Fast Transients Professors and Supervisors | ApplySharif

جست‌وجوی استاد و پژوهشگر

استاد راهنما، استاد دانشگاه یا پژوهشگر مناسب برای مسیر پژوهشی‌تان را پیدا کنید و با او ارتباط بگیرید.

نمایش ۳۳۱-۳۴۵ از ۳۷۰ استاد راهنما

اطلاعات این پروفایل‌ها از صفحات عمومی دانشگاه‌ها جمع‌آوری شده و ممکن است به‌روز نباشد.

Aurélien Tissotمشاهده پروفایل

پژوهشگر

Polytechnic University of MilanItaly

Aurélien Tissot is a Researcher affiliated with the Nuclear Reactors Group (NRGroup) at Politecnico di Milano. His primary role involves advanced R&D in nuclear engineering, particularly focusing on fuel performance modeling and GenIV reactor technologies. He has been continuously involved with NRGroup since 2016, contributing to projects on lead-cooled fast reactors, reduced-order modeling, and inert gas behavior in nuclear fuels. Education: MSc in Engineering (Mechanical Systems), Université de Technologie de Troyes, France (2013) PhD in Nuclear Engineering, Politecnico di Milano (2015) Research Highlights: Tissot’s work spans nuclear fuel behavior analysis, transient modeling of nuclear systems, and computational methods for reactor design. His PhD thesis addressed inert gas dynamics in UO₂ fuel, while his MSc thesis explored fuel pin performance codes. Recent efforts include MSR/LFR (Molten Salt/Lead Fast Reactors) and control-oriented modeling of GenIV systems. Labs & Teams: Active member of NRGroup, specializing in next-generation reactor technologies and fuel performance simulation. Collaborates with institutions like POLIMI and NRGroup alumni networks.

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Mostafa Jamalipourمشاهده پروفایل

پژوهشگر

Polytechnic University of MilanItaly

Mostafa Jamalipour is a Researcher affiliated with the Nuclear Reactor Group (NRGroup) at Politecnico di Milano. His research focuses on advanced nuclear reactor technologies, including neutronics analysis, fuel performance modelling, and Gen IV reactor systems such as Small Modular Reactors (SMR) and Lead-Cooled Fast Reactors (LFR). He conducted a 20-month R&D period at NRGroup from 2016–2017, collaborating on configuration studies for innovative reactor cores. His work involves developing reduced-order models and analyzing inert gas behavior in nuclear fuels under transient conditions. Educational Background: MSc from Kerman Graduate University of Advanced Technology (KGUAT, Iran). R&D Contributions: Fuel performance modelling, helium behavior analysis in oxide fuels, and transient analysis methodologies. Collaborators include researchers like Stefano Lorenzi (specializing in Gen IV MSR/LFR systems) and Davide Pizzocri (PhD in fuel transient analysis). His research bridges theoretical modelling with practical applications in next-generation nuclear energy systems.

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Dario Colorado Garridoمشاهده پروفایل

پژوهشگر

Polytechnic University of MilanItaly

Dario Colorado Garrido is a Researcher affiliated with the Department of Energy at Politecnico di Milano (NRGroup). His primary role involves R&D activities since 2016, focusing on GenIV reactors (e.g., Molten Salt Reactors, Lead-Cooled Fast Reactors) and advanced computational modeling techniques. He has held continuous R&D periods at NRGroup since 2016, contributing to projects like fuel performance analysis and reduced-order modeling. Education: PhD in Nuclear Engineering (2015): Thesis on control-oriented modeling of GenIV lead-cooled reactors. MSc in Nuclear Engineering (2011): Thesis on fuel pin performance code extensions. Additional MSc (2020): Thesis on helium behavior in oxide nuclear fuel. His research interests span fuel behavior under transient conditions, computational model validation, and advanced reactor design. Collaboration with institutions like the Universidad Autónoma del Estado de Morelos (Mexico) highlights interdisciplinary work in energy systems. No scientific awards or grants are explicitly mentioned in the provided text.

