جستجوی استاد راهنمای دانشگاهی

Allen I. Mincerمشاهده پروفایل

استاد

• Experimental High Energy Particle Physics
• Astrophysics
• Cosmic Ray Physics
• +۲ مورد دیگر

Allen Mincer is a Professor of Physics and Collegiate Professor at New York University's College of Arts and Science, Department of Physics. He leads research in experimental high energy particle physics and astrophysics as a member of the NYU Experimental Particle Physics Group, with major contributions to the ATLAS and Milagro collaborations. His educational background includes a Ph.D. from the University of Maryland, College Park (1984) and a B.S. from Brooklyn College (1978). Mincer's research spans particle physics discoveries (top quark, Higgs boson) and cosmic ray astrophysics. He specializes in detector development, data analysis for high-energy collisions, and cosmic ray observations. His work integrates experimental physics with innovative educational approaches, particularly in physics pedagogy. Analysis of his publications (2020-2005) reveals dual research trajectories: LHC-focused studies on Higgs physics, supersymmetry searches, and trigger systems via ATLAS, alongside Milagro-based cosmic ray research mapping TeV emissions and anisotropies in the Galactic plane. His scientific recognition includes: Teach/Tech Award, New York University (2018) Collegiate Professor appointment at NYU (2008) Golden Dozen Teaching Award, NYU (1995, 2000) Mincer mentors undergraduate and graduate researchers while pioneering physics education through flipped classrooms, experimental pedagogy courses, and curriculum development for courses ranging from introductory physics to graduate particle physics. He actively contributes to the NYU Experimental Particle Physics Group, maintaining leadership roles in ATLAS detector operations and Milagro cosmic ray data analysis.

• Nonlinear Dynamics
• Planetary Dynamics
• Solar Physics
• +۶ مورد دیگر

Norm Murray is a Professor at the Canadian Institute for Theoretical Astrophysics (CITA) within the University of Toronto . With a Ph.D. from UC Berkeley (1986), his research spans nonlinear dynamics , planetary formation , solar system evolution , and active galactic nuclei . His work combines theoretical physics with observational data from radio telescopes, X-ray satellites, and cosmological simulations. Recent research focuses on galaxy formation (via FIRE simulations), dark matter interactions in dwarf galaxies, and AGN disk dynamics . He employs machine learning for planetary collision modeling and investigates the interplay of magnetohydrodynamics and radiative transfer in quasar environments. Publications highlight his expertise in computational astrophysics, spanning topics from cosmic molecular gas mapping to the stability of exoplanetary systems.

G. Scott Watsonمشاهده پروفایل

استاد

• Early Universe Cosmology
• Inflation
• Dark Matter
• +۳ مورد دیگر

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).

Kevin Clarnoمشاهده پروفایل

دانشیار

• Nuclear and Radiation Engineering
• Computational Nuclear Energy
• Multiphysics Simulation
• +۵ مورد دیگر

Kevin Clarno is a tenured Associate Professor in the Department of Nuclear and Radiation Engineering at the University of Texas at Austin, holding the Charlotte Maer Patton Centennial Fellowship in Engineering. His research focuses on computational nuclear energy, multiphysics reactor simulation, and high-performance computing (HPC). Previously, he spent 15 years at Oak Ridge National Laboratory (ORNL), where he led major initiatives such as the Consortium for Advanced Simulation of Light Water Reactors (CASL) and contributed to the development of software tools like SCALE, CTF, and VERA. Education and Career: Assistant Professor at University of Tennessee-Knoxville (2010–2016) Senior Research Scientist at ORNL (2006–2021) Research Interests: Multiphysics coupling methods for reactor simulation Multiscale neutronics and thermal-hydraulics modeling Advanced reactor design (e.g., molten salt reactors) HPC-driven software integration for nuclear analysis Uncertainty quantification in coupled simulations Grants and Projects: Lead of CASL’s Physics Integration Focus Area Development of the Advanced Multi-Physics (AMP) fuel code ORNL-led strategic research projects in reactor simulation Labs and Tools: VERA: Virtual Environment for Reactor Applications CTF: Thermal-hydraulic solver for PWR analysis MPACT: Neutronics simulation tool within SCALE

