جستجوی استاد راهنمای دانشگاهی

Andreas Görgenمشاهده پروفایل

استاد

• experimental nuclear physics
• nuclear structure
• nuclear reactions
• +۲ مورد دیگر

Andreas Görgen is a Professor in the Department of Physics at the University of Oslo, Norway, specializing in experimental nuclear physics. He has held this position since 2012, following an Associate Professorship at the same institution from 2010 to 2012. His prior experience includes a Staff Scientist role at CEA Saclay (2002-2010) and a Postdoctoral Fellowship at Lawrence Berkeley National Laboratory (2000-2002). His educational background is rooted at the Universität Bonn, where he earned his Diplom-Physiker in 1996 and Dr. rer. nat. in 2000. During his doctoral studies, he served as a Research Assistant at the Institut für Strahlen- und Kernphysik. Görgen's research centers on experimental nuclear physics, with a focus on nuclear structure, nuclear reactions, exotic nuclei, and resonances in atomic nuclei. He employs advanced techniques such as Coulomb excitation, in-beam spectroscopy, and gamma-ray spectroscopy to investigate nuclear shapes, shell evolution, and the properties of nuclei far from stability. Analysis of his recent publications (2016-2023) reveals a consistent emphasis on nuclear structure phenomena, particularly shape coexistence in neutron-rich isotopes (e.g., Sr, Zr, Sm), shell evolution near 78Ni, and the spectroscopy of exotic copper isotopes. His work also spans nuclear astrophysics (e.g., the Hoyle state in carbon-12) and medical physics applications (e.g., proton-dynamic therapy). No scientific awards were mentioned in the provided text. Details regarding student advising and research grants were not specified in the available information. However, Görgen is a key member of the Oslo Cyclotron Laboratory (OCL) team and maintains active collaborations with CERN/ISOLDE and GANIL/SPIRAL2, contributing to international nuclear physics research efforts. Görgen's primary research facility is the Oslo Cyclotron Laboratory (OCL), which provides experimental capabilities for nuclear structure studies using radioactive ion beams. His collaborative network extends to major European facilities, enhancing the scope and impact of his research program in fundamental and applied nuclear physics.

Michael Klasenمشاهده پروفایل

استاد

• Particle Physics
• Quantum Chromodynamics
• Physics beyond the Standard Model
• +۳ مورد دیگر

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.

Jay Straderمشاهده پروفایل

استاد

• Compact Objects
• Black Holes
• Neutron Stars
• +۵ مورد دیگر

Jay Strader is a Professor in the Department of Physics and Astronomy at Michigan State University, where he serves as Graduate Director for the astronomy PhD program and Associate Chair for astronomy. His research focuses on compact objects, particularly black holes and neutron stars in globular clusters, neutron star binaries in Fermi gamma-ray sources, and intermediate-mass black holes. He has received a Packard Fellowship for Science and Engineering and grants from NSF and NASA. His research group includes postdoc Ryan Urquhart, graduate students Thomas Do and Rebecca Kyer, and several undergraduates, with past students like Teresa Panurach (now director of NoVEL Consortium) and Samuel Swihart (NRC fellow at Naval Research Lab). Education: PhD in Astronomy, UC-Santa Cruz/Lick Observatory Awards: Packard Fellowship Collaborations: Member of Rubin Observatory's Stars, Milky Way, and Local Volume science collaboration since 2008 Previous Positions: Hubble Fellow and Menzel Fellow at Harvard-Smithsonian Center for Astrophysics (2007-2012) Program Initiatives: Co-founder of PAREDS program for early research opportunities at MSU His work has been supported by NSF and NASA grants, and he has contributed to studies on black holes in M22, hypervelocity globular clusters around M87, and transitional millisecond pulsars. His group collaborates with Laura Chomiuk and contributes to data catalogs like the M31 globular cluster velocity dispersion database.

