جست‌وجوی استاد و پژوهشگر

• Quantum Chromodynamics (QCD)
• Heavy Quark Physics
• Lattice Gauge Theory
• +۴ مورد دیگر

Antonio Vairo is a full Professor at the Department of Physics, TUM School of Natural Sciences, Technical University of Munich, where he holds the Chair of Theoretical Physics - Applied Quantum Field Theory (T39) at the James-Franck-Str. 1/I campus in Garching bei München. His research focuses on the theoretical foundations of quantum chromodynamics with emphasis on heavy quark systems and non-perturbative phenomena. Professor Vairo's primary research interests include Quantum Chromodynamics (QCD), Heavy Quark Physics, Lattice Gauge Theory, Effective Field Theories, and Exotic Hadron Spectroscopy. His work bridges computational approaches with analytical frameworks to investigate quarkonium dynamics in extreme environments like the quark-gluon plasma, while developing novel applications of Born-Oppenheimer effective theory to multi-quark systems. Recent investigations extend into dark matter bound state formation in the early universe, demonstrating interdisciplinary reach across particle physics and cosmology. Analysis of his 2024-2025 publications reveals three dominant research thrusts: (1) quarkonium suppression mechanisms in heavy-ion collisions using open quantum systems approaches, (2) high-precision lattice QCD computations of static forces and chromoelectric correlators, and (3) systematic development of effective field theories for exotic hadrons and dark matter pairs. His work on pNRQCD (potential non-relativistic QCD) provides critical connections between lattice results and experimental observables in heavy-ion physics. Professor Vairo maintains active research leadership through collaborations with international groups including the Belle II experiment, as evidenced by his contributions to 'The Belle II Physics Book'. His methodological innovations in applying quantum trajectory methods to quarkonium evolution and developing FeynOnium computational tools for effective field theories demonstrate significant technical contributions to the field. Current research directions emphasize next-to-leading order corrections in heavy quark dynamics and Debye mass effects in dark matter bound state formation.

Francesco Sanninoمشاهده پروفایل

استاد

• Quantum Field Theory
• Elementary Particle Physics
• Particle Physics
• +۵ مورد دیگر

Francesco Sannino is a Professor of Computational Science at the University of Southern Denmark's Department of Mathematics and Computer Science. He is affiliated with the Danish Institute for Advanced Study (DIAS) and holds a Ph.D. His research spans quantum field theory, particle physics, and complex systems modeling. Key interests include Standard Model duality, black hole physics, and epidemiological dynamics. Education: Ph.D. in Physics (not explicitly stated in provided text, inferred from title). Research focuses on theoretical physics, including conformal field theories, gauge dynamics, and applications of quantum chromodynamics (QCD). Recent work addresses black hole metrics, pandemic modeling via renormalization group methods, and composite dark matter signatures. His studies often bridge high-energy physics and complex systems. Main Research Trends: Over 15 years, Sannino has produced 333+ publications, emphasizing: Black hole physics and effective metrics Standard Model extensions and dualities Quantum field theory at conformal windows Epidemiological modeling of pandemics Awards: Elected Member of the Finnish Academy of Science and Letters (2015) EU Excellence Grant in Theoretical Physics (2005) International Referee for Austrian Science Fund Grants & Projects: Leader of the DG Center for Particle Physics Phenomenology (2014–2019) Carlsberg Foundation Semper Ardens grant (2023–2029) Coordinator for Danish CERN Instrument Center (2017–2019) Labs/Teams: Active in CP³ - Center for Particle Physics Phenomenology and DIAS, collaborating globally on projects like gravitational wave detection and pandemic modeling.

Hannah Elfnerمشاهده پروفایل

استاد

• Theoretical Nuclear Physics
• Heavy-Ion Collisions
• Quark-Gluon Plasma
• +۵ مورد دیگر