• Dark Matter Research
• Particle Physics
• Plasma Physics
• +۳ مورد دیگر

Prof. Dieter H.H. Hoffmann is a distinguished academic in the Department of Physics , specializing in high-energy physics, dark matter detection, and plasma-based fusion research. His work focuses on particle astrophysics, including axion searches via helioscopes like CAST, nuclear fusion mechanisms (particularly proton-boron reactions), and plasma dynamics in extreme conditions. He collaborates on major projects such as the Cherenkov Telescope Array (CTA) for gamma-ray astronomy and heavy-ion beam experiments at facilities like FAIR. Research interests include: Dark matter axion detection and theoretical modeling Proton-boron fusion as an alternative energy pathway Plasma interactions in high-intensity laser and beam experiments Stopping power and beam transport in dense matter High-energy-density physics for inertial confinement fusion Recent work highlights advancements in: CAST experiment sensitivity improvements for solar axions Experimental validation of proton-boron fusion yields in dense plasmas Development of NectarCAM cameras for CTA's gamma-ray detection Simulation of proton beam dynamics in solid-state materials His contributions bridge fundamental physics with applied research in energy and detector technology, with active involvement in international collaborations like CTA and FAIR experiments.

Edison P. Liangمشاهده پروفایل

استاد

• High Energy Density Physics
• High Energy Astrophysics
• Plasma Physics
• +۵ مورد دیگر

Edison P. Liang is the Andrew Hays Buchanan Professor of Astrophysics at Rice University, where he has served since 1991. Previously, he held positions at Stanford University, Michigan State University, and Lawrence Livermore National Laboratory (LLNL), where he led research groups in plasma physics and astrophysics. His research focuses on relativistic plasma physics, high-energy density physics, laser-plasma interactions, and high-energy astrophysical phenomena. He earned his BA (1967) and PhD (1971) in Physics from UC Berkeley, supported by the UC Science Fellowship and Anthony Scholarship. Key professional milestones include: Recipient of the British SRC Senior Visiting Scientist Fellowship (1974) Co-founder of the High Energy Density Laboratory Astrophysics (HEDLA) conference series Contributor to major NAS and SAUUL reports on High Energy Density Physics Organized over a dozen international astrophysics conferences Current research emphasizes computational modeling of relativistic plasmas, laboratory astrophysics, and antimatter creation using intense lasers. His group collaborates on both theoretical and experimental projects, with active involvement in HEDP applications to fusion, gamma-ray generation, and medical physics. Recent studies include relativistic jet dynamics, magnetic reconnection mechanisms, and shock-driven particle acceleration processes. Awarded over 300 peer-reviewed publications and conference proceedings, Liang is a Fellow of the American Physical Society and holds honorary memberships in Sigma Xi and Phi Beta Kappa. His group advises current graduate students Kyle Perez and Brandon Cage, with notable alumni including Guy Hilburn and Yingchao Lu. Research infrastructure includes advanced computational simulations and collaborations with national labs like LLNL.

