrant group with postdocs (Tao Xu, Fazlollah Hajkarim, Kun-Feng Lyu) and graduate students (Aditi Shahani, Badal Bhalla, etc.). His awards include the Carl T. Bush Professorship. Key collaborations include organizing the 2020/2021 PPC conference and hosting CUWiP 2020. His publications span gravitational wave signatures, dark matter constraints, and string phenomenology. Advising spans over a dozen students/postdocs, with alumni such as Huaike Guo (University of Utah) and Daniel Vagie (industry). Education: Ph.D. in Physics, Rutgers University (2008) Research Interests: Early Universe cosmology, axion physics, primordial black holes, gravitational waves, string landscape

• Gravitational Wave Physics
• General Relativity
• Astrophysics
• +3 more

Elisa Maggio is a Research Fellow at the Max Planck Institute for Gravitational Physics (Albert Einstein Institute) in Potsdam, Germany. She holds a PhD from Sapienza University of Rome, where her thesis, Probing new physics on the horizon of black holes with gravitational waves , earned multiple awards including the Amaldi Research Center Prize, Giulio Rampa Prize, and Fubini Prize. Her work focuses on testing general relativity in extreme environments using gravitational waves, particularly investigating the nature of black hole horizons and alternative theories of gravity. As a Marie Curie Fellow, she contributes to the ThorGW project, exploring horizon properties with future detectors like LISA and the Einstein Telescope. Her research involves modeling gravitational wave signals from compact object mergers, analyzing ringdown phases, and developing parametrized waveform models for precision tests. Notable contributions include studies on horizonless compact objects and their gravitational wave signatures. Maggio’s position is supported by grants from the Leibniz Prize (DFG) and Marie Skłodowska-Curie Actions. Elisa has been recognized with prestigious honors such as the Laura Bassi Prize for early-career women in physics (2024) and the Sapienza University of Rome’s thesis prize (2025). Her work bridges theoretical physics with observational challenges, advancing our understanding of gravity’s limits in strong-field regimes.

• Beyond the Standard Model physics
• Neutrino phenomenology
• Astroparticle physics
• +2 more

Vedran Brdar is an Assistant Professor in the Department of Physics at Oklahoma State University, where he has been serving since November 2023. His academic journey includes a PhD from Johannes Gutenberg University of Mainz (2014-2017), followed by postdoctoral positions at Max Planck Institute for Nuclear Physics in Heidelberg, Fermilab and Northwestern University, and a Senior Research Fellowship at CERN. Dr. Brdar's research focuses on Beyond the Standard Model physics , with particular emphasis on neutrino phenomenology and astroparticle physics . His work bridges theoretical particle physics with experimental observations from neutrino detectors and astrophysical sources. Key areas of investigation include: Neutrino properties and interactions beyond the Standard Model Connections between neutrino physics and cosmology Novel experimental approaches to detect new physics Applications of astrophysical phenomena as laboratories for particle physics Analysis of Dr. Brdar's recent publications reveals a strong focus on neutrino physics across multiple contexts - from terrestrial experiments to astrophysical sources. His work frequently explores connections between different areas of physics, particularly the interface between particle physics, astrophysics, and cosmology. A notable trend is the development of novel experimental approaches to detect physics beyond the Standard Model, often by repurposing existing facilities or combining different types of detectors. Dr. Brdar has received funding from the U.S. Department of Energy for his project "Seeking New Physics Across the Scales: From Neutrinos and Gravitational Waves to Exotics" (2024-2026), demonstrating recognition of his research program by major funding agencies. His teaching portfolio at Oklahoma State University includes advanced courses such as Introductory Quantum Mechanics and Doctoral Dissertation Research, as well as undergraduate courses like University Physics II. He also serves as a judge for the Oklahoma State Science and Engineering Fair, demonstrating commitment to outreach and education.

