جستجوی استاد راهنمای دانشگاهی

Sabine Hossenfelderمشاهده پروفایل

پژوهشگر

• Quantum Foundations
• Quantum Mechanics
• Dark Matter
• +۳ مورد دیگر

Dr. Sabine Hossenfelder is a Researcher at Ludwig-Maximilians-Universität München (LMU), where she explores foundational questions in physics. She holds a PhD in Physics from the University of Frankfurt (2003) and has conducted research across particle physics, quantum gravity, dark matter, and quantum foundations. Her current work focuses on superdeterminism and locality in quantum mechanics, challenging conventional assumptions about Bell’s theorem and finetuning. Dr. Hossenfelder is also a prominent science communicator, hosting the YouTube channel “Science without the Gobbledygook” and authoring books like *Lost in Math* (2018) and *Existential Physics* (2022), which critique biases in theoretical physics and explore the philosophical dimensions of science. Her research interests include the mathematical and philosophical underpinnings of quantum mechanics, with recent emphasis on experimental tests of superdeterminism and its implications for locality. She has also contributed to astrophysics studies, such as analyzing dark matter profiles in galaxies using superfluid models. Through her writing and media work, she advocates for scientific rigor and skepticism of unfalsifiable theories.

• Astronomy
• Astrophysics
• Galaxy Dynamics
• +۵ مورد دیگر

Renzo Sancisi is a Professor at the Faculty of Science and Engineering, University of Groningen, affiliated with the Department of Astronomy. His research focuses on galaxy dynamics, dark matter distribution, and the interplay between baryonic components and galactic rotation curves, particularly in spiral and dwarf galaxies. Key Topics: Spiral galaxies, dwarf galaxies, dark matter, galaxy rotation curves, baryonic mass distribution His publications analyze the dynamics of starbursting dwarf galaxies like I Zw 18 and UGC 4483, the relationship between baryonic mass and rotation curve shapes, and the structural properties of low surface brightness galaxies. Notable collaborations include studies with F. Lelli and M. Verheijen. Email contact: r.sancisi@rug.nl .

Ivan Charles Sterlingمشاهده پروفایل

استاد

• Differential Geometry
• 3D Printing
• Mathematical Visualization
• +۳ مورد دیگر

Ivan Charles Sterling is a Professor of Mathematics at St. Mary's College of Maryland, where he has been teaching since July 2000. He earned his B.A. from the University of California at Santa Cruz in 1980 and his Ph.D. from the University of California at Berkeley in 1985. His academic career includes positions as Researcher at Max-Planck-Institut für Mathematik in Bonn (1985-1986), Visiting Lecturer at UC Santa Cruz (1986-1987), Assistant Professor at Technische Universität Berlin (1987-1991) and the University of Toledo (1991-1995), and Associate Professor at the University of Toledo (1995-2000). Professor Sterling's research focuses on differential geometry with particular emphasis on pseudospherical surfaces, minimal surfaces, and discrete curves. His work bridges theoretical mathematics with practical applications in 3D printing and geometric visualization. His teaching portfolio includes a wide range of courses from Calculus sequences to specialized topics like '3D Printing Galaxies' and '3D Printing Constant Negative Curvature Fabrics.' His publication history reveals a clear evolution from classical differential geometry toward more applied areas involving computational methods and 3D fabrication. Starting with theoretical work on minimal surfaces and pseudospherical surfaces in the 1980s-1990s, his research progressed through discrete geometry topics in the 2000s-2010s, culminating in his recent work on integrating 3D printing technology with mathematics education. This trajectory demonstrates how Sterling has successfully connected pure mathematical theory with tangible applications in visualization and digital fabrication. At St. Mary's College of Maryland, Sterling maintains an office in Schaefer Hall, Room 177, where he continues to teach undergraduate mathematics courses and conduct research that combines geometric theory with modern fabrication techniques. His work exemplifies how theoretical mathematics can find practical expression through emerging technologies.

