جست‌وجوی استاد و پژوهشگر

Dragan Hutererمشاهده پروفایل

استاد

• Cosmology
• Dark Energy
• Large-Scale Structure
• +۳ مورد دیگر

Dragan Huterer is a Professor of Physics and Associate Chair for the Graduate Program at the University of Michigan. His research focuses on cosmology, particularly dark energy and large-scale structure, utilizing data from the Dark Energy Survey (DES) and the Dark Energy Spectroscopic Instrument (DESI) collaborations. He earned his Ph.D. from the University of Chicago (2001) and B.S. from MIT (1996). His work explores the nature of dark energy through cosmological probes like Type Ia supernovae, galaxy clustering, and cosmic microwave background anisotropies. Key contributions include co-leading DESI's first-year cosmological analysis, revealing unprecedented constraints on dark energy and neutrino masses. He also investigates the statistical isotropy of the universe and authored the textbook A Course in Cosmology: From Theory to Practice . Awards include the Friedrich Wilhelm Bessel Research Award (2019) and the Chambliss Astronomical Writing Award (2025). He has advised numerous graduate and undergraduate students, and his funding includes DOE, NSF, and NASA grants. Current projects include the Michigan Cosmology Summer School and leadership in the DESI Collaboration.

• Nuclear Magnetic Resonance (NMR)
• In vivo imaging
• MRI pulse sequence development
• +۷ مورد دیگر

Professor Guy Williams is a leading academic at the University of Cambridge with a focus on imaging science and clinical neurosciences, affiliated with Downing College and the Wolfson Brain Imaging Centre . Holding a PhD in Physics from his initial Natural Sciences degree, he specializes in nuclear magnetic resonance (NMR) and MRI techniques for brain imaging. Education: BA, PhD in Physics His research centers on non-invasive imaging of brain structure and function, particularly in traumatic brain injury (TBI) and dementia. His work involves developing novel MRI pulse sequences and advanced data analysis algorithms, including AI-based diagnostic tools. He leads studies on white matter integrity post-trauma, longitudinal dementia assessment, and applications of MRI in disorders of consciousness and addiction. Recent publications highlight collaborations in traumatic brain injury outcomes, AI-guided dementia prediction, and neuroimaging of post-COVID cognitive deficits. His team's work on ultra-high field laminar fMRI and distortion correction methods has advanced clinical neuroscience applications. Key techniques include diffusion tensor imaging (DTI), 7 Tesla MRI, and positron emission tomography (PET/MR). His research spans from basic NMR physics to clinical translation, with a strong emphasis on multi-site studies and real-world diagnostic implementation.

Alexandra Gadeمشاهده پروفایل

استاد

• Nuclear Physics
• Exotic Nuclei
• Nuclear Structure
• +۵ مورد دیگر

Alexandra Gade is a University Distinguished Professor at the Department of Physics and Astronomy in the College of Natural Science , Michigan State University (MSU). She serves as the FRIB Scientific Director and has held leadership roles at both the National Superconducting Cyclotron Laboratory (NSCL) and FRIB. Her research focuses on the structure of exotic nuclei using radioactive isotope beams , with expertise in Coulomb excitation and nucleon knockout reactions . Education: Ph.D. in Physics (Dr. rer. nat.), University of Köln (2002) Diploma thesis, University of Köln (1998) Vordiplom, University of Köln (1995) Her nuclear structure research investigates how neutron-proton asymmetry alters nuclear properties like deformation, excitation patterns, and shell closures. She employs advanced experimental techniques at NSCL/FRIB, including the S800 spectrograph and GRETINA/SeGA gamma-ray detectors , to study exotic nuclei across the nuclear chart. Key projects include proton/neutron removal reactions and intermediate-energy Coulomb excitation , providing insights into nuclear deformation , collective modes , and single-particle orbit modifications . Recent scientific contributions focus on high-profile FRIB experiments , triaxial nuclear shapes , and shell evolution near drip lines . Her work bridges experimental observations with nuclear theory , particularly in refining shell model calculations and reaction models for exotic systems. Scientific Awards: 2023-24 Research Leadership Award (MSU) 2020 AAAS Fellow 2018 William J. Beal Outstanding Faculty Award (MSU) 2017 NatSci Outstanding Faculty Award (MSU) 2015 Zdzislaw Szymanski Prize 2014 GENCO Membership Award (GSI) 2013 APS Fellow 2010 Thomas H. Osgood Excellence in Teaching Award (MSU) 2008 Alfred P. Sloan Fellow 2008 DOE Outstanding Junior Investigator Her research group has trained numerous PhD students and postdoctoral researchers , many of whom hold academic or national laboratory positions. Collaborations include nuclear theorists , instrumentation experts , and international facilities like CERN, Argonne, and Lawrence Livermore National Laboratory.