• Radio Astronomy
• Exoplanets
• Stellar Mass-loss
• +3 more

Dr. H.K. Vedantham is a Research Fellow at the Kapteyn Astronomical Institute , part of the Faculty of Science and Engineering at the University of Groningen . His work focuses on radio astronomy and astrophysics, particularly the study of exoplanets, brown dwarfs, and stellar systems through low-frequency radio observations and interferometric techniques. Research Interests: Radio astronomy of exoplanets and sub-stellar objects Stellar mass-loss and magnetic interactions Space weather phenomena Astrometric and radial velocity measurements Publications highlight his contributions to understanding radio emission mechanisms in exoplanetary systems, stellar magnetospheres, and dwarf galaxies. His work frequently involves collaborations using advanced instruments like LOFAR and VLBI networks. Contact: Email: h.k.vedantham@rug.nl Phone: +31 50 36 34073

Karsten DanzmannView profile

Professor

• Gravitational Wave Astronomy
• Laser Interferometry
• Quantum Measurement
• +2 more

Karsten Danzmann is a Professor at Leibniz Universität Hannover and Director of the Max Planck Institute for Gravitational Physics (Albert Einstein Institute) since 2002. He leads the Laser Interferometry and Gravitational Wave Astronomy department, focusing on advanced technologies for gravitational wave detection. Education : Diploma in Physics (1977), Universität Hannover PhD in Atomic and Molecular Physics (1980), Universität Hannover His research interests span gravitational wave astronomy, laser interferometry, quantum measurement, and space-based detector technology. He pioneered key innovations at the GEO600 detector, including squeezed light implementation and high-power lasers, now used in LIGO, Virgo, and KAGRA. He also leads the LISA space mission consortium for low-frequency gravitational wave detection in space. Scientific awards : Honorary Doctorate (RWTH Aachen, 2025) Edison Volta Prize (2018) Princess of Asturias Award (2017) Gruber Prize (2016) Hall of Fame der deutschen Forschung (2019)

Mathieu RenzoView profile

Assistant Professor

• Stellar astrophysics
• Massive stars
• Binary evolution
• +7 more

Mathieu Renzo is an Assistant Professor in the Astronomy Department and Steward Observatory at the University of Arizona, Tucson. His research focuses on stellar physics, particularly massive stars, binary evolution, and stellar explosions. He employs both detailed stellar structure and evolution models (using MESA) and rapid population synthesis codes (binary_c and COSMIC), combined with galactic dynamics simulations. Current Position: Assistant Professor, University of Arizona (2024-present) Previous Positions: Research Fellow at Flatiron Institute and Columbia University (2019-2023) Education: PhD from University of Amsterdam (2019), Masters and Bachelors from University of Pisa Dr. Renzo's research interests span stellar kinematics (including runaway, "walkaway", and hyper-velocity stars), core-collapse and (pulsational) pair-instability supernovae, nuclear astrophysics, X-ray binaries, and gravitational-wave astronomy. His work combines analytical calculations with numerical simulations to understand massive star evolution, their explosions, and binary interactions. He is particularly interested in how binary evolution impacts stellar outcomes and gravitational wave sources. His recent publications reveal a strong focus on binary star systems across different metallicities, with significant contributions to understanding common envelope evolution, supernova feedback mechanisms, and the formation channels of compact objects. His work often involves large collaborations like the BLOeM (Binarity at LOw Metallicity) project. KITP Graduate fellowship (2017) NSF AAG grant 'One step back and two step forward' (2025, $372,000) NASA ATP grant 'multi-D RHD simulations of mass transfer' (2023, $380,000) PI of multiple computing projects on Dutch supercomputer Cartesius Dr. Renzo actively mentors students at various levels, including PhD candidates at the University of Arizona and international collaborations. His research group uses advanced computational tools including MESA (where he's a core developer), ATHENA++, and COSMIC. He is involved in several major collaborations studying massive stars across different environments, with particular attention to how binary interactions shape stellar evolution and end states.