William M. Wolfمشاهده پروفایل

دانشیار

• Stellar Astrophysics
• Novae and Supernovae
• Computational Physics
• +۲ مورد دیگر

William M. Wolf serves as Associate Professor in the Department of Physics and Astronomy within the College of Arts and Sciences at the University of Wisconsin-Eau Claire. He is affiliated with the Blugold Center for High Performance Computing and is currently on sabbatical for the 2025–2026 academic year. His educational background includes: Ph.D. in Physics, University of California, Santa Barbara M.A. in Physics, University of California, Santa Barbara B.S. in Physics, Eastern Illinois University B.A. in Mathematics, Eastern Illinois University Wolf specializes in computational stellar astrophysics, particularly modeling classical and recurrent novae through thermonuclear runaway simulations. His research leverages the open-source MESA software framework to investigate white dwarf evolution, supernova progenitors, and galactic chemical enrichment. As a core MESA developer, he bridges theoretical modeling with observational astronomy to explain transient phenomena visible across galaxies. Analysis of his 12 publications (2014–2023) reveals consistent focus on stellar evolution codes, nova/supernova mechanisms, and white dwarf physics. Key trends include MESA code development for pulsating stars and convection modeling, plus observational studies of supersoft X-ray sources and recurrent novae. His work increasingly integrates multi-wavelength data with high-performance computing. Major recognitions include: NSF CAREER Award (2023): $526,813 for "Mixing and Oscillations in Novae" NASA Astrophysics Theory Program Grant (2024): $423,518 as Co-Investigator for "A New Paradigm for Supersoft X-ray Oscillations of Novae" Wolf mentors students in computational astrophysics projects using campus high-performance resources. His grant portfolio exceeds $950,000, supporting research on nova oscillations and supersoft source modeling. Future work targets MESA enhancements for supernova progenitor studies and recurrent nova recurrence mechanisms. He actively contributes to the international MESA developer team and collaborates on multi-institutional projects studying white dwarf binaries and transient events through facilities like Swift and iPTF.

Donald Terndrupمشاهده پروفایل

دانشیار

• Angular Momentum Evolution in Stars
• Star Clusters
• Stellar Populations
• +۳ مورد دیگر

Donald Terndrup is an Associate Professor of Astronomy at The Ohio State University, specializing in observational astronomy with a focus on stellar populations, quasar winds, and galactic evolution. He joined the faculty in 1990 and has contributed extensively to studies of quasar outflows and their impact on galaxy formation. His research bridges stellar astrophysics and extragalactic phenomena, particularly examining angular momentum evolution in stars and the structure of the Galactic bulge. Education: Ph.D. in Astronomy & Astrophysics from UC Santa Cruz (1986), A.B. in Physics and Astronomy from UC Berkeley (1981). He served as Program Director in the Division of Astronomical Sciences at the National Science Foundation (2008–2012), emphasizing his leadership in astronomical research policy. Courses taught include Astronomy 3350 (Methods of Astronomical Observation) and Astronomy 1221 (Astronomy Data Analysis). Research Interests: Terndrup’s work centers on quasar winds and feedback mechanisms, using multi-wavelength observations and spectral synthesis techniques. He investigates how outflows from active galactic nuclei influence galaxy evolution, with recent focus on iron low-ionization broad absorption-line (FeLoBAL) quasars. His studies employ advanced tools like SimBAL simulations to model outflow dynamics and energetics. Articles Trends: His publications (2020–2024) emphasize quasar outflow physics, including geometric modeling, spectral variability analysis, and connections between accretion processes and radiation-driven winds. Collaborations span institutions worldwide, addressing topics like γ-ray novae and stellar rotation in the Kepler field. Grants & Advising: Funded by NSF grants such as the Collaborative Research on BAL quasar spectral synthesis (2020). Advises graduate students on AGN feedback projects and undergraduate research through initiatives like 'Quasar Outflows for Undergraduates and Everyone.' Labs/Teams: Active in collaborative projects such as the 4MOST-Gaia Quasar Survey and Dragonfly Galaxy studies, focusing on high-redshift galaxy mergers and radio jet interactions.

Lawrence Widrowمشاهده پروفایل

استاد

• Galactic Dynamics
• Dark Matter
• Cosmology
• +۲ مورد دیگر

Lawrence Widrow is a Professor in the Department of Physics, Engineering Physics & Astronomy at Queen's University, where he leads research in theoretical astrophysics and cosmology. He earned his PhD from the University of Chicago under Michael Turner and held postdoctoral positions at Harvard-Smithsonian Center for Astrophysics and Canadian Institute for Theoretical Astrophysics. Research focuses on galactic dynamics, dark matter, and cosmic structure formation. Key contributions include: Galactoseismology (studying galactic disk perturbations via SEGUE/Gaia data), equilibrium modeling of the Milky Way, orbital torus imaging techniques, dark matter substructure analysis, and simulations of disk-halo interactions. Recent work explores pulsar-based dark matter detection, phase mixing theory, and fuzzy dark matter dynamics. Methodological innovations include the GalactICS code for equilibrium initial conditions, discrete spectral analysis of phase space, and MilkyWay@home distributed computing for stream reconstruction. No scientific awards, students, or laboratory affiliations are detailed in the provided information.