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.

Scott Englandمشاهده پروفایل

استاد

• Planetary Atmospheres
• Space Environment
• Atmospheric Tides
• +۳ مورد دیگر

Scott England is a Professor in the Department of Aerospace and Ocean Engineering at the College of Engineering, Virginia Polytechnic Institute and State University. He serves as the Project Scientist for NASA’s Ionospheric Connection Explorer (ICON), Co-Investigator for Global-scale Observations of the Limb and Disk (GOLD), and Participating Scientist for Mars Atmosphere and Volatile Evolution (MAVEN). Education PhD, University of Leicester (UK), 2005 MPhys First Class Honors, University of Leicester (UK), 2001 England’s research focuses on planetary atmosphere-space environment interactions, particularly gravity waves, atmospheric tides, and ionosphere-thermosphere coupling on Earth and Mars. His work integrates NASA mission data (ICON, GOLD, MAVEN) with numerical modeling to study thermal dynamics, wind systems, and solar flare impacts. Recent publications highlight his expertise in thermospheric gravity wave science, planetary wave-induced ionospheric variability, and Mars atmosphere studies using EMUS and IUVS instruments. Articles span topics like Seasonal variability of DE3/DE2 tides , Transient Martian hot oxygen corona , and Shock-induced plasma dynamics . Scientific Honors 2020 Dean's Award for Teaching Excellence 2016 RHG Exceptional Achievement for Mars Science As a professional leader, England served as Thermospheric Lead for the 2019 Planetary Mission Concept Studies Program and on the National Academy of Sciences Decadal Survey panel. He manages Virginia Tech’s participation in the Virginia Space Grant Consortium and has contributed to high-performance computing committees.

Dan McCammonمشاهده پروفایل

استاد

• X-ray Astronomy
• Astrophysics
• Diffuse X-ray Background
• +۵ مورد دیگر

Dan McCammon is a Professor in the Department of Physics at the University of Wisconsin-Madison, affiliated with the College of Letters & Science. His research focuses on X-ray astronomy, including studies of the diffuse X-ray background, interstellar and intergalactic media, and the development of advanced X-ray instrumentation. He is a key contributor to the XRISM (X-ray Imaging and Spectroscopy Mission) satellite, leading efforts in high-resolution X-ray spectroscopy and mission operations. McCammon's work emphasizes understanding cosmic plasma dynamics, galaxy cluster physics, and supernova remnant evolution through cutting-edge observational techniques and detector technology. His research interests span multiple subfields, including the thermodynamic properties of galactic clusters, charge-exchange processes in astrophysical plasmas, and the design of cryogenic microcalorimeters for space-based observatories. He has pioneered advancements in transition-edge sensors (TES) and superconducting detectors, enhancing the precision of X-ray spectral measurements. McCammon has contributed to numerous sounding rocket missions, such as Micro-X, and has been instrumental in the development of the Line Emission Mapper (LEM) probe concept, aimed at mapping the soft X-ray sky with unprecedented resolution. His work on the Hitomi (ASTRO-H) satellite demonstrated breakthroughs in resolving the thermal and dynamic properties of cosmic plasmas, such as the Perseus galaxy cluster and the Crab Nebula. His publications highlight a focus on high-resolution X-ray spectroscopy of cosmic sources, including galaxy clusters, active galactic nuclei, and supernova remnants. He has explored topics like non-thermal pressure contributions in cluster cores, ionized plasma diagnostics, and the role of charge-exchange emissions in interpreting diffuse X-ray backgrounds. McCammon's instrumentation innovations have enabled breakthroughs in measuring spectral features with sub-eV resolution, advancing our understanding of astrophysical processes. Despite the absence of explicitly listed awards or grants in the provided text, his leadership in major space missions and pioneering detector technologies underscores his contributions to the field. His research team collaborates on international projects, such as XRISM and LEM, reflecting a commitment to advancing observational astrophysics through interdisciplinary collaboration.