Richard J. FurnstahlView profile

Professor

• Effective field theory
• Renormalization group methods
• Computational nuclear physics
• +3 more

Richard J. Furnstahl is a Professor in the Department of Physics at The Ohio State University. His research focuses on effective field theory (EFT), renormalization group methods, computational nuclear physics, and low-energy nuclear theory. He holds prestigious fellowships from the American Physical Society (2001) and the American Association for the Advancement of Science (2007), and was recognized as an APS Outstanding Referee (2009). He also received the OSU Alumni Award for Distinguished Teaching (1997). Education: B.S. in Physics from MIT (1981), Ph.D. in Physics from Stanford University (1986). Research emphasizes applying EFT and Bayesian methods to nuclear systems, including neutron star equations of state, nucleon-nucleon scattering, and uncertainty quantification. His work bridges computational techniques like eigenvector continuation and reduced-order emulators with foundational theories such as chiral EFT. Recent efforts focus on interpolating between small- and large-coupling regimes and quantifying correlated truncation errors in dense nuclear matter models. Key contributions include developing the Density Matrix Expansion approach for energy density functionals and advancing the FRIB Theory Alliance for nuclear dynamics studies. His emulators reduce computational costs while maintaining accuracy in scattering problems. He also explores the intersection of machine learning and nuclear theory through Bayesian additive regression trees and neural network applications. He leads projects on nuclear symmetry energy, proton Compton scattering experiments, and the NUCLEI initiative for ab initio nuclear structure calculations. His work emphasizes rigorous uncertainty analysis and theoretical consistency across scales.

• Astrophysics
• Radio Astronomy
• Active Galactic Nuclei
• +3 more

Rajan Chhetri is an Adjunct Research Associate at Curtin University, affiliated with the Curtin Research Institute and Curtin Institute of Radio Astronomy (CIRA), within the School of Electrical Engineering, Computing, and Mathematical Sciences. His research focuses on active galactic nuclei (AGNs), populations of radio sources, and multi-wavelength studies of extragalactic phenomena. He has conducted extensive work using radio interferometry and interplanetary scintillation techniques with instruments like the Murchison Widefield Array (MWA) and the Australia Telescope 20 GHz (AT20G) survey. Chhetri’s investigations include studying compact AGNs at high radio frequencies, analyzing gravitational lensing in the Southern hemisphere, and exploring how AGNs interact with their galactic environments. His recent projects involve leveraging interplanetary scintillation to detect sub-arcsecond compact objects at low radio frequencies, enabling unprecedented resolution without upgrading telescope capabilities. This work contributes to understanding cosmic phenomena like supermassive black hole activity and the structure of the interplanetary medium. His research outputs span over two decades, with notable contributions to surveys like GLEAM, AT20G, and MWA IPS, yielding insights into radio source populations, galaxy evolution, and space weather effects. Chhetri has also engaged in public outreach, bridging astronomy research with broader audiences.

Sarp AkcayView profile

Assistant Professor

• General Relativity
• Gravitational Waves
• Black Holes
• +3 more

Sarp Akcay is an Assistant Professor/Lecturer in the School of Mathematics and Statistics at University College Dublin (UCD). He holds an Ad Astra Fellowship and has prior postdoctoral roles including IRC Postdoctoral Fellow at UCD (2014–2016) and STFC Fellowships at the University of Southampton (2009–2012 and 2013–2014). His research focuses on general relativity, gravitational waves, and compact binary systems, with affiliations in the LIGO-Virgo Collaboration and LISA Consortium. Education: PhD in Physics from the University of Texas at Austin, and a Professional Certificate in University Teaching & Learning from UCD. Research interests include modeling gravitational waveforms for compact binaries, spin precession effects, and extreme mass ratio inspirals. He leads the TEOBResumS waveform model development and collaborates on LIGO/Virgo data analyses. Currently supervises one PhD student and three undergraduates in gravitational wave projects. Grants include the Ad Astra Start-Up Grant (2020–2025) and Irish Research Council funding for self-force research. Teaching includes modules on General Relativity, Vector Calculus, and Mathematical Modelling.