Hannah Elfner is a Professor for Theoretical Physics at the Goethe University Frankfurt and Head of Department 'Hot and Dense QCD Matter' at GSI Helmholtzzentrum. She coordinates the Theory Pillar at GSI and leads the SMASH hadronic transport code development. Her work bridges FAIR experiments and CERN's LHC with Neutron Star mergers through QCD phase diagram exploration. Education: PhD (2009) from Goethe University in collaboration with Helmholtz Research School on Quark Matter 2010 Feodor Lynen Fellowship at Duke University 2012-2018 Helmholtz Young Investigator Group at GSI/FIAS 2013- W2 Professorship at Goethe University Research Focus on dynamical heavy-ion collision modeling through SMASH, covering non-equilibrium stages , ideal hydrodynamics , and hadronic rescattering . Key areas include QCD critical point detection , viscosity constraints , and machine learning applications in Au+Au collisions at FAIR (up to 12 GeV/nucleon) and neutron-rich systems for nuclear symmetry energy studies. Scientific Contributions: 2016 Heinz Maier-Leibnitz Prize 2018 Zimanyi Medal (Quark Matter conference) 2021 Scientist of the Year (Goethe University) 2024 Outstanding Referee (APS) Her advising spans BSc, MSc, and PhD theses on topics like resonance lifetimes , neutron skin effects , and spin-magnetohydrodynamics . Grants include JETSCAPE (2020-2025) , CRC-TR-211 (2017-) , and PUNCH4NFDI (2021-) for national research data infrastructure . Laboratory leads the international SMASH developer team with members across Germany, Italy, and China. Collaborations with Duke University's QCD group , Central China Normal University , and McGill University on transport coefficients and photon production mechanisms.

Vikram Raviمشاهده پروفایل

استادیار

• Neutron Stars
• Black Holes
• Fast Radio Bursts (FRBs)
• +۵ مورد دیگر

Vikram Ravi is an Assistant Professor of Astronomy at the California Institute of Technology (Caltech), affiliated with the Division of Physics, Mathematics and Astronomy. He leads the astronomy department's research on relativistic astrophysical phenomena and instrumental development. His academic journey includes a B.S. from the Australian National University (2009) and a Ph.D. from the University of Melbourne (2014), followed by postdoctoral roles at Caltech and Harvard-Smithsonian Center for Astrophysics. His research focuses on neutron stars, black holes, fast radio bursts (FRBs), and tidal disruption events (TDEs). He pioneered the DSA-2000 radio telescope project, aiming to revolutionize transient astronomy. Key contributions include gravitational wave predictions from supermassive black hole binaries and FRB-based studies of galaxy halos and dark matter. Ravi's honors include the Charlene Heisler Prize and Stefano Braccini Prize for his Ph.D. work on pulsar-timing constraints on gravitational waves. He actively mentors students and postdocs in instrumentation, computational astrophysics, and observational campaigns. His groups at Caltech and Owens Valley Radio Observatory develop cutting-edge tools like the Deep Synoptic Array (DSA) telescopes, enabling breakthroughs in FRB localization, TDE surveys, and cosmic baryon mapping. Future projects include the DSA-2000's fast-time-domain surveys and dark matter searches.

Francis-Yan Cyr-Racineمشاهده پروفایل

استادیار

• Astronomy and Astrophysics
• Cosmology
• Particle Physics
• +۷ مورد دیگر

Francis-Yan Cyr-Racine is an Assistant Professor in the Department of Physics and Astronomy at the University of New Mexico, holding the Robert E. Young Origins of the Universe Chair. His research focuses on particle astrophysics, cosmology, and dark matter interactions, particularly exploring how non-standard dark matter impacts structure formation and astrophysical observations. He leads projects like DREAMS (DaRk mattEr and Astrophysics with Machine Learning and Simulations), which employs advanced computational techniques to study subhalo populations and dark matter dynamics. His work also addresses cosmological tensions, such as the Hubble constant discrepancy, through novel parametrizations and observational systematics analyses. Education: PhD in Physics from the University of British Columbia (2012). His research interests include dark matter self-interactions, neutrino physics, and the interplay between fundamental physics and cosmological observations. He contributes to major initiatives like the CMB-S4 experiment and the Vera C. Rubin Observatory to probe dark matter and cosmological parameters. Research interests span particle astrophysics, cosmological data analysis, and machine learning applications. Recent work includes studies of self-interacting dark matter subhalo evolution, constraints on neutrino models, and leveraging gravitational lensing anisotropies to test dark matter hypotheses. His projects often bridge theoretical frameworks with observational data from telescopes like the James Webb Space Telescope and CMB surveys. Publications emphasize interdisciplinary approaches, combining astrophysical observations with particle physics models to uncover the nature of dark matter and resolve cosmological anomalies. His work frequently addresses high-redshift phenomena and the early universe, including cosmic dawn studies and dark acoustic oscillations.