Carsten Rottمشاهده پروفایل

استاد

• Particle Physics
• Astrophysics
• Neutrino Physics
• +۵ مورد دیگر

Carsten Rott is a Professor in the Department of Physics & Astronomy at the University of Utah and holds the Jack W. Keuffel Memorial Chair until December 2025. His academic journey began with a Ph.D. in Physics from Purdue University (2004), preceded by undergraduate studies at the Universität Hannover. Rott has held academic positions at institutions including The Ohio State University (CCAPP Senior Fellow 2009-2013), Penn State University (postdoc 2005-2008), and Sungkyunkwan University in South Korea (Assistant Professor 2013-2017, Associate Professor 2017-2025). He has been a member of the IceCube Neutrino Telescope collaboration since 2005 and serves on committees like the IceCube-Gen2 Coordination Committee and JSNS2 Speakers Board. His research spans Particle Physics , Neutrino Astronomy , and Dark Matter Detection . Key projects include analyzing IceCube data for sterile neutrino signatures, studying cosmic-ray anisotropy, and investigating terrestrial gamma-ray flashes. Notable achievements include the Bruno Rossi Prize (2021) for high-energy astrophysics contributions. Rott's work involves multimessenger observations (neutrinos, gamma-rays, radio signals) and detector calibration innovations, such as those for the JSNS2 experiment. Recent publications focus on atmospheric neutrino oscillation parameters, TGF spectroscopy, and dark matter constraints. He employs machine learning techniques (CNNs) for event reconstruction and leads initiatives like the IceCube Master Class for student engagement. Grants include funding for IceCube upgrades (2024-2026) and Hyper-Kamiokande collaborations (2023-2026). As department chair since 2023, Rott continues to bridge experimental particle physics with astrophysical discoveries.

John Martinمشاهده پروفایل

دانشیار

• Stellar Astrophysics
• Massive Stars
• Luminous Blue Variables
• +۵ مورد دیگر

John Martin is an Associate Professor at the University of Illinois Springfield, affiliated with the School of Integrated Sciences, Sustainability, and Public Health. Since 2006, he has taught introductory physics for science majors and astronomy courses while directing the Henry R. Barber Research Observatory and hosting public UIS Star Parties. His research focuses on stellar astrophysics, particularly the life cycles of massive stars and phenomena like Eta Carinae. Stellar Astrophysics Massive Star Evolution Luminous Blue Variables (LBVs) Supernova Impostors Be Stars and Disks Photometry and Spectroscopy His publications, including over 100 peer-reviewed works, emphasize Eta Carinae's 5.5-year spectroscopic events, LBVs in M31/M33, Be star dynamics, and supernova impostors like SN 2009ip. Awards include the 2011 University of Illinois University Scholar title, JJ Nassau Fellowship (1997), and Dean's List recognitions. He earned his PhD in Astronomy from Case Western Reserve University (2003) and BS in Astro-Physics from the University of Virginia (1995). Scientific awards include 2011 University of Illinois University Scholar 1997 JJ Nassau Graduate Research Fellowship 1995 Mastin Graduate Fellowship 1995 Dean's List, University of Virginia 1994 Dean's List, University of Virginia

Paul Wiegertمشاهده پروفایل

استاد

• Planetary Science
• Astronomy
• Celestial Mechanics
• +۶ مورد دیگر

Paul Wiegert is a Full Professor in the Department of Physics and Astronomy at the University of Western Ontario , where he has been since 1996 after positions at York University and Queen's University. He is a member of the Institute for Earth and Space Exploration (IESX) and the Centre for Planetary Science and Exploration (CPSX) . His research spans asteroid dynamics , exoplanet systems , and celestial mechanics , with notable work on Earth co-orbital asteroids like (3753) Cruithne and Earth's first Trojan asteroid 2010 TK7. Education : PhD in Astronomy (University of Toronto, 1996) Research Domains : Planetary Science, Astronomy, Big Data Analytics His recent publications focus on interstellar transport mechanisms , asteroid impact risks , and exomoon detection . Key findings include quantifying risks from asteroid 2024 YR4's potential lunar impact and demonstrating the feasibility of detecting alpha Centauri-origin material in our solar system. He actively supervises graduate students like Cole Gregg and participates in NSERC-funded summer research programs for undergraduates. For planetary defense, he has analyzed collision probabilities for Apophis and developed meteoroid hazard models for spacecraft. His work appears in Planetary Science Journal , Nature Astronomy , and Astrophysical Journal Letters , with media coverage in 60+ outlets and 126 X (Twitter) mentions .