Anna Mooreمشاهده پروفایل

استاد

• Astronomy
• Astrophysics
• Space Instrumentation
• +۳ مورد دیگر

Professor Anna Moore is a prominent academic and researcher in Astronomy & Astrophysics at the Australian National University (ANU). She holds dual roles as Director of the ANU Institute for Space and Director of the Advanced Instrumentation and Technology Centre at Mount Stromlo Observatories. Her research focuses on space and ground-based instrumentation, including the Palomar Gattini-IR survey and DREAMS telescope projects. She contributed to the formation of the Australian Space Agency as a member of the Space Expert Reference Group (2018). Her work emphasizes infrared transient detection, stellar astrophysics, and instrumentation development. Key projects include the Palomar Gattini-IR survey for near-infrared transients and the DREAMS telescope for Antarctic-based wide-field astronomy. Recent research includes studies of Be stars in X-ray binaries, supernova progenitors, and Galactic novae. Moore’s publications span over a decade, addressing topics like Lyman-α emission in cosmic structures, multi-messenger astronomy, and instrumentation challenges. She has pioneered methods to uncover optically obscured Galactic novae and symbiotic stars using near-infrared data. Her professional service includes leadership in Australian space initiatives and academic instrumentation. The Advanced Instrumentation Technology Centre (AITC), under her directorship, develops cutting-edge tools for astrophysical research despite operational challenges posed by environmental and pandemic disruptions.

• Galaxy Evolution
• Astrophysics
• Dark Matter
• +۳ مورد دیگر

Erwin de Blok is a Professor at the University of Groningen's Faculty of Science and Engineering, affiliated with the Kapteyn Astronomical Institute. He holds an honorary chair in the Structure and Evolution of Nearby Galaxies. His research focuses on galaxy dynamics, HI surveys, and extragalactic astronomy, with notable contributions to projects like MHONGOOSE and MeerKAT. He is also a Research Scientist at ASTRON, the Netherlands Institute for Radio Astronomy. Research Interests: Prof. de Blok explores galactic evolution, HI gas distribution, and dark matter's role in galaxy formation. His work emphasizes large-scale surveys like MHONGOOSE, which uses MeerKAT to study nearby galaxies' neutral hydrogen content. Key themes include circumgalactic medium dynamics, star formation triggers, and the interplay between gas and stellar components in galaxies. Publications: His recent work includes HI surveys revealing extraplanar gas structures and analyzing TNG50 cosmological simulations. Articles highlight transient detection methods and molecular gas fraction studies in spiral galaxies. Awards & Grants: No specific awards listed, but his extensive research collaborations and high-impact publications reflect sustained academic excellence. He contributes to international projects like PHANGS and TYPHOON, leveraging advanced radio telescope infrastructure. Labs & Teams: Active in the Kapteyn Astronomical Institute and ASTRON, focusing on HI surveys and radio astronomy innovations. His work bridges observational data with theoretical models to advance understanding of galactic evolution and structure.

• Dark Matter
• Stellar Streams
• Galactic Dynamics
• +۳ مورد دیگر

Nathaniel Starkman is a Brinson Prize Fellow and Astrophysics Postdoc at MIT. He is a key maintainer for open-source projects including @astropy , @GalacticDynamics , and @cosmology-api , with over 2,500 GitHub contributions in the last year. His work focuses on dark matter detection, stellar stream dynamics, and computational astrophysics using JAX and differentiable simulations. Current affiliations: MIT, GalacticDynamics, cosmology-api Former affiliations: Astropy Project, Quax, Potamides Research interests span dark matter substructure mapping via stellar streams, Hamiltonian perturbation theory applications, and JAX-based galactic dynamics tools. He develops unit-aware numerical frameworks (unxt, coordinax) and contributes to astronomical data infrastructure standards. Scientific contributions include: Leading differentiable simulations for galactic potentials Creating data-driven stellar stream characterization methods Advancing type annotations in astropy Awards: Brinson Prize Fellowship (MIT) Contact: starkman@mit.edu | ORCiD

Hamid Ait Abderrahmaneمشاهده پروفایل

دانشیار

• Fluid Mechanics
• Fluid-Structure Interaction
• Hydrodynamic Stability
• +۸ مورد دیگر