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Jonas Narvaez Arruaمشاهده پروفایل

پژوهشگر

Polytechnic University of MilanItaly

Jonas Narvaez Arrua is a Researcher affiliated with Politecnico di Milano (POLIMI) as part of the NRGroup. His R&D activities span from 2016 to the present, focusing on advanced nuclear technologies including fuel performance modeling, Gen IV reactors (e.g., Molten Salt Reactors, Lead-Cooled Fast Reactors), and neutronics/thermal fluid dynamics under projects like SAMOSAFER. He holds two conflicting PhD degrees: one in 2015 titled *'Improvement of the control-oriented modelling of the Gen-IV lead-cooled fast reactor'* and another in 2018 titled *'Modelling and assessment of inert gas behaviour in UO2 nuclear fuel for transient analysis.'* His MSc degrees were completed in 2013 and 2011. Research interests emphasize fuel behavior analysis, reduced-order modeling techniques, and safety assessments for next-generation reactors. His work bridges theoretical modeling with practical applications in nuclear energy systems. No scientific awards or published articles are explicitly listed in the provided text. Current roles include R&D contributions at NRGroup and research assistantship at POLIMI.

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James Turnerمشاهده پروفایل

پژوهشگر

The University of ManchesterUnited Kingdom

James Turner is an active researcher specializing in radio astronomy with a strong focus on pulsar physics and transient phenomena. His work primarily utilizes the MeerKAT radio telescope and TRAPUM survey for astronomical observations. His research interests center on pulsar physics (100% of his research fingerprint), transient astronomy (64%), and related areas including nebula physics, supernova remnants, and the Small Magellanic Cloud. His work has significant implications for understanding neutron stars, galactic structure, and extragalactic phenomena. Turner's recent publications demonstrate a strong trend toward multi-wavelength observations, combining radio data with gamma-ray measurements, and expanding pulsar surveys to dwarf galaxies beyond the Milky Way. His work frequently addresses technical challenges in signal processing and transient detection. His research has garnered attention across academic platforms with multiple publications picked up by X users and readers on Mendeley, indicating growing influence in the field of radio astronomy.

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Paul Grootمشاهده پروفایل

استاد

Radboud UniversityNetherlands

Prof. Paul Groot is a Professor of Astrophysics at Radboud University (Nijmegen, Netherlands) and holds a SARChI Chair in Fast Transients and Gravitational Wave Astronomy at the University of Cape Town and South African Astronomical Observatory. He co-founded the Department of Astrophysics at Radboud University (2002) and served as its chair (2006–2016). He was also chair of the Netherlands Research School for Astronomy (NOVA, 2012–2016). His research focuses on compact binary systems, gravitational wave sources, and astronomical instrumentation. Key projects include leadership of the BlackGEM telescope array in Chile for gravitational wave optical counterpart detection and the MeerLICHT telescope in South Africa for radio-optical transient studies. He was Project Scientist for the VLT X-Shooter spectrograph and co-initiator of the European Galactic Plane Surveys. Major awards include the 2016 Breakthrough Prize in Fundamental Physics (shared with LIGO collaboration) and the 2016 Gruber Cosmology Prize. His educational background includes a PhD from the University of Amsterdam (1999) and a postdoctoral fellowship at the Harvard-Smithsonian Center for Astrophysics.

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David Reitzeمشاهده پروفایل

استاد پژوهشی

California Institute of Technology (Caltech)United States

David Reitze is the Executive Director of the Laser Interferometer Gravitational-wave Observatory (LIGO) and a Research Professor of Physics at the California Institute of Technology. He leads LIGO's operations and research initiatives, focusing on gravitational wave detection and multi-messenger astrophysics. His leadership was pivotal in achieving the first direct observation of gravitational waves from a black hole merger, a milestone recognized by his 2018 AAAS Fellowship. Reitze's research emphasizes advanced interferometry, detector technology, and observational cosmology. His work bridges fundamental physics with engineering innovations to push the frontiers of gravitational wave astronomy. Key contributions include developing operational protocols for LIGO's observing runs, optimizing data analysis techniques, and fostering international collaborations with facilities like Virgo and KAGRA. His recent efforts expand into next-generation observatories, including Cosmic Explorer, and involve exploring gravitational wave signatures from extreme astrophysical events such as neutron star mergers, supernovae, and potential dark matter interactions. Reitze also advocates for open data policies to democratize gravitational wave research. Major accolades include the AAAS Fellowship (2018) and leadership in LIGO's Nobel Prize-winning 2015 discovery. He remains central to advancing gravitational wave science through technological advancement and global research coordination.