Matthias Ihmeمشاهده پروفایل

استاد

• Combustion Science
• Fluid Dynamics
• Computational Fluid Dynamics
• +۵ مورد دیگر

Matthias Ihme is a Professor in the Department of Mechanical Engineering and Photon Science Directorate at Stanford University. His research focuses on large-eddy simulation (LES) of turbulent reacting flows, aeroacoustics, combustion-generated noise, numerical methods, and high-order schemes. He holds a Ph.D. from Stanford University (2008), an M.Sc. in Computational Engineering from the University of Erlangen (Germany, 2002), and a Dipl.-Ing. in Mechanical Engineering from Munich University of Applied Sciences (Germany, 2000). His work bridges computational fluid dynamics, combustion science, and photon science, with notable contributions to supercritical fluid dynamics, machine learning integration in fluid simulations, and high-fidelity atmospheric transport modeling. Recent research emphasizes ultrafast cluster dynamics, shock-induced interface behavior, and stochastic ignition mechanisms in advanced fuel systems. Publications highlight interdisciplinary advancements, including physics-informed ML frameworks for reacting flows and experimental studies using X-ray photon correlation spectroscopy. His projects often involve high-performance computing and collaboration with national labs like SLAC.

Gordon J. Staceyمشاهده پروفایل

استاد

• Star Formation
• Galaxy Formation and Evolution
• Far-Infrared/Submillimeter Spectroscopy
• +۴ مورد دیگر

Gordon J. Stacey is the David C. Duncan Professor in the Physical Sciences and CCAT Project Director at Cornell University's Department of Astronomy. He received his PhD in Astronomy from Cornell in 1985 and joined the faculty in 1991 after postdoctoral work at UC Berkeley. His research focuses on star and galaxy formation across cosmic time, utilizing far-infrared/submillimeter spectroscopy. He leads the CCAT Project, developing the FYST telescope in Chile, and is Principal Investigator for the POEMM mission targeting protoplanetary disks. Notable contributions include instrumental advancements like ZEUS-2 and EoR-Spec, as well as seminal studies on [CII], [NII], and [OIII] lines in high-redshift galaxies. Education: PhD in Astronomy from Cornell University (1985). Research emphasizes interstellar medium interactions, cosmic evolution, and instrumentation. Key projects include EoR-Spec for FYST (first light 2027) and the VIPA-based POEMM mission (2029 balloon flight). Awards include the David C. Duncan Professorship. His work bridges observational cosmology, galaxy evolution, and technological innovation in astronomy. Scientific awards include the endowed David C. Duncan Professorship. Current roles involve directing the CCAT Project and advancing instrumentation for submillimeter astronomy. Future projects focus on protoplanetary disk studies via POEMM and FYST observations of the Epoch of Reionization.

• Galaxy Evolution
• Active Galactic Nuclei (AGN)
• Interstellar Medium (ISM)
• +۳ مورد دیگر

Jarle Brinchmann is an Associate Professor at Leiden University's Leiden Observatory, part of the Faculty of Science. He holds a PhD from the University of Cambridge and has held postdoctoral positions at Oxford University, the Max Planck Institute for Astrophysics, and the University of Porto. His research focuses on galaxy evolution, active galactic nuclei (AGN), and interstellar medium dynamics. Notable contributions include studies on gas outflows in galaxies and emission line diagnostics for AGN identification. Recent work includes analysis of Lyman-alpha emitters and binary star systems in globular clusters using the MUSE instrument. Education: BSc and MSc in Astronomy from the University of Oslo, PhD from the University of Cambridge (thesis: 'The physical evolution of galaxies'). Research emphasizes observational and theoretical astrophysics, with a focus on high-redshift galaxies, intergalactic medium interactions, and stellar populations. Collaborates widely on large-scale surveys and spectroscopic analyses.