Dr. Hamid Ait Abderrahmane is an Associate Professor in the Department of Mechanical & Nuclear Engineering at Khalifa University. His research spans fluid mechanics, fluid-structure interactions, and hydrodynamic instabilities, with applications across multiple industries including renewable energy, oil and gas, aerospace, and biomedical fields. Education: PhD in Mechanical Engineering, Concordia University (Canada), 2009 Dr. Ait Abderrahmane's research focuses on tackling fundamental fluid dynamics problems through experimental, mathematical, and numerical approaches. His work centers on four key areas: fluid-structure interactions, swirling flows, interfacial flows, and multiphase flows in porous media. He has recently expanded his expertise into data-driven modeling and machine learning applications for fluid dynamics, developing methods to discover physical laws from observational data. His research approach involves synthesizing problems into canonical forms and iterating between experiment and theory to unravel physical system dynamics. Dr. Ait Abderrahmane has published over 50 research papers in top journals including Physical Review Letters, Journal of Fluid Mechanics, Physics of Fluids, and Physical Review E, plus 50+ conference proceedings. His work demonstrates consistent excellence in fluid dynamics research with emphasis on both theoretical foundations and practical applications. He has received several prestigious awards including two Postdoctoral Scholarships in Canada and Quebec, recognition as one of the top 10 discoveries of 2009 by Quebec Science Magazine, and the Milton Van Dyke Award for Gallery of Fluid Motion in 2010. Dr. Ait Abderrahmane currently supervises multiple graduate students including PhD candidates Ramanzani S. Kalule and Yuxi Zang, and Master's students Antim Gupta and Shaikh Abdullah Rais Ahmed Shaikh Rais Ahmed Shaikh. He teaches advanced courses including Advanced Fluid Mechanics, Computational Methods for Mechanical Engineers, Finite Element Analysis, and Introduction to Hydrodynamic Stability. His laboratory conducts cutting-edge research on point vortices, tornado modeling, galaxy rotational curve experiments, and AI/ML approaches to discovering physical laws. The lab utilizes spectral analysis techniques including proper orthogonal and dynamical mode decomposition, finite-time Lyapunov exponent analysis, and Poincaré map techniques for flow visualization and mixing analysis.

Ricardo Floresمشاهده پروفایل

استاد

• Astrophysical Cosmology
• Quantum Field Theory
• Particle Physics
• +۳ مورد دیگر

Ricardo Flores is a Professor in the Department of Mathematics, Physics, Astronomy and Statistics at the University of Missouri-St. Louis, specializing in astrophysical cosmology and particle physics with emphasis on dark matter halos, galaxy clusters, and gravitational phenomena. Education: PhD (1984) - Thesis on Higgs bosons His research integrates cosmological simulations with multi-wavelength observations to study dark matter distribution, cluster dynamics, and cosmological parameters. Key focus areas include gravitational lensing shear maps, Sunyaev-Zel'dovich effect evolution, and Cold Dark Matter cosmology validation through X-ray and simulation comparisons. His work bridges theoretical particle physics with observational astrophysics, particularly in supersymmetric field theories and large-scale structure formation. Publication trends from 1996-2007 reveal consistent focus on dark matter halo properties across cosmic epochs, cluster merger dynamics, and gravitational lensing applications. These studies predominantly utilize data from The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society, demonstrating methodological evolution from analytical predictions to advanced simulation-observation comparisons. No specific scientific awards or honors are documented in the provided materials. Dr. Flores actively mentors graduate students on gravitational-lensing simulations and Sunyaev-Zel'dovich effect modeling, with research sustained through: National Science Foundation grants University of Missouri System Research Board funding UM-St. Louis Research Awards He maintains extensive international collaborations across cosmological research networks, coordinating long-term projects on cluster physics and simulation-observation integration without dedicated institutional lab facilities.

• Astrophysics
• Galaxy Evolution
• Artificial Intelligence in Astronomy
• +۱ مورد دیگر

Dr. John Stott is a Senior Lecturer in Astrophysics at the Physics Department, Lancaster University . His research focuses on galaxy evolution in dense environments, particularly the transformation of star-forming galaxies in galaxy clusters, and the application of artificial intelligence to astronomical data analysis. Current projects: LSST: UK Data Release Processing , ICECOMM: AI for Iceberg Detection Key collaborations: Data Science Institute , Observational Astrophysics Group Research Interests include: Galaxy quenching mechanisms in massive clusters Environmental effects on galaxy formation AI applications in astronomy and maritime safety Multi-telescope observational campaigns (Hubble, James Webb, LSST) Recent Publications highlight studies of: High-redshift emission-line galaxies Environmental quenching in cosmic filaments Galaxy cluster scaling relations Deep learning for astrophysical data analysis