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Huirong Yanمشاهده پروفایل

استاد

German Electron SynchrotronGermany

Huirong Yan is a Professor (W3) at the University of Potsdam and a Leading Scientist at DESY, a Helmholtz research center. Her research focuses on plasma astrophysics, cosmic ray physics, and the interstellar medium. She leads the Plasma Astrophysics group, developing diagnostics for magnetic fields and turbulence. Her work integrates observational data with theoretical models to understand cosmic ray propagation, turbulence dynamics, and interstellar medium properties. Academic Career: Since 2015: Leading Scientist at DESY and Professor at University of Potsdam 2009–2015: Professor at Kavli Institute for Astronomy and Astrophysics, Peking University 2008–2010: Arizona Prize Fellow, University of Arizona 2005–2008: Postdoctoral Fellow at CITA, Toronto 2005: PhD from University of Wisconsin-Madison Research Interests: Her studies explore fundamental plasma processes in cosmic ray acceleration, interstellar turbulence, and magnetic field dynamics. Key areas include: Turbulence in interplanetary and interstellar plasmas Cosmic ray transport mechanisms Magnetic field diagnostics via synchrotron polarization and atomic alignment Shock dynamics and particle acceleration in supernova remnants Key Contributions: Her group has pioneered techniques to measure magnetic fields in diffuse media and analyze turbulence transitions in space plasmas. Recent work includes observational evidence of Alfvénic turbulence regime shifts and studies of TeV halos around pulsars. Memberships: American Astronomical Society American Geophysical Union European Physical Society German Astronomical Society Lab/Team: She leads the Plasma Astrophysics group at DESY, collaborating on projects like FAST telescope polarization analyses and Parker Solar Probe data interpretation.

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James H. Buckleyمشاهده پروفایل

استاد

Washington University in St. LouisUnited States

James H. Buckley is a Professor of Physics at Washington University in St. Louis, affiliated with the McDonnell Center for the Space Sciences and the Center for Quantum Leaps. His research focuses on Particle Astrophysics, particularly dark matter searches using experiments like ADMX, gamma-ray astronomy with collaborations such as VERITAS and CTA, and multi-messenger studies of astrophysical transients like Fast Radio Bursts. He also develops advanced photonic semiconductor and superconducting devices, including quantum-noise limited sensors and high-speed imaging sensors for biomedical applications. Education: PhD in Physics, University of Chicago BS in Physics, University of Toledo Research Interests: Professor Buckley explores the origins of cosmic rays, gamma-ray observations of active galaxies, and multiwavelength/multimessenger physics. He pioneered ground-based gamma-ray astronomy and is a leader in experimental cosmology, with a focus on dark matter detection through axion searches and gamma-ray signatures. His work bridges astrophysics and cutting-edge detector technology, such as superconducting thin films and parametric amplifiers for high-sensitivity experiments. Awards & Honors: 2020 Fellow of the American Physical Society 2016 Outstanding Referee for Physical Review Letters 2004 The Academy of Science of St. Louis Innovation Award 1998 Department of Energy Outstanding Junior Investigator Award 1997 Shakti Duggal Award (25th International Cosmic Ray Conference) 1996 Smithsonian Institution Special Achievement Award Grants & Leadership: As Principal Investigator (PI), he leads an NSF-funded project to enhance VERITAS’s optical monitoring capability and a DOE program developing NbTiN superconducting thin films. He is Spokesperson for the Advanced Particle-astrophysics Telescope (APT) mission concept and PI of the ADAPT suborbital mission (scheduled for 2025). His grants include a NASA Graduate Student Researchers Program grant (1989–1992) and collaborative roles with faculty like Murch and Henriksen on quantum sensors for ADMX. Labs & Collaborations: He is a founding member of the VERITAS experiment and the US-CTA consortium, and plays a key role in the ADMX collaboration. His involvement in the APT and ADAPT missions underscores his leadership in advancing space-based and ground-based gamma-ray探测技术.

