جست‌وجوی استاد و پژوهشگر

Philip Changمشاهده پروفایل

استاد

• Theoretical Astrophysics
• Cosmology
• Supernovae
• +۴ مورد دیگر

Philip Chang is a Professor and Department Chair in the Department of Physics at the University of Wisconsin-Milwaukee (UWM), specializing in theoretical and computational astrophysics. He holds editorial responsibilities as an associate editor at Physical Review D (PRD). His primary research investigates fundamental astrophysical phenomena through advanced computational models and theoretical frameworks. Chang received his academic training at premier institutions: Bachelor of Arts (BA) from Harvard University (1998) PhD in Physics from the University of California, Berkeley (2005) under Professor Lars Bildsten He conducted postdoctoral research at UC Berkeley (2005-2009) and the University of Toronto (2005-2009) before joining UWM in 2011. His research program focuses on high-energy astrophysical processes and cosmological phenomena, with particular emphasis on: Supernova dynamics and stellar explosion mechanisms Compact object physics including white dwarfs and neutron stars Plasma astrophysics of relativistic environments Disk dynamics in accretion systems Turbulent star formation processes in interstellar media Cosmological implications of TeV blazars and gamma-ray backgrounds Theoretical modeling of gravitational phenomena This work bridges computational simulations with observational astrophysics to address fundamental questions about cosmic evolution. His publication record demonstrates interdisciplinary reach, with recent work spanning: Core astrophysics topics like white dwarf mergers, blazar heating, and star formation quenching Particle physics through LHC collaborations Medical research including hepatology and oncology studies Theoretical astrophysics remains the dominant theme, representing approximately 60% of recent publications. Chang leads the Astronomy, Gravitation and Cosmology research group at UWM, where he develops computational frameworks for astrophysical simulations. He maintains an active research website documenting projects and publications.

Chanda Prescod-Weinsteinمشاهده پروفایل

دانشیار

• Astrophysics
• Theoretical Physics
• Dark Matter
• +۳ مورد دیگر

Chanda Prescod-Weinstein is an Associate Professor in the Department of Physics & Astronomy at the University of New Hampshire. Her research focuses on theoretical physics, astrophysics, and dark matter, with particular expertise in neutron star physics, ultralight dark matter dynamics, and multifield inflationary cosmology. She holds a Ph.D. from the University of Waterloo, an M.S. from the University of California-Santa Cruz, and an A.B. from Harvard University. Her work bridges particle physics and astrophysics, addressing questions about dense matter equations of state via neutron star observations, axion-like dark matter simulations, and cosmological structure formation. Recent contributions include developing the NEoST Python package for neutron star studies and analyzing NICER mission data to constrain dense matter properties. Prescod-Weinstein teaches advanced courses such as Astrophysics I, Quantum Mechanics I, and doctoral research seminars. Her research incorporates numerical simulations, Bayesian statistical methods, and observational data from space-based telescopes like NICER and XMM-Newton.

Jillian Bornakمشاهده پروفایل

عضو هیئت علمی

• Astronomy Education
• Infrared Photometry
• Novae
• +۱ مورد دیگر

Jillian Bornak is a Distinguished University Lecturer specializing in astronomy education reform. Her astrophysical research modeled dust formation in classical novae using DIRTY radiative transfer code. Awarded Provost Outstanding Teacher Award (2017). Teaches introductory astronomy and physics courses using evidence-based pedagogical approaches. Research background includes crowded field photometry and analysis of periodic emission in X-ray binaries.

Neil Cornishمشاهده پروفایل

استاد

• Gravitational Wave Astronomy
• Cosmology
• Relativistic Astrophysics
• +۲ مورد دیگر

Neil Cornish is a Regents Professor and Distinguished Professor in the Department of Physics at Montana State University's College of Letters & Science, where he directs research through the eXTreme Gravity Institute (XGI). His work focuses on gravitational wave detection and relativistic astrophysics, with collaborations spanning CalTech, MIT, Harvard, Princeton, and European institutions. Education: Ph.D. in Physics, University of Toronto (1996) M.S. in Physics, University of Melbourne (1992) B.S. in Physics, University of Melbourne (1990) Cornish's research explores extreme gravity phenomena including black hole mergers, neutron star binaries, and early-universe cosmology. His 2024 publications demonstrate consistent focus on gravitational wave data analysis techniques, pulsar timing arrays, and multi-messenger astrophysics, with particular emphasis on noise modeling and detection methodologies for LIGO/Virgo observations. Awards & Honors: Outstanding Referee, American Physical Society (2021) College of Letters and Science Distinguished Professor (2021) Regents Professorship, MUS (2018) Springer Physics Highlights (2017) Provost’s Award for Graduate Research Mentoring, MSU (2017) He has advised numerous graduate students including Meg Millhouse and Laura Sampson, and secured major grants from NASA and NSF for LISA gravitational wave research and Bayesian signal reconstruction. Cornish co-leads the eXTreme Gravity Institute, coordinating research across gravitational wave theory, data analysis, and cosmology.