• Solar Physics
• Space Physics
• Heliospheric Physics
• +۵ مورد دیگر

Zigong Xu is a Postdoctoral Scholar Research Associate in Physics at the California Institute of Technology (Caltech), affiliated with the Division of Physics, Mathematics, and Astronomy. His research focuses on solar energetic particles (SEPs), heliospheric physics, and cosmic ray dynamics. His work leverages data from missions like Solar Orbiter, Parker Solar Probe, and Chang’E-4 to study particle acceleration mechanisms, interplanetary shock dynamics, and the propagation of energetic particles in the solar environment. His research interests span solar flares, coronal mass ejection interactions, and the interplay between solar eruptions and the Earth-Moon radiation environment. He has contributed to understanding phenomena such as inverse velocity dispersion in SEPs, cosmic ray cavities in near-Earth space, and the composition variations of 3He-rich SEP events. Collaborations with multi-spacecraft missions highlight his expertise in analyzing particle data across diverse heliospheric distances. Zigong has explored topics including galactic cosmic ray shielding on the lunar surface, thermodynamic properties of solar protons, and the role of coronal shocks in particle acceleration. His studies often involve advanced statistical methods and comparative analyses of observations from instruments like EPT and HET aboard Solar Orbiter, and ISOIS on Parker Solar Probe. No formal awards or grants are explicitly mentioned, though his extensive publication record reflects active engagement in the field. He collaborates with international teams on missions such as Chang’E-4’s Lunar Lander Neutron and Dosimetry (LND) experiment, advancing lunar surface radiation studies.

• High-Energy Astrophysics
• Astrophysics

Norbert Meidinger is a Researcher in the High-Energy Astrophysics department at the Max Planck Institute for Extraterrestrial Physics (MPE) in Garching, Germany, focusing on cosmic high-energy phenomena including X-ray and gamma-ray emissions from celestial sources. His research spans High-Energy Astrophysics , investigating extreme astrophysical environments such as black holes, neutron stars, and active galactic nuclei to understand particle acceleration and radiation mechanisms in the universe. Contact is available via email at nom@mpe.mpg.de or telephone at +49 89 30000-3866.

David Seckelمشاهده پروفایل

استاد

• Cosmic Ray Physics
• Neutrino Astrophysics
• High Energy Physics
• +۳ مورد دیگر

David Seckel is a Professor of Physics & Astronomy at the University of Delaware, affiliated with the College of Arts & Sciences. His research focuses on cosmic rays, neutrino astrophysics, and the development of large-scale observatories like the IceCube Neutrino Observatory and the ANITA detector. He has contributed to studies of ultra-high-energy cosmic rays, neutrino detection techniques, and cosmological implications of particle interactions. Key research areas include analyzing atmospheric and astrophysical neutrino fluxes, probing cosmic ray composition via air shower measurements, and investigating neutrino emission from active galactic nuclei. His work leverages advanced detector technologies and machine learning methods for data analysis. Collaborations include the IceCube Collaboration, RNO-G radio array, and the PUEO payload for airborne neutrino detection.

• Theoretical Astroparticle Physics
• High-Energy Astrophysics
• Gamma-Ray Astronomy
• +۱۰ مورد دیگر

Anita Reimer is a Full Professor at the Institute for Astro- and Particle Physics, Faculty of Mathematics, Computer Science and Physics, University of Innsbruck. Her research focuses on theoretical astroparticle physics, particularly high-energy phenomena in active galactic nuclei (AGN), blazars, gamma-ray bursts, and cosmic-ray acceleration, with strong involvement in major international collaborations such as Fermi-LAT, H.E.S.S., and the Cherenkov Telescope Array (CTA). Her research interests center on multi-messenger astrophysics, exploring the connections between gamma rays, neutrinos, and cosmic rays. She develops theoretical models for particle acceleration and emission in relativistic jets, photohadronic interactions, and neutrino production in AGN. Her work often bridges theoretical predictions with observational data from space- and ground-based telescopes. The recent publications of Prof. Reimer span topics such as TeV gamma-ray emission from Eta Carinae, periodic modulation in blazars, cosmic-ray electron spectra, and dark matter searches. These works reflect a strong emphasis on observational constraints for theoretical models, multiwavelength analysis, and the physics of extreme astrophysical environments. She has delivered numerous invited talks at international conferences on topics including neutrino-emitting blazars, multi-messenger astronomy, and theoretical modeling of AGN jets. She collaborates extensively with leading research groups worldwide and contributes to major catalog efforts like the Fermi-LAT source catalogs. She advises students and junior researchers in high-energy astrophysics and is actively involved in large-scale projects such as the Cherenkov Telescope Array, contributing to both instrumentation and science preparation. Her work is central to advancing our understanding of particle acceleration and emission in the most energetic sources in the universe.