Jorge Piekarewiczمشاهده پروفایل

استاد

• Nuclear Theory
• Neutron Stars
• Dense Matter
• +۶ مورد دیگر

Prof. Jorge Piekarewicz is a Professor of Physics at Florida State University (FSU), affiliated with the College of Arts and Sciences. He earned his Ph.D. in theoretical nuclear physics from the University of Pennsylvania in 1985, followed by postdoctoral research at Caltech and Indiana University. Since 1990, he has been a faculty member at FSU. Education: Ph.D. in Theoretical Nuclear Physics, University of Pennsylvania (1985) Postdoctoral Fellowships: California Institute of Technology and Indiana University Research Interests: His work focuses on extreme-density nuclear matter in neutron stars, bridging terrestrial experiments and astrophysical observations. Key areas include: Neutron star structure and equation of state Weak interaction probes (e.g., parity-violating electron scattering) Multi-messenger astronomy insights from neutron star mergers Covariant energy density functionals and symmetry energy constraints Articles Trends: Recent work emphasizes refining the nuclear equation of state using PREX-CREX experiments, gravitational wave data (e.g., GW170817), and Bayesian methods. Key themes include neutron skin thickness, crust-core interactions, and symmetry energy sensitivity. Service & Outreach: Nuclear Science Advisory Committee (2012–2015) FRIB Theory Alliance Director (2017–2021) INT National Advisory Committee Chair (2018–2020) OLLI Lecturer on stellar evolution and neutron stars Collaborations: Active involvement with CERN, FRIB, JLab, and the Facility for Rare Isotope Beams (FRIB). Research leverages facilities like the Relativistic Heavy Ion Collider and the National Superconducting Cyclotron Laboratory.

Imre Bartosمشاهده پروفایل

دانشیار

• Multi-messenger Astrophysics
• Black Hole Mergers
• Gravitational Waves
• +۲ مورد دیگر

Imre Bartos is an Associate Professor of Physics at the University of Florida, specializing in multi-messenger astrophysics that combines gravitational waves, neutrinos, and electromagnetic signals. His research investigates extreme cosmic explosions involving black holes and neutron stars, with emphasis on merger environments in active galactic nuclei. Groundbreaking work includes demonstrating how nearby neutron star mergers influenced Solar System composition, identifying AGN disks as factories for eccentric black hole mergers, and developing techniques to probe black hole origins through gravitational wave localization. His group participates in major collaborations including LIGO, LISA, and IceCube observatories. Professor Bartos received the Sloan Fellowship and shares Breakthrough Prize honors for contributions to gravitational wave astronomy. He leads observational programs using Chandra, VLA, and Fermi telescopes while mentoring students in computational astrophysics techniques.

Ann-Cecilie Larsenمشاهده پروفایل

استاد

• Nuclear Physics
• Nuclear Astrophysics
• Quantum Mechanics
• +۲ مورد دیگر

Ann-Cecilie Larsen is a Professor in Nuclear and Energy Physics at the University of Oslo, leading research in nuclear physics and astrophysics. She works with the Oslo Cyclotron Laboratory (OCL) and collaborates with institutions like Université libre de Bruxelles, Lawrence Livermore National Laboratory, and CERN's ISOLDE facility. Master of Science in Physics, University of Oslo (2002) Cand.scient. in Nuclear Physics, University of Oslo (2004) Ph.D. in Nuclear Physics, University of Oslo (2008) Her research focuses on nuclear properties at extreme temperatures, particularly level density and gamma decay functions. These studies inform astrophysical reaction rates for understanding cosmic element formation. She teaches FYS-MEK1110 - Mechanics and KJM-FYS5920 - Nuclear Measurement Methods . Recent publications analyze nuclear decay patterns in Sn isotopes, neutron interactions on 89Y, and shape coexistence in rare isotopes. Her work connects nuclear structure studies with stellar nucleosynthesis. Prize for Young Outstanding Researchers, Norwegian Research Council (2016) Fulbright Scholarship (2015) ERC Starting Grant (2015-2020) Best Poster, Zakopane Conference (2006) She holds a Research Council of Norway project (2021-2026) and has previously received personal postdoctoral funding (2011-2014). Collaborations include Facility for Rare Isotope Beams, ISOLDE@CERN, IReNA, and ChETEC-INFRA networks.