Thomas Corbittمشاهده پروفایل

استاد

• Experimental General Relativity
• Quantum Optomechanics
• Gravitational Wave Detection
• +۲ مورد دیگر

Thomas Corbitt is Professor of Physics at Louisiana State University's College of Science, Department of Physics & Astronomy. He holds a PhD from MIT and specializes in Experimental General Relativity and quantum optomechanics. His research focuses on precision measurements at the quantum limit, gravitational wave detection, and developing advanced interferometric techniques. Research examines quantum noise suppression in gravitational wave detectors, optomechanical systems approaching the quantum regime, and multi-messenger astrophysics collaborations. Work contributes to LIGO-Virgo-KAGRA scientific collaborations searching for gravitational waves from cosmic events like neutron star mergers and black hole collisions. Recent publications demonstrate strong focus on developing quantum-enhanced measurement techniques for gravitational wave detectors, searching for exotic astrophysical phenomena including dark matter signatures, and analyzing data from international detector networks. Laboratory develops advanced optical techniques including optical springs and quantum squeezing methods to surpass standard quantum limits in precision measurements. Leads research in quantum optomechanics and contributes to large-scale international collaborations in gravitational wave astronomy.

Juhan Frankمشاهده پروفایل

استاد

• Astrophysics
• Black Hole Accretion
• White Dwarf Binaries
• +۳ مورد دیگر

Juhan Frank is the Lorraine and Leon August Professor of Physics & Astronomy at Louisiana State University (LSU), within the College of Science and the Department of Physics & Astronomy . He holds a Ph.D. from the University of Cambridge (1978) and a Licenciado en Ciencias Físicas from the Universidad de Buenos Aires (1970). His research focuses on accretion processes in compact astrophysical systems, including active galactic nuclei, X-ray binaries, and white dwarf binaries. Notably, he explores the dynamics of accretion onto black holes, neutron stars, and white dwarfs, emphasizing hydrodynamics, radiative transfer, and binary system evolution. Frank’s work includes studies on double white dwarf mergers, their implications for gravitational wave observations (e.g., LISA), and the origins of R Coronae Borealis stars. He has contributed to developing numerical methods like the Octo-Tiger code for simulating stellar mergers and mass transfer in binaries. His research also addresses the role of irradiation in cataclysmic variables and the transient behavior of low-mass X-ray binaries. Frank has authored influential textbooks, including Accretion Power in Astrophysics (3rd ed., 2002), a graduate-level treatise on accretion disk theory. His affiliations include the Landolt Astronomical Observatory and the Hearne Institute of Theoretical Physics. Courses he has taught include Astronomy 1102: Stellar Astronomy , emphasizing scientific method and observational astronomy. His recent research leverages high-performance computing to model complex systems, such as binary mergers and galactic structure formation. Collaborations with institutions like ORNL highlight his engagement with cutting-edge computational tools. Frank’s work bridges theoretical astrophysics, numerical simulation, and observational astronomy, with implications for understanding galaxy evolution, stellar dynamics, and gravitational wave sources.

Øystein Elgarøyمشاهده پروفایل

استاد

• Cosmology
• Astrophysics
• Dark Matter
• +۴ مورد دیگر

Øystein Elgarøy is a Professor at the Department of Astrophysics, University of Oslo. His research focuses on cosmology, astrophysics, and fundamental physics, particularly in areas such as dark matter behavior, neutrino physics, modified gravity theories, and superfluid dynamics in neutron stars. He has contributed extensively to understanding cosmic structures, cosmological models, and the interplay between particle physics and cosmology. His work spans decades, addressing topics like the cosmic microwave background (CMB), neutrino mass constraints, and alternative cosmological frameworks such as f(R) gravity and Friedmannless models. Collaborations include projects like the Euclid Strategic Dark Matter Initiative and the Cosmology and Extragalactic Astronomy research group. His recent studies explore quantized vortices in superfluid dark matter and cross-correlation analyses involving neutrinos and modified gravity. Elgarøy’s publications frequently bridge theoretical concepts with observational data, such as WMAP and KATRIN experiments. His research also touches on foundational questions like the expansion of space in Friedmann models and gravitational entropy’s role in inflationary scenarios.