Mauricio Bustamanteمشاهده پروفایل

استادیار

• Astroparticle physics
• Neutrino physics
• Ultra-high-energy astrophysical neutrinos and cosmic rays
• +۵ مورد دیگر

Mauricio Bustamante is an Assistant Professor at the Niels Bohr Institute , University of Copenhagen, specializing in theoretical high-energy astrophysics, astroparticle physics, and neutrino phenomenology. His research bridges cosmic phenomena with fundamental particle physics, focusing on ultra-high-energy neutrinos, cosmic rays, gamma-ray bursts, and new physics beyond the Standard Model. PhD in Physics (2012-2014) M.Sc. in Physics (2007-2010) B.Sc. in Physics (2001-2006) His work explores neutrino oscillations, self-interactions, and decay in extreme astrophysical environments. He contributes to major international collaborations like GRAND (Giant Radio Array for Neutrino Detection) and IceCube-Gen2, developing simulation pipelines and forecasting detection methods for EeV-scale neutrinos. Recent publications highlight energy-dependent flavor transitions, Lorentz invariance testing, and constraints on long-range neutrino interactions via DUNE and T2HK experiments. He actively participates in peer review for journals such as Physical Review D , Physical Review Letters , and Astrophysical Journal , and has attended conferences like TeV Particle Astrophysics (2017). His research emphasizes detector design, cosmic ray reconstruction via graph neural networks, and multi-messenger astronomy.

Elisa Resconiمشاهده پروفایل

استاد

• Particle Astrophysics
• Neutrino Physics
• Multi-Messenger Astronomy
• +۳ مورد دیگر

Prof. Dr. Elisa Resconi is a Professor of Experimental Physics with Cosmic Particles at the Technische Universität München (TUM) within the TUM School of Natural Sciences. Her research bridges particle physics and astrophysics, focusing on cosmic neutrinos as messengers to study high-energy astrophysical accelerators, dark matter, and non-standard neutrino properties. Academic Affiliation: TUM School of Natural Sciences, Department of Physics Research Interests : Investigating cosmic neutrino sources (e.g., IceCube-170922A blazar TXS0506+056) Probing neutrino mass hierarchy and dark matter through astrophysical observations Developing experimental techniques for high-energy neutrino detection (e.g., PMT characterization) Multi-messenger astronomy combining neutrino, photon, and cosmic ray data Scientific Awards : Heinz Maier-Leibnitz Medal (2017) Max Planck Fellow (2017) Heisenberg Professorship (2012) Emmy Noether Junior Research Group Leader (2005) Marie Curie Individual Fellowship (2002) Teaching Roles : Lecturer in Applied Multi-Messenger Astronomy Instructor for Python programming boot camps Advisor for FOPRA experiments and journal clubs on neutrino and dark matter research Organizer of colloquia on neutrino and dark matter topics

• Medical Physics
• Radiation Therapy
• Radiation and Matter Interactions
• +۳ مورد دیگر