• Theoretical Particle Physics
• Nuclear Physics
• Cosmic Ray Physics
• +۷ مورد دیگر

Masatoshi Takano is a Professor at the Faculty of Science and Engineering, Waseda University, specializing in theoretical studies of nuclear physics, particle physics, and astrophysics. His work focuses on nuclear equations of state (EOS) for neutron stars and core-collapse supernovae, incorporating realistic nuclear forces like the Argonne v18 and Urbana IX potentials. He has developed variational methods with explicit energy functionals to model hyperonic nuclear matter, spin-orbit forces, and finite-temperature effects. Education : PhD in Science, Waseda University Professional Memberships : American Physical Society, Japan Physical Society Research spans neutron star structure, supernova simulations, and nuclear matter phase transitions. His recent presentations address neutrino emission rates, braking radiation in nuclear matter, and cluster variational methods. Key collaborations include H. Togashi, K. Nakazato, and K. Sumiyoshi. Scientific contributions involve refining variational energy expressions for asymmetric nuclear matter, incorporating three-body forces, and studying pion condensation effects on neutron star cooling. He has applied his EOS models to multidimensional supernova simulations and cosmic ray detector design.

Gines Martinezمشاهده پروفایل

استاد پژوهش

• Quark Gluon Plasma
• Heavy Ion Collisions
• Particle Physics
• +۴ مورد دیگر

Dr. Gines Martinez is a Director of Research at CNRS/IN2P3 and Director of SUBATECH laboratory at IMT Atlantique. His research focuses on experimental study of quark-gluon plasma using relativistic heavy ion collisions at ALICE (LHC) and PHENIX (RHIC) experiments. He teaches Experimental Physics of Strong/Weak Interactions at Université de Nantes and electromagnetism/quantum mechanics at IMT Atlantique. Research Interests: Quark-gluon plasma formation, particle production in hadronic collisions, deuteron formation mechanisms, and ultra-relativistic nuclear collisions. Recent Publications: Focus on femtoscopy, flow harmonics, and QCD phase diagram using LHC data. Research reveals insights into nucleosynthesis in hadronic collisions and QCD matter behavior under extreme conditions. Outreach: Featured in Ouest-France and El País, with seminars on physics education in prisons and schools.

• Cosmochemistry
• Presolar Grains
• Nucleosynthesis
• +۴ مورد دیگر

Sachiko Amari serves as a Research Professor of Physics in the Department of Physics at Washington University in St. Louis, where she conducts pioneering research in cosmochemistry through the McDonnell Center for the Space Sciences. Her work bridges laboratory astrophysics and planetary science, focusing on extraterrestrial materials to unravel solar system formation and stellar processes. Amari's educational foundation includes a PhD from Kobe University and both Master of Engineering and Bachelor of Engineering degrees from Waseda University in Japan. This engineering background informs her precise analytical approach to meteoritic materials. Her research centers on presolar grains—stardust formed in stellar outflows that were incorporated into primitive meteorites. Using secondary ion mass spectrometry, she analyzes isotopic ratios to investigate nucleosynthesis in stars, mixing processes in stellar ejecta, and Galactic chemical evolution. A secondary focus examines noble gas trapping mechanisms in meteorites to understand volatile origins and early solar system processes. Her work reveals how microscopic grains preserve macroscopic cosmic histories. Analysis of her recent publications shows consistent emphasis on silicon carbide and graphite presolar grains, with increasing technical sophistication in NanoSIMS analysis. Research trends include correlating multi-element isotopic systems, identifying rare stellar sources like novae, and resolving phase Q—the elusive noble gas carrier in meteorites. Her work demonstrates how laboratory studies of individual grains constrain astrophysical models. Amari leads an active research group within the McDonnell Center for the Space Sciences and collaborates on major initiatives including the Mars Sample Return Science Definition Team. She mentors graduate students in meteoritics research while developing analytical protocols for extraterrestrial material characterization. Her laboratory serves as a hub for stardust analysis, utilizing advanced mass spectrometry techniques to decode isotopic fingerprints of stellar processes.