Simon Mittonمشاهده پروفایل

استاد

• History of Astronomical Sciences
• Relativistic Cosmology
• History of Cosmology
• +۳ مورد دیگر

Simon Mitton is a Life Fellow at St Edmund's College and Professor in the Department of History and Philosophy of Science at the University of Cambridge. He is a leading scholar in the history of astronomical sciences and cosmology, focusing on 19th-20th century developments. His research explores controversies in cosmology, pioneers like Einstein and Hoyle, and the history of deep carbon science. He holds fellowships with the Royal Astronomical Society, Geological Society, and Royal Historical Society. Research Interests: Mitton’s work bridges history and science, examining how conflicts shaped cosmology. Key topics include relativistic cosmology’s evolution, the role of figures like Lemaître and Gamow, and the discovery of Earth’s deep carbon systems. His books, such as Vera Rubin, a Life and From Crust to Core , showcase interdisciplinary approaches to scientific biography and geochemical history. Publications & Lectures: Mitton has authored over 20 books and numerous articles. Recent works analyze the Big Bang-Steady State debate and deep carbon science’s 500-year history. He frequently lectures at institutions like the Royal Astronomical Society and international cruises, emphasizing science communication and historical narratives. Awards: His contributions earned recognition through fellowships in learned societies and honorary roles. He has been a Visiting Scholar at multiple institutions, reflecting his global impact in science history.

• Galaxy Formation and Evolution
• Circumgalactic Medium (CGM)
• Quasar Absorption Spectroscopy
• +۴ مورد دیگر

Prof. Glenn Kacprzak is a Professor at Swinburne University's Centre for Astrophysics and Supercomputing, specializing in galaxy formation and evolution. He uses quasar absorption spectroscopy to study circumgalactic medium (CGM) dynamics, particularly focusing on gas inflows/outflows and their role in galactic evolution. His research integrates gravitational lensing techniques and high-resolution imaging to explore galaxy evolution at cosmological scales. Affiliations: Swinburne University of Technology Key Roles: Interim Director (2019-2020), ARC Centre of Excellence Participation His research interests span quasar absorption line studies , CGM kinematics , and high-redshift galaxy evolution . He employs Hubble, JWST, and ground-based telescopes to analyze galactic winds, inflows, and AGN feedback mechanisms. Recent work includes detecting gas inflows in starbursting galaxies and mapping cool gas around quiescent systems using gravitational lensing. Publications highlight advancements in understanding outflow mass loading, AGN fractions in massive galaxies, and the role of mergers in shaping CGM complexity. His work bridges observational data with cosmological simulations, addressing discrepancies in galaxy evolution models. Awards: ARC Fellowships (2014, 2011), Vice-Chancellor's Research Excellence Awards (2020, 2016) Grants: ARC Centre of Excellence (2017-2024), Physics of Gas Flows around Galaxies (2017-2021) Prof. Kacprzak supervises PhD students in topics like gravitational lensing applications, baryon cycle dynamics, and CGM-environment interactions. His laboratory focuses on multi-wavelength observational astronomy and computational modeling of galactic-scale processes.

• Galaxy Dynamics
• Astrophysics
• Astronomy
• +۶ مورد دیگر

Marc S Seigar is the Dean of the College of Natural Sciences and Mathematics at The University of Toledo, effective August 2021. He holds a B.Sc. in Physics from Imperial College London (1993) and a Ph.D. in Astrophysics from Liverpool Astrophysics Research Institute (1998). Prior roles include tenure-track faculty at the University of Arkansas, Head of Physics & Astronomy at the University of Minnesota Duluth, and Associate Dean at Swenson College of Science & Engineering. From 2020–2021, he served as Program Director at the National Science Foundation’s Division of Astronomical Sciences. His research focuses on astronomy and astrophysics, particularly galaxy dynamics, structure, and morphology. He has utilized data from major observatories like the Hubble Space Telescope, Spitzer, and Kitt Peak. Key interests include supermassive black hole-galaxy connections, dark matter halo profiles, and spiral arm pitch angle correlations. Publications span topics such as black hole mass functions, galaxy evolution, and morphological analysis. While no scientific awards are explicitly listed, his extensive academic contributions reflect significant scholarly impact. No grants or student advisement data are included in the provided text.