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Matt Nichollمشاهده پروفایل

دانشیار

Queen’s University BelfastUnited Kingdom

Dr. Matt Nicholl is a Reader in the Astrophysics Research Centre at Queen's University Belfast's School of Mathematics and Physics. His research focuses on cosmic explosions, black holes, and extreme astrophysical phenomena such as supernovae, tidal disruption events, and gravitational wave counterparts. He utilizes global and space-based telescopes to study energetic events involving massive stars, neutron stars, and black holes. Dr. Nicholl is particularly interested in understanding the physical mechanisms behind luminous transients and their implications for stellar evolution and relativistic processes. Affiliations: Astrophysics Research Centre (ARC), Queen's University Belfast Media Experience: BBC Sky at Night, ITV, BBC World Service, and other national/international outlets His research interests span transient astrophysics, with a focus on supernovae, gamma-ray bursts, and tidal disruption events caused by supermassive black holes. He has led observational campaigns to identify optical counterparts to gravitational wave events and X-ray transients. Notable contributions include studies of the brightest supernova to date (SN 2018gvb) and the discovery of recurring tidal disruption events. Dr. Nicholl has received prestigious awards including the Royal Astronomical Society Penston Prize (2016), RAS Research Fellowship (2018), and a European Research Council Starting Grant (2020). His work has been widely covered in media, including features in The New York Times and BBC News. Labs/Teams: Leads observational programs in collaboration with international telescopes and contributes to surveys like Pan-STARRS and ZTF.

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Hsin-Yu Chenمشاهده پروفایل

استادیار

University of Texas at AustinUnited States

Hsin-Yu Chen is an Assistant Professor of Physics at the University of Texas at Austin, affiliated with the Weinberg Institute and Center for Gravitational Physics . Previously, she held positions as a NASA Einstein-MIT Kavli Institute Fellow and Black Hole Initiative Fellow at Harvard University. Her research focuses on gravitational waves , multi-messenger astrophysics , and the study of black holes and neutron stars . She actively participates in the LIGO Scientific Collaboration and the Dark Energy Survey-Gravitational Wave working group , aiming to discover electromagnetic counterparts of gravitational-wave signals. Her work integrates observational data from gravitational wave detectors with multi-wavelength astronomy. Key research themes include binary neutron star mergers , heavy element production , cosmological measurements of the Hubble constant , and signal detection algorithms for gravitational wave networks. She also explores the potential of future missions like LISA and Cosmic Explorer to advance gravitational wave astronomy. Her publications highlight advancements in detecting gravitational waves from compact binaries, analyzing calibration uncertainties in cosmological measurements, and investigating eccentric black hole mergers. Collaborations with DECam , Swift-BAT , and CHIME/FRB underscore her multi-faceted approach to multi-messenger astrophysics. Chen’s research has contributed to understanding the astrophysical origins of heavy elements and the cosmological implications of gravitational wave observations . She leads efforts in optimizing observational strategies for transient follow-up and refining detector network characterizations.

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Jens Hoeijmakersمشاهده پروفایل

مدرس ارشد

Lund UniversitySweden

Jens Hoeijmakers is an Associate Senior Lecturer in the Department of Physics at Lund University, specializing in astrophysics with a focus on exoplanet atmospheres and transmission spectroscopy. He is a Principal Investigator in the eSSENCE collaboration, contributing to projects like the ANDES spectrograph for the Extremely Large Telescope (ELT). His research explores atmospheric composition, dynamics, and chemistry of exoplanets, particularly ultra-hot Jupiters, using advanced instruments such as ESPRESSO and CRIRES+. He investigates topics like titanium chemistry, volatile/refractory ratios, and atmospheric oxidation processes, with implications for planetary habitability and formation. Collaborations include studies of exoplanet transits, stellar abundances, and the development of observational techniques for future missions. Key research interests include high-resolution spectroscopy, exoplanet dynamics, and the application of machine learning to spectral analysis. Notable projects include the HEARTS survey (Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy), the Mantis Network for template-based analyses, and the Hot Rocks Survey to study terrestrial exoplanets. His work bridges observational astrophysics with theoretical models, advancing understanding of planetary atmospheres and their evolution. Publications highlight contributions to exoplanet atmospheric characterization, including studies of WASP-121b, KELT-9b, and WASP-189b. He actively participates in international collaborations, leveraging cutting-edge instruments and methodologies to push the frontiers of exoplanet science.