• Astrophysics
• Gravitational Waves
• Pulsar Timing
• +۳ مورد دیگر

Dr. Michael Keith is a Senior Lecturer in Astrophysics at the University of Manchester's Astronomy and Astrophysics Theory Group. His research focuses on pulsar timing arrays, gravitational wave detection, and neutron star physics. He collaborates extensively with international teams like the European Pulsar Timing Array and uses facilities such as MeerKAT and LIGO. Key areas include studying millisecond pulsars, pulsar glitches, and the interstellar medium. His work contributes to understanding gravitational wave backgrounds and fundamental physics through precision timing. Recent projects involve analyzing pulsar data from the International Pulsar Timing Array and exploring axion dark matter effects using pulsar observations. Keith has published over 123 articles in journals like the Astrophysical Journal and Monthly Notices of the Royal Astronomical Society. His research is supported by grants involving collaborations with institutions worldwide, including NASA, LIGO, and MeerKAT projects.

Aaron Vincentمشاهده پروفایل

دانشیار

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

Aaron Vincent is an Associate Professor in the Department of Physics, Engineering Physics and Astronomy at Queen's University. He is affiliated with the Faculty of Arts and Science and holds a cross-appointment at the Arthur B. McDonald Canadian Astroparticle Physics Institute. His research focuses on astroparticle physics and cosmology, particularly dark matter interactions, neutrino astronomy, and high-energy astrophysical phenomena. Prof. Vincent completed his PhD at McGill University (2012) and held postdoctoral positions at the University of Valencia, Durham University, and Imperial College London. He joined Queen's in 2018. His educational background includes a B.A. from Laval University and an M.Sc. from McGill. Research interests span dark matter's impact on stars, neutrino telescopes, and cosmological implications. He teaches courses like ASTR102 (Astronomy II) and advanced graduate seminars on quantum mechanics and the early universe. Key affiliations: QHEAT Group, Queen's Astronomy Research Group Key grants/funding: Not explicitly listed in provided texts Labs/teams: Involved with the McDonald Institute and collaborations using facilities like IceCube Neutrino Observatory.

Joseph Bramanteمشاهده پروفایل

استادیار

• Particle Theory
• Dark Matter
• Cosmology
• +۵ مورد دیگر

Joseph Bramante is an Assistant Professor of Physics at Queen’s University, with a joint appointment at the Arthur B. McDonald Canadian Astroparticle Physics Institute. He holds a visiting fellowship at the Perimeter Institute for Theoretical Physics. His research focuses on dark matter, the early universe, and fundamental physics puzzles such as dark matter’s nature, baryon asymmetry, and the Higgs mass hierarchy problem. He explores novel detection methods for dark matter, including underground experiments like SNO+ and PICO, and has contributed to projects like the Future Circular Collider feasibility study. He earned a BA in Liberal Arts from Sarah Lawrence College (2007) and a PhD in theoretical physics from the University of Hawaii (2013). His postdoctoral work included stints at the University of Notre Dame and Perimeter Institute. Current research emphasizes multiply interacting massive particles (MIMPs) and dark matter’s role in astrophysical phenomena like supernovae. Bramante collaborates with experimentalists to design innovative detection strategies, such as using superheated liquids and scintillator doping. His theoretical contributions span cosmology, particle physics, and quantum gravity interfaces. He advises three postdoctoral researchers and actively engages in cross-disciplinary projects at Queen’s and the McDonald Institute. Notable venues for his work include the Journal of Cosmology and Astroparticle Physics and the Future Circular Collider conceptual design reports.

Matthew L. Listerمشاهده پروفایل

استاد

• Active Galactic Nuclei (AGN)
• Astrophysical Jets and Shocks
• Quasars
• +۵ مورد دیگر

Matthew L. Lister is a Professor of Physics at Purdue University, specializing in active galactic nuclei (AGN) and relativistic jets. He leads the MOJAVE program, a long-term VLBA monitoring initiative to study AGN jets' kinematics and polarization. His research focuses on AGN jets, gamma-ray emission, and young AGN systems like compact symmetric objects (CSOs). Lister earned his Ph.D. from Boston University in 1999, with earlier degrees from the University of Victoria (M.S.) and the University of Toronto (B.S.). He has held roles including Karl Jansky Fellow at the National Radio Astronomy Observatory and Faculty Lecturer at the University of Virginia. His work includes studying blazars, narrow-line Seyfert 1 galaxies, and supermassive black hole binaries. Notable grants include a NASA Fermi Guest Investigator award (2019) and MOJAVE's ongoing VLBA funding. He advised students like Mary Ann Hodge and contributed to major collaborations like TANAMI and IceCube. Lister transitioned to MathWorks in 2022 but remains active in AGN research. Education: Ph.D. Astronomy (Boston U, 1999), M.S. Physics & Astronomy (Victoria, 1993), B.S. Physics & Astronomy (Toronto, 1991). Research Interests: AGN jet dynamics, VLBI imaging, gamma-ray astrophysics, and the MOJAVE program's role in linking radio and gamma-ray emission. Key projects include analyzing AGN kinematics, redshift determinations of BL Lacs, and young jet systems. His work bridges observational astronomy with theoretical models of jet formation and relativistic effects. Publications span over 150 peer-reviewed articles, emphasizing multiwavelength studies and jet structure. He is a member of the American Astronomical Society and serves as a referee for major journals.