Stuart C. Althorpeمشاهده پروفایل

استاد

• Theoretical Chemistry
• Quantum Dynamics
• Quantum Mechanics
• +۴ مورد دیگر

Professor Stuart C. Althorpe is a Professor of Theoretical Chemistry at the Department of Chemistry, University of Cambridge, where he leads the Althorpe Research Group. His work focuses on quantum dynamics and the application of quantum mechanics to chemical reactions, particularly examining how quantum effects influence atomic and molecular motion in systems ranging from isolated reactions to liquid water and ice. Professor Althorpe's research interests center on quantum dynamics , with specific focus on quantum tunneling , conical intersections , and path-integral methods . His group develops computational techniques that bridge quantum statistics and classical dynamics, creating methods like Matsubara dynamics to model quantum effects in complex systems. Key research areas include visualizing complete wave functions of chemical reactions, calculating tunneling splittings in water clusters, and investigating quantum interference effects at electronic degeneracies. The group employs both pen-and-paper theoretical derivations and high-performance computational algorithms for parallel CPUs and GPUs to tackle these challenging problems. The trends in Professor Althorpe's recent publications (2018-2024) reveal an evolution from foundational quantum dynamics methods toward increasingly sophisticated applications in complex, dissipative environments. His work consistently bridges computational chemistry and quantum physics, with growing emphasis on connections between quantum dynamics, chaos theory, and quantum information concepts. The publications demonstrate methodological innovation in path-integral approaches, particularly in handling quantum effects in condensed-phase systems like water and ice, while maintaining strong connections to experimental observations. Professor Althorpe has mentored over two dozen PhD students and postdoctoral researchers who have secured positions at leading institutions including ETH Zürich, UCL, EPFL, and various industry roles. His research group maintains active international collaborations, most notably with Professor D.J. Wales at Cambridge (on water clusters) and Professor Richard N. Zare at Stanford University, where theoretical calculations interpret detailed experimental measurements of reaction dynamics. The Althorpe Group operates within the Department of Chemistry at the University of Cambridge as part of the Theoretical Research Interest Group. The group's work contributes significantly to understanding quantum mechanical phenomena in chemical processes, with implications for fields ranging from atmospheric chemistry to biochemistry. Professor Althorpe organized the 2019 Faraday Discussion on "Quantum effects in complex systems," demonstrating his leadership in advancing theoretical frameworks for quantum phenomena in chemistry.

• Astronomy Education
• Observational Astronomy
• High-energy Astrophysics
• +۴ مورد دیگر

Professor Andrew Newsam is a faculty member at Liverpool John Moores University's Astrophysics Research Institute (ARI), where he serves as Professor of Astronomy Education and Engagement since 2012. He has been instrumental in developing the National Schools' Observatory and astronomy distance learning courses, bridging observational astronomy with STEM education initiatives. Education: PhD in Astrophysics from University of Glasgow (1994), BSc in Physics with Computing from University of Warwick (1991) His research spans observational astronomy, high-energy astrophysics, and science education. Recent publications focus on nova remnants (RS Ophiuchi), gamma-ray bright novas (Nova Persei 2018, V392 Persei), microlensing surveys (Angstrom Project), and educational outreach. He has contributed to planetary eclipse studies and interstellar dynamics research. Key trends in his publications include: binary star systems (56% of works), transient phenomena (43%), and educational technology (35%). His citations show strong engagement with nova studies (22% of total citations) and microlensing research (19% of total citations). Scientific Awards: Teaching Fellowship Award for Individual Excellence (2009) Curriculum Innovation Award (2007) Queens Anniversary Prize for Higher and Further Education (2005) As chair of multiple education and outreach panels (2016-2025), he has shaped astronomy policy and public engagement strategies. He received STFC grants for STEM capacity building (2020) and BBSRC funding for citizen science projects (2019).

Tesla Jeltemaمشاهده پروفایل

استاد

• observational cosmology
• particle astrophysics
• dark matter
• +۳ مورد دیگر

Tesla Jeltema is a Professor in the Department of Physics at the University of California, Santa Cruz and serves as Associate Director of the Santa Cruz Institute for Particle Physics (SCIPP). Her office is located in ISB 305 at 1156 High Street, Santa Cruz, CA 95064. She currently holds the position of Deputy Spokesperson for the LSST Dark Energy Science Collaboration (DESC). Her research centers on: Observational cosmology and particle astrophysics Constraints on dark matter and dark energy properties Galaxy evolution and large-scale structure formation She actively contributes to major international projects: Rubin Observatory LSST DESC Dark Energy Survey (DES) Dark Energy Spectroscopic Instrument (DESI) Scientific recognition includes: 2020 Meenakshi Narain Mentoring Award from the American Physical Society Dr. Jeltema mentors 3-5 graduate students and 4-8 undergraduate/postbaccalaureate researchers through programs including Cal-Bridge, DESC, DES, and UCSC's STEM Diversity initiatives (CAMP and UC LEADS). She founded and advises the UCSC Women in Physics and Astrophysics Club since 2011 and serves on multiple diversity and inclusion committees. Her institutional affiliations include the Santa Cruz Institute for Particle Physics and the Department of Physics at UC Santa Cruz.