David Bolst is a Research Fellow at the School of Physics, University of Wollongong, within the Faculty of Engineering and Information Sciences. His research focuses on medical physics, radiation therapy, and computational modeling with applications in both clinical and space environments. Dr. Bolst has contributed significantly to the development and validation of Geant4-based models for hadron therapy, microdosimetry systems, and radiation protection technologies. Research Interests: His work spans medical physics (radiation therapy dosimetry, particle therapy modeling), radiation-matter interactions (secondary fragmentation, LET analysis), and space radiation protection (astronaut shielding, galactic cosmic ray studies). He has pioneered the use of silicon-on-insulator (SOI) microdosimeters for radiation quality assessment in diverse environments. Funding & Collaborations: He leads projects including the 'Advanced microdosimetry for particle therapy and space medicine' (2021-2022) and 'Anthropomorphic Phantom Ionising Radiation Modelling and Simulation' (2021-2022). Collaborations include institutions like CATANA and the Geant4 Medical Simulation Benchmarking Group. Grants: RevITAlise Research Grant Scheme (RITA): Advanced microdosimetry for particle therapy and space medicine (2021) Defence Materials Technology Centre: Anthropomorphic Phantom Modelling (2021) Labs/Teams: Involved in the G4-Med system development and the SOI microdosimeter project teams. Engaged with international collaborations in radiation physics and space medicine.

Nassim Bozorgniaمشاهده پروفایل

استادیار

• Astroparticle Physics
• Dark Matter Phenomenology
• Cosmology
• +۳ مورد دیگر

Nassim Bozorgnia is an Assistant Professor in the Department of Physics at the University of Alberta and a Tier 2 Canada Research Chair in Astroparticle Physics. He specializes in theoretical astroparticle physics and dark matter phenomenology, focusing on dark matter's particle nature and its implications for direct/indirect detection experiments. His research uses cosmological simulations and observational data to study dark matter distribution in galaxies like the Milky Way. Education: Ph.D. in Physics, UCLA (2012), Dissertation: 'Ion Channeling in Direct Dark Matter Detection' M.S. in Physics, San Francisco State University (2006) B.S. in Physics, Kharazmi University (2004) Research Interests: His work explores dark matter interactions, galactic distribution modeling, and astroparticle physics. Key areas include: Dark matter direct detection using crystal detectors Impact of Large Magellanic Cloud on dark matter signals Velocity-dependent annihilation radiation Dark matter distribution correlations with stellar kinematics Grants & Awards: Canada Research Chair (2022–2027) Natural Sciences and Engineering Research Council (NSERC) Discovery Grant (2020–2025) McDonald Institute Highly Qualified Personnel Pooled Resources (2021–2023) Recipient of multiple fellowships including UCLA's Cota Robles Fellowship Teaching & Supervision: Currently supervising 6 Ph.D./M.S. students and mentoring EXPLORE program participants Teaches courses like 'Physical Cosmology' and 'Dark Matter: from cosmology to underground searches' Developed the EXPLORE international research collaboration program Labs & Collaborations: Active in collaborations like the EXPLORE program and international initiatives such as GRAPPA and IPPP. His work integrates cosmological simulations (EAGLE, APOSTLE) with observational datasets to refine dark matter models.

David A. Williamsمشاهده پروفایل

استاد مدعو

• High-Energy Astrophysics
• Gamma-Ray Astronomy
• Cosmic Rays
• +۳ مورد دیگر

David A. Williams is an Adjunct Professor of Physics at the University of California, Santa Cruz . He is a member of the VERITAS and CTA collaborations, focusing on high-energy gamma-ray astronomy. Additionally, he is an Affiliated Scientist with the Fermi -Large Area Telescope project. Ph.D. from Harvard University (1987) Office: Room 319, Natural Science 2 Email: daw@ucsc.edu Research Interests Williams investigates high-energy astrophysical phenomena using ground-based gamma-ray telescopes. Key research areas include: Understanding gamma-ray bursts and their emission mechanisms Analyzing active galactic nuclei (particularly blazars) and their relativistic jets Studying cosmic rays and their acceleration processes in astrophysical systems Developing advanced instrumentation for experiments like VERITAS and CTA Investigating absorption of gamma rays via cosmic microwave background interactions His recent publications highlight collaborative work on TeV gamma-ray detection, source analysis, and telescope design advancements. Collaborations VERITAS : Observational gamma-ray astronomy with 12m telescopes CTA : Chair of the CTA-US group for next-generation telescope development Fermi -LAT : Multi-wavelength studies combining satellite and ground-based data