• Dark Matter
• Particle Astrophysics
• Cosmology
• +۲ مورد دیگر

Pearl Sandick is a Professor in the Department of Physics and Astronomy and Interim Dean in the College of Science at the University of Utah. She has previously served as Associate Chair of the Department of Physics and Astronomy and Associate Dean for Faculty and Research in the College of Science. Her academic journey at the University of Utah began in 2011 as an Assistant Professor, progressing to Associate Professor in 2017, and achieving the rank of Professor in 2022. Her educational background includes: BA in Mathematics from New York University (2003) PhD in Physics from the University of Minnesota (2008) Sandick is a theoretical particle physicist whose research focuses on physics beyond the Standard Model, with particular emphasis on dark matter. Her work spans theoretical modeling, connections to astrophysical observations, and implications for experimental detection. She investigates various dark matter candidates and their potential signatures in current and future experiments, including collider searches, direct detection experiments, and indirect detection through astrophysical observations. Her research also extends to connections between particle physics and cosmology, including early universe phenomena and implications for cosmic structure formation. She has developed computational tools like MADHAT for dark matter analysis and has made significant contributions to understanding how stellar evolution can constrain axion physics. Her scholarly contributions have been recognized with several prestigious awards: University of Utah Early Career Teaching Award (2016) University of Utah Distinguished Mentor Award Linda K. Amos Award for Distinguished Service to Women University of Utah Presidential Scholar Sandick has been actively involved in mentoring graduate students, as evidenced by her teaching of PhD thesis research and Master's research courses. She has secured significant research funding from the National Science Foundation and other agencies to support her work on dark matter, dark energy, and new physics. Her grant portfolio includes projects on theoretical particle physics, connections to astrophysical observations, and studies on graduate education reform following a departmental tragedy. She is an active member of the American Physical Society, having served as Chair of the regional Four Corners Section in 2021-2022, demonstrating her commitment to the broader physics community and leadership in her field.

Malcolm Fairbairnمشاهده پروفایل

استاد

• Dark Matter
• Dark Energy
• Cosmological Inflation
• +۳ مورد دیگر

Professor Malcolm Fairbairn is a faculty member at King's College London's Department of Physics, part of the Faculty of Natural, Mathematical & Engineering Sciences. His research focuses on the intersection of cosmology, particle physics, and astrophysics, particularly dark matter, dark energy, and cosmological inflation. He leads projects like the ERC Consolidator Grant (2015–2020) investigating dark matter in the early Universe. He collaborates with initiatives such as the MoEDAL experiment at CERN (magnetic monopole searches) and the Cherenkov Telescope Array (CTA) for gamma-ray astronomy. His interests extend to gravitational waves, supermassive black hole formation, and particle astrophysics. Fairbairn has contributed to studies on axion dark matter, primordial black holes, and dark matter constraints from dwarf galaxies. He is affiliated with the Theoretical Particle Physics & Cosmology (TPPC) Group, exploring beyond-Standard-Model physics, including supersymmetry and extra dimensions. Publications span topics like dark matter relic abundance, JWST observations of black holes, and LHC searches for exotic particles. He has advised on outreach projects like the 'Dark Matter' exhibition at Science Gallery London and interviews with alumni (e.g., Royal Navy submariner Chris Tuckley).