• Antenna Engineering
• 6G/5G Communications
• Metamaterials
• +6 more

Ming Shen is an Associate Professor at the Department of Electronic Systems, part of The Technical Faculty of IT and Design at Aalborg University. His research focuses on antennas, millimeter-wave systems, and AI-driven RF sensors with applications in 5G/6G communications, biomedical engineering, and smart systems. His research interests span antenna design (including phased arrays, metamaterials, and compact structures), AI integration in electromagnetic systems, and medical sensor technologies. Recent projects include drone-based electromagnetic signature analysis, vibration energy harvesting for pacemakers, and smart healthcare systems for posture recognition and surgical site infection monitoring. Key projects include DRONES: Drone-Obtained Electromagnetic Signatures (2024–2028), Sensor Intelligence for Healthcare and Sports (2022–2027), and DeepBone (2021–2022), which explored deep learning for surgical infection detection. His work also bridges machine learning and electromagnetic design, with breakthroughs in surrogate modeling and automated antenna optimization. Ming Shen has supervised 6 PhD students and published over 160 peer-reviewed articles. Notable contributions include AI-assisted NLOS sensing, ultra-wideband antenna innovations, and medical applications such as electrical impedance-based bone healing assessment.

Woodam ChungView profile

Professor

• Forest Operations
• Forest Management
• Forest Planning
• +3 more

Woodam Chung serves as Professor and Stewart Professor of Forest Operations in the College of Forestry at Oregon State University. He leads research in forest operations planning and management, specializing in harvesting systems, biomass utilization, and wildland fire management. His work integrates engineering solutions with sustainable forestry practices. Research interests include forest management planning, steep slope harvesting, tethered equipment applications, biomass logistics, and fuel treatment optimization. Current projects focus on reducing wildfire risks through strategic fuel break networks and enhancing operational efficiency in challenging terrains. Publications demonstrate consistent focus on operational efficiency, environmental impacts, and technological innovation in forestry. Recent work emphasizes tethered harvesting systems, soil disturbance mitigation, computer vision applications, and wildfire risk management strategies. Currently advises seven graduate students on topics spanning forest operations, biomass utilization, and wildfire management. Maintains active collaborations with industry partners and land management agencies.

Alan MurrayView profile

Professor

• Geographic Information Science
• Spatial Optimization
• Emergency Response Planning
• +5 more

Alan Murray is a **Professor and Vice Chair for Academic Personnel** in the Department of Geography at the University of California, Santa Barbara (UCSB), where he also holds the Yardi Chair in Geography. He previously held professorial roles at Ohio State University, Arizona State University, and Drexel University before returning to UCSB in 2015. Murray earned his BS in Mathematics, Master’s in Statistics and Applied Probability, and PhD in Geography, all from UCSB. His research focuses on **geographic information science (GIScience)**, **spatial optimization**, **emergency response**, **health informatics**, **urban development**, and **infrastructure systems**. He has pioneered methodologies for integrating multi-objective spatial optimization with GIS to address urban planning challenges, such as smart mobility and wildfire risk mitigation. His work emphasizes practical applications in disaster response, public health, and sustainable land use planning. Murray has advised numerous graduate students and contributed to cross-disciplinary initiatives in GIScience education and technology integration. His research has been disseminated through high-impact publications in journals like *Geographical Analysis* and *International Journal of Geographical Information Science*. He has also directed centers such as the Center for Urban and Regional Analysis. Key areas of current research include: GIScience education reform Spatial optimization for emergency response systems Wildfire risk assessment and community resilience Equitable urban planning frameworks His work bridges theoretical advancements with real-world applications, addressing pressing issues like climate adaptation, infrastructure resilience, and smart city design.