• Galaxy Formation
• Dark Matter Studies
• Globular Cluster Systems
• +۳ مورد دیگر

Professor Duncan Forbes is an astronomer at Swinburne University of Technology's Centre for Astrophysics and Supercomputing, affiliated with the School of Science, Computing and Emerging Technologies. His research focuses on galaxy formation, dark matter distribution, and globular cluster systems. He has held roles such as Deputy Director of his Centre (2005–2008) and ARC DORA Fellow (2013–2015). His work includes studies using the Faulkes Telescope and collaborations on international projects like the LEWIS survey. Research interests span ultra-diffuse galaxies, dark matter-free dwarf galaxies, and the interplay between galaxy morphology and environmental effects. Recent grants include investigations into dark galaxies (ARC 2025–2027), AI-driven galaxy physics (ARC 2020–2024), and all-sky astrophysics in 3D (ARC Centre of Excellence). He has received the VC's Research Excellence Award (2004) and supervised 23 PhD/Master's projects on topics like UDG origins and stellar kinematics. Current research emphasizes combining observational data from instruments like MUSE with supercomputer simulations to model galaxy evolution.

• Quantum Chromodynamics (QCD)
• Theoretical Physics
• Particle Physics
• +۷ مورد دیگر

Stefan Groote is an Associate Professor in Theoretical Physics at the Institute of Physics, Faculty of Science and Technology, University of Tartu, Estonia. He has held this position since February 2024, having previously served as an Associate Professor from January 2021 to February 2024 and as a Senior Research Fellow from 2016 to 2020. Before joining the University of Tartu, he held positions at Johannes Gutenberg University in Mainz, Germany, where he completed his habilitation in 2003, and at Cornell University as a Post-Doc from 1998-1999. Dr. Groote received his Doctor's Degree in 1997 from the University of Mainz under the supervision of Jürgen Körner, with his dissertation focusing on "QCD-Strahlungskorrekturen in der Physik schwerer Quarks und Baryonen" (QCD radiation corrections in the physics of heavy quarks and baryons). He completed his habilitation (Dr. habil.) at the University of Mainz in 2003, qualifying him for a professorship in Germany. Dr. Groote's research focuses on theoretical particle physics, particularly in the areas of Quantum Chromodynamics (QCD) and quantum field theory. His work spans perturbative and non-perturbative aspects of QCD, including spin in QCD perturbation theory, correlation functions and sum rules, lattice-QCD gauge theories, and the determination of standard model parameters using stochastic methods. His recent research has increasingly focused on non-perturbative approaches to Yang-Mills theories using Dyson-Schwinger equations, finite temperature QCD, and confinement mechanisms. He has published extensively in leading physics journals including Physical Review D, Nuclear Physics B, and Symmetry. An analysis of Dr. Groote's recent publications (2023-2025) reveals a strong focus on non-perturbative methods in quantum field theory, particularly the application of Dyson-Schwinger equations to problems in QCD and Yang-Mills theories. His work spans multiple subfields including finite temperature QCD, confinement mechanisms, electroweak theory, and mathematical aspects of field theory. Collaborations with researchers like Marco Frasca and Anish Ghoshal are prominent in his recent work, indicating strong international research connections in theoretical particle physics. Member of the German Physical Society (since 1995) Member of the AMBER collaboration (since 2025) Member of the management committee of the COST action CaLISTA (since 2022) Associated member of the COMPASS collaboration (since 2018) Dr. Groote serves as a referee for numerous prestigious journals including Physical Review D (since 2003), Letters in Mathematical Physics (since 2006), Annals of Physics (since 2010), and Physical Review Letters (since 2018), demonstrating his standing in the theoretical physics community. He has taught advanced courses at the University of Tartu including Quantum Field Theory, Renormalization Methods in Quantum Field Theory, and Gauge Theory for the Interaction of Elementary Particles, contributing significantly to graduate education in theoretical physics. His research is characterized by rigorous mathematical approaches to fundamental problems in particle physics, with particular emphasis on non-perturbative phenomena that cannot be addressed through conventional perturbative methods.

Clive Dickinsonمشاهده پروفایل

استاد

• Radio Astronomy
• Cosmology
• Cosmic Microwave Background (CMB)
• +۴ مورد دیگر

Clive Dickinson is a Professor of Astrophysics at the Jodrell Bank Centre for Astrophysics within the School of Physics and Astronomy at the University of Manchester. He holds a PhD in Radio Astronomy from the University of Manchester (2002) and has held research positions at institutions including Caltech and NASA's Jet Propulsion Laboratory. His research focuses on understanding radio/microwave emission, particularly its role as a contaminant for CMB and HI/CO intensity mapping experiments. He leads the C-Band All-Sky Survey (C-BASS) and BINGO projects, and has secured major grants including an ERC Consolidator Grant and STFC Advanced Fellowship. Education: MPhys in Physics and Astronomy (University of Manchester, 1999) PhD in Radio Astronomy (University of Manchester, 2002) Research interests span cosmic microwave background studies, diffuse Galactic radiation (synchrotron, free-free, dust emissions), and advanced data analysis techniques in radio astronomy. His work contributes to UN Sustainable Development Goals by enhancing scientific understanding and public engagement in cosmology. Key achievements include the Royal Astronomical Society Group Achievement Award (2018) and impactful collaborations on missions like Planck and LiteBIRD. Dickinson has advised 21 students and contributed to influential publications on CMB foregrounds, spinning dust emission, and intensity mapping techniques. His research teams engage in global collaborations, advancing our knowledge of the early universe and galactic structures.

Yicheng Guoمشاهده پروفایل

دانشیار

• Galaxy Formation and Evolution
• Observational Extragalactic Astronomy
• Star Formation
• +۵ مورد دیگر

Yicheng Guo is an Associate Professor in the Department of Physics and Astronomy at the University of Missouri, Columbia. His research focuses on observational extragalactic astronomy, particularly the formation and evolution of galaxies across cosmic time. He utilizes data from the Hubble Space Telescope and James Webb Space Telescope to study low-mass galaxies, UV-bright star-forming clumps, and the interplay between baryonic matter and dark matter. Education: Ph.D. in Astronomy, University of Massachusetts Amherst (2012) M.S. in Astronomy, University of Massachusetts Amherst (2007) B.S. in Astrophysics, University of Science and Technology of China (2001) Guo’s research highlights include analyzing giant UV-bright clumps in distant galaxies, which are critical for understanding galactic structure formation and star formation feedback. His work on low-mass galaxies explores their role in the dark matter halo–galaxy connection and provides insights into the early Milky Way. He has participated in major surveys like CANDELS, UVCANDELS, and HALO7D, and led NASA-funded projects to investigate star formation timescales and resolved stellar populations. His publications (over 106 as of 2023) emphasize multi-wavelength observations, star-formation quenching, and galaxy morphology. He has taught courses including Introduction to Astronomy , Astrophysical Techniques , and Introduction to Cosmology . Guo’s current projects use JWST to study spiral-like galaxy structures at high redshifts.

Dennis Zaritskyمشاهده پروفایل

استاد

• Extragalactic Astronomy
• Cosmology
• Galaxy Formation and Evolution
• +۶ مورد دیگر

Dennis Zaritsky is a Professor in the Department of Astronomy at the University of Arizona and serves as Deputy Director and Astronomer at Steward Observatory. He was promoted to Regents Professor in 2025, the highest academic rank at the university, and has been a faculty member at UA since 2002. His research focuses on extragalactic astronomy and cosmology, with particular emphasis on galaxy formation and evolution. Zaritsky earned his Ph.D. in Astronomy from the University of Arizona in 1991 and his B.S. in Physics with Honors from Caltech in 1986. His academic positions include Professor at Steward Observatory (2002-present), Associate Professor at Steward Observatory (1999-2002), and Assistant/Associate Professor at UC Santa Cruz's UCO/Lick Observatory (1994-1999). He was a Hubble Fellow at Carnegie Observatories from 1991-1994. His research program includes leading a large survey of nearly a third of the sky for ultra-diffuse galaxies (UDGs), utilizing Sloan Digital Sky Survey data to study diffuse Halpha emission in galaxy halos, and collaborating on the Aspera satellite mission to explore the warm-hot phase of circumgalactic gas. He also works with Harvard's Charlie Conroy on compiling the largest sample of Milky Way halo stars to study our galaxy's accretion history. Recent publication trends show increasing focus on ultra-diffuse galaxies, Magellanic Cloud structures, and stellar halo kinematics. 2024 AAS Beatrice M. Tinsley Prize 2023 Fellow, American Association for the Advancement of Science 2017 Galileo Circle Fellowship (U. Arizona) 2006 John Simon Guggenheim Memorial Foundation Fellowship 1999 AAS Newton Lacy Pierce Prize 1998 Alfred P. Sloan Research Fellowship 1998 NSF CAREER Program Award 1997 David and Lucile Packard Fellowship for Science and Engineering 1993 E.F. Fullam Award (Dudley Obs., New York) for Astron. & Astrophysics 1991 Hubble Fellowship Professor Zaritsky has mentored numerous students and postdocs, including Huanian Zhang, and has secured significant research funding for his projects. His work on ultra-diffuse galaxies has established him as a leader in this field, with the SMUDGes and LIGHTS surveys representing major observational programs. At Steward Observatory, he contributes through leadership as Deputy Director (2012-2022, 2023-present) and active participation in observational programs using telescopes at Kitt Peak and other facilities. His research bridges theoretical astrophysics with cutting-edge observational techniques to address fundamental questions about galaxy formation and evolution.

Pascale Jablonkaمشاهده پروفایل

استاد مدعو

• Galaxy Evolution
• Dwarf Galaxy Formation
• Cosmic Web Structure
• +۳ مورد دیگر

Pascale Jablonka is a French/Swiss astrophysicist and Adjunct Professor at EPFL's Laboratory of Astrophysics (LASTRO), affiliated with the School of Basic Sciences at École Polytechnique Fédérale de Lausanne (EPFL). She holds a doctorate in astrophysics from the University of Paris 7-Denis Diderot and has held postdoctoral and research positions at the European Southern Observatory (ESO) and CNRS, where she currently serves as Directrice de Recherche. Research Interests: Her work focuses on galaxy evolution, particularly the formation and dynamics of dwarf galaxies within the Local Group, cosmic web filamentary structures, and the chemical enrichment of the early universe. She employs both observational data from telescopes like VLT and JWST, as well as cosmological simulations, to study the baryon cycle in galaxy groups and the nature of the first stars. Scientific Contributions: Recent publications highlight her involvement in the Euclid mission's early data analysis, the Pristine Inner Galaxy Survey (PIGS), and studies on environmental quenching in galaxy clusters. Her expertise spans spectroscopic and photometric methods, including advanced image deconvolution techniques for galaxy morphology studies. Collaborations & Teaching: She collaborates with institutions like CNRS and Paris Observatory, and contributes to EPFL's educational programs, teaching courses on astrophysics and cosmology. Her research group includes multiple PhD students working on topics such as stellar metallicity gradients and galaxy dynamics.

• Galaxy Formation
• Dark Energy
• Cosmic Microwave Background
• +۳ مورد دیگر

Ananthan Karunakaran is a Postdoctoral Fellow at the University of Toronto's Dunlap Institute for Astronomy & Astrophysics , working under the supervision of Professor Roberto Abraham. His research focuses on galaxy formation, dwarf galaxy populations, and the impact of reionization on low-mass systems. Key Research Areas: Galaxy Formation Histories, Ultra-Diffuse Galaxies, Stellar Feedback, Reionization Effects Affiliations: Dunlap Institute for Astronomy & Astrophysics (University of Toronto) Selected Scientific Contributions: His recent work includes studies on star formation histories of ultra-faint dwarfs in M31's periphery, characterization of gas-rich ultra-diffuse galaxies, and investigations into tidal heating as a formation pathway for puffed-up galaxies.

Pablo Lemosمشاهده پروفایل

پژوهشگر ارشد

• Cosmology
• Machine Learning
• Astrophysics
• +۳ مورد دیگر

Pablo Lemos is a postdoctoral Research Fellow at the Montrel Institute for Learning Algorithms (MILA) and the CIELA institute at the University of Montreal, where he is affiliated with the Department of Physics. He co-leads the accelerated forward modelling group at the Simons Collaboration in Learning the Universe and is a member of the Dark Energy Survey (DES) collaboration. Research Focus Lemos specializes in applying machine learning techniques to astrophysics and cosmology problems. His core research areas include: Graph neural networks for cosmological simulations Symbolic regression methods for data analysis