Witold Nazarewiczمشاهده پروفایل

استاد

• Theoretical Nuclear Physics
• Nuclear Structure
• Quantum Many-Body Problem
• +۷ مورد دیگر

Witold "Witek" Nazarewicz is a John A. Hannah Distinguished Professor in the Department of Physics & Astronomy at Michigan State University and serves as the Chief Scientist at the Facility for Rare Isotope Beams (FRIB). He is also a Corporate Fellow Emeritus at Oak Ridge National Laboratory (ORNL) and maintains a professorship at Warsaw University, Poland. Nazarewicz previously held positions as James McConnell Distinguished Professor at the University of Tennessee and served as Scientific Director of ORNL's Holifield Radioactive Ion Beam Facility from 1999-2012. His academic career spans multiple international institutions including Lund University, University of Cologne, Kyoto University, University of Liverpool, and Peking University. Nazarewicz's research focuses on theoretical nuclear physics with particular emphasis on exotic nuclei at the limits of nuclear existence. His work spans quantum many-body problems, physics of open quantum systems, superheavy elements, and nuclear fission. He has pioneered approaches to unify structure and reaction aspects of nuclei based on open quantum system many-body formalism, including the Gamow Shell Model. His research connects nuclear physics with high-performance computing, developing comprehensive descriptions of all nuclei through theoretical and experimental investigations of rare atomic nuclei. An analysis of Nazarewicz's recent publications reveals a strong focus on cutting-edge nuclear structure research, particularly concerning exotic nuclei near the driplines, charge radii measurements, superheavy elements, and the development of advanced computational methods. His work increasingly incorporates machine learning and Bayesian analysis techniques to address nuclear physics challenges. The publications demonstrate his leadership in connecting fundamental nuclear physics with applications in nuclear astrophysics, while also addressing foundational questions about the limits of nuclear existence and the nature of nuclear forces. Fellow of the American Physical Society Fellow of the U.K. Institute of Physics Fellow of the American Association for the Advancement of Science 2008 Carnegie Centenary Professor Honorary Doctorates from University of the West of Scotland (2009) and University of York (2019) 2012 Tom W. Bonner Prize in Nuclear Physics 2012 ORNL Distinguished Scientist 2013 UT-Battelle Corporate Fellow 2017 G.N. Flerov Prize 2025 Marian Smoluchowski Medal Nazarewicz has authored approximately 500 peer-reviewed publications with over 37,000 citations and an h-index of 103 (Web of Science). He has delivered over 220 invited talks at major international conferences and organized approximately 70 scientific meetings. His research has been supported by numerous grants from the Department of Energy, National Science Foundation, and international funding agencies. Nazarewicz plays a leadership role in major nuclear physics initiatives including the UNEDF, NUCLEI, and BAND collaborations, and has contributed to several National Academies reports on nuclear physics. As FRIB Chief Scientist, Nazarewicz leads theoretical efforts at one of the world's premier facilities for rare isotope research. His research group at MSU collaborates extensively with experimentalists worldwide, bridging theoretical predictions with cutting-edge measurements. He directs the FRIB Theory Alliance, fostering international collaboration in nuclear theory, and has established strong connections between nuclear physics and other disciplines including quantum information science and machine learning.

Sumit Saxenaمشاهده پروفایل

استاد

• First principles calculations
• Electronic structure of materials
• Graphene and 2D materials
• +۶ مورد دیگر