Avery Broderickمشاهده پروفایل

دانشیار

• Astrophysics
• Gravitation
• Black Hole Imaging
• +۳ مورد دیگر

Avery Broderick is an Associate Professor in the Department of Physics & Astronomy at the University of Waterloo and an Associate Faculty Member at the Perimeter Institute for Theoretical Physics. He holds a PhD in Physics from the California Institute of Technology (2004) and a BS in Physics and Mathematics from SUNY Stony Brook (1999). His research focuses on black hole physics, gravitational effects, and their observational signatures, particularly through participation in the Event Horizon Telescope Collaboration. He has contributed to the first horizon-resolving images of astronomical black holes and explores the interplay between plasma physics, gamma-ray emission, and cosmological magnetic fields. Broderick's work spans scales from black hole horizons to cosmological structures, emphasizing strong gravity phenomena and high-energy astrophysics. He has published extensively in journals like ApJ and Scientific American , and his teaching includes courses like PHYS 263 (Classical Mechanics) and PHYS 363 (Intermediate Classical Mechanics). Awards include the 2007 Certificate of Distinction in Teaching from Harvard University's Derek Bok Center. His affiliations include the Waterloo Centre for Astrophysics and editorial roles with Scientific Reports . Research interests include white dwarf interactions with black holes, gamma-ray burst dynamics, and magnetic field evolution in astrophysical plasmas.

Seth Gossageمشاهده پروفایل

پژوهشگر ارشد

• Stellar Evolution
• Binary Star Systems
• Stellar Rotation Modeling
• +۲ مورد دیگر

Seth Gossage is a Research Associate at the Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) at Northwestern University, where he was promoted from CIERA postdoc in 2024 after three years (2021-2024). He collaborates extensively with Professor Vicky Kalogera on stellar evolution modeling and population synthesis. His research focuses on stellar evolution , particularly through computational modeling using MESA and development of the POSYDON population synthesis code. Key interests include: Effects of stellar rotation on observational signatures Binary star evolution pathways Convective dynamics in low-mass stars Progenitor systems for supernovae and gravitational wave sources Analysis of his 15 most recent publications (2023-2025) reveals a strong emphasis on binary interactions across metallicity ranges, with significant contributions to understanding stripped-envelope supernovae, double neutron star formation, and gamma-ray burst progenitors. His work bridges theoretical modeling with observational constraints from HST and spectroscopic surveys. Notable scientific contributions include: First-author paper on convective turnover times in low-mass stars (ApJ 2025) Key role in POSYDON v2 development for cosmological metallicity ranges Analysis of Be star-black hole binaries using LAMOST data Gossage mentors through CIERA's REU program (evidenced by student presentations at AAS meetings) and contributes to outreach initiatives. His current work involves developing grids of 1D stellar models to replicate population data while investigating rotational effects.

• Astrophysics
• Cosmology
• Gravitational Wave Astronomy
• +۳ مورد دیگر

Yue Zhao is a Research Fellow at the University of Southampton, specializing in astrophysics and gravitational wave astronomy. His work focuses on dark matter detection, compact object binaries, and early-universe physics phenomena. Current research interests include: Dark photon dark matter Low-frequency gravitational wave detection Natal kicks in black hole X-ray binaries Compact object populations in globular clusters Recent publications demonstrate expertise in multi-messenger astronomy using data from Gaia-like astrometry missions, Chandra X-ray Observatory, and Very Large Array (VLA). Key collaborations span institutions like Royal Astronomical Society and NASA facilities. Yue Zhao's work addresses fundamental questions about the universe's structure through astrophysical observations and theoretical modeling, particularly in gravitational wave signatures and dark matter interactions.

E. S. Sterl Phinneyمشاهده پروفایل

استاد

• Astrophysics
• Relativistic Astrophysics
• High-Energy Astrophysics
• +۷ مورد دیگر

E. S. Sterl Phinney is a renowned Professor of Theoretical Astrophysics at the California Institute of Technology (Caltech). With a PhD from Cambridge University (1983) and a BS from Caltech (1980), he has made significant contributions to high-energy relativistic astrophysics and low-energy Newtonian astrophysics. His work often explores the role of antimatter in astrophysical systems.