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Hans Jakob Wörnerمشاهده پروفایل

استاد

ETH ZurichSwitzerland

Prof. Dr. Hans Jakob Wörner is a Full Professor of Physical Chemistry and Head of the Laboratory of Physical Chemistry at ETH Zürich's Department of Chemistry and Applied Biosciences. His research focuses on ultra-fast molecular spectroscopy with attosecond resolution (10 -18 s), aiming to characterize molecular valence shell dynamics through novel experimental methods. He leads the Atto Group, developing attosecond X-ray and laser spectroscopy techniques for studying electron and nuclear dynamics in liquids, clusters, and gases. Education: BSc (2003) and PhD (2007) in Physical Chemistry from ETH Zürich. Postdoctoral Work: Laboratoire Aimé Cotton (France) and National Research Council (Canada). Roles: Full Professor since 2013, ERC Consolidator Grant recipient (2017), and numerous international awards including the Coblentz Award (2018). Research interests include attosecond electron dynamics in molecules, liquids, and clusters; X-ray transient absorption spectroscopy; and intermolecular Coulombic decay in liquids. His lab pioneered attosecond techniques for imaging electron wave packets and studying conical intersection dynamics in aqueous systems. Awards: New Horizon Lectureship (2020) Coblentz Award (2018) ERC Consolidator Grant (2017) Carus Medal (2015) Young Academy Membership (2013) Lab & Collaborations: The Laboratory of Physical Chemistry at ETH Zürich focuses on ultrafast dynamics with state-of-the-art attosecond sources and liquid-jet technologies. Current projects explore proton transfer in aqueous solutions and Jahn-Teller effects in molecular cations.

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Chryssa Kouveliotouمشاهده پروفایل

استاد

George Washington UniversityUnited States

Chryssa Kouveliotou is a Professor of Physics at The George Washington University , specializing in High-Energy Astrophysics . Her research focuses on magnetars, gamma-ray bursts (GRBs), and other transient astrophysical phenomena. University: The George Washington University Academic Rank: Professor of Physics Contact: Email: Chryssa Kouveliotou | Office Phone: (202) 994-5898 Office Location: 411 Corcoran Hall, 725 21st St NW, Washington DC 20052 Her work in High-Energy Astrophysics includes detailed studies of magnetars' X-ray polarization, spectral evolution during outbursts, and their potential links to GRBs. She investigates transient events like giant flares and fast radio bursts (FRBs), using instruments such as Swift , Fermi/GBM , and NICER . Recent publications highlight advancements in understanding magnetar dynamics, GRB host galaxies, and high-redshift cosmology. Key topics include: Magnetar Outbursts: Timing analysis, spectral variability, and burst forest characterization. GRB Studies: Host galaxy constraints, kilonova searches, and jet structure analysis. Instrumentation: Contributions to missions like the High-Energy X-ray Probe (HEX-P) and Gamow Explorer. No scientific awards or student advising details were mentioned in the provided text.

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Matthew Evansمشاهده پروفایل

استاد

Massachusetts Institute of TechnologyUnited States

Matthew Evans is the MathWorks Professor of Physics at the Massachusetts Institute of Technology (MIT), leading research on gravitational wave detectors and next-generation observatories like Cosmic Explorer. He is affiliated with MIT's Kavli Institute for Astrophysics and Space Research and directs the Cosmic Explorer laboratory. His work focuses on improving Advanced LIGO sensitivity through low-thermal-noise coatings and quantum-optical control, including frequency-dependent squeezing techniques. Evans holds a B.S. in Physics from Harvey Mudd College (1996) and a Ph.D. from Caltech (2002). He contributed to LIGO/Virgo until 2007 before joining MIT's Advanced LIGO team. Since 2013, he has spearheaded technologies to enhance detector performance and leads the U.S. Cosmic Explorer initiative. His research interests span astrophysical instrumentation, quantum noise reduction in gravitational wave interferometers, and experimental methods for future observatories. Key awards include the 2019 New Horizons in Physics Prize, 2019 American Physical Society Fellowship, and a team Special Breakthrough Prize (2016) for LIGO's gravitational wave discoveries. Evans' advising and grants focus on advancing detector technologies and training next-generation researchers. His lab collaborates globally on Cosmic Explorer's design and deployment, aiming to detect gravitational waves from the earliest universe.

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