Dr. Sumit Saxena is a Professor in the Department of Metallurgical Engineering and Materials Science (MEMS) at the Indian Institute of Technology Bombay (IIT Bombay), India. He leads the NEMO Laboratory, which focuses on multifaceted research combining experimental and theoretical approaches in materials science and metastructures. His academic affiliations include IIT Bombay, where he has progressed from Assistant Professor (2012) to Associate Professor (2016) and Professor (2021). His research interests span first-principles calculations of electronic structure , graphene and 2D materials , metamaterial design and fabrication , and novel materials for energy storage . These areas are supported by both computational modeling and experimental synthesis. The recent publications reflect a strong trend in 2D materials , particularly graphene and its derivatives, with a focus on electronic and structural properties using density functional theory . Additional themes include carbon-based nanostructures , sol-gel synthesis of functional oxides , and even nuclear mass measurements from earlier work. The research bridges fundamental physics with applications in energy and sustainability. Scientific recognitions include: Fellow of the Institute of Materials, Minerals and Mining (FIMMM), UK Fellow of the National Environmental Science Academy (FNESA), India Fellow of the Royal Society of Chemistry (FRSC), London Member of the Materials Research Society India (MRSI) Dr. Saxena supervises multiple PhD and research scholars, particularly in the NEMO Lab and IITB-Monash Research Academy. His research is supported by projects on 2D material synthesis , metamaterial fabrication , and energy storage materials . He holds patents in areas such as achromatic microlenses and carbon-based desalination membranes . He collaborates with researchers at Harvard, UIUC, and Monash University, and is involved in water technology initiatives through WICTRE at IIT Bombay. He leads the NEMO Laboratory, a multidisciplinary research group working on nano-bio systems, photonics, and environmental applications of nanomaterials. The lab supports graduate students, postdoctoral fellows, and project staff working on topics ranging from optical sensors to water purification.

Brian Appelbeمشاهده پروفایل

پژوهشگر ارشد

• Inertial Confinement Fusion (ICF)
• Nuclear Physics
• Plasma Physics
• +۴ مورد دیگر

Brian Appelbe is a Research Fellow in the Department of Physics at Imperial College London, affiliated with the Centre for Inertial Fusion Studies (CIFS), Plasma Physics Group, and the Faculty of Natural Sciences. His research focuses on inertial confinement fusion (ICF) and high-energy-density physics, particularly nuclear processes in ICF plasmas, neutron production, and plasma-plasma interactions. He explores applications of ICF experiments to stellar nucleosynthesis and quantum computing in plasma physics. Research topics include measuring neutron capture cross sections in excited states, optimizing neutron sources, and leveraging quantum computing for plasma modeling. He collaborates on projects at facilities like the National Ignition Facility (NIF) and Omega laser, investigating magnetic field effects in plasma dynamics and burn propagation mechanisms. His work addresses challenges like plasma temperature/density measurement, magnetic field transport in burning plasmas, and mitigating hydrodynamic instabilities. Recent articles highlight advancements in neutron spectroscopy, magnetized implosion performance, and diagnostic innovations bridging magnetic and inertial confinement fusion. Despite no listed awards, his contributions to CIFS and plasma physics research are significant. He advises on experimental platforms for magnetized implosions and explores multi-disciplinary applications of ICF diagnostics. Labs/teams include the Plasma Physics Group and CIFS, advancing ICF theory and experimental techniques.

• Astrophysical Fluid Dynamics
• Star Formation
• Protostellar Disks
• +۷ مورد دیگر

Chris Matzner is a Professor and Associate Graduate Chair at the University of Toronto's Department of Astronomy and Astrophysics, affiliated with the Dunlap Institute for Astronomy & Astrophysics. He earned his Ph.D. from UC Berkeley in 1999. His research focuses on astrophysical fluid dynamics, particularly star formation processes (protostellar disks, molecular clouds, energy feedback) and stellar explosions (supernovae, gamma-ray bursts), employing analytical, numerical, and observational approaches. His research encompasses: Dynamics of protostellar outflows and molecular cloud interactions Models for supernova shocks and gamma-ray burst mechanisms Fragmentation in star and planet formation Massive black hole accretion processes Evolution of giant molecular clouds Stellar feedback in galactic environments Analysis of his 15 most recent publications reveals strong emphasis on supernova dynamics (particularly Type Ia explosions), star formation mechanisms in clusters and molecular clouds, shock wave physics in astrophysical contexts, and the development of astronomical instrumentation. The works demonstrate consistent focus on explosive transients, fluid dynamics in cosmic environments, and observational constraints on theoretical models. As Associate Graduate Chair, he oversees academic programs and student development. His laboratory affiliations include the Dunlap Institute's computational astrophysics and instrumentation groups. Current work involves modeling star cluster-galaxy interactions, tidal disruption events, and developing next-generation UV/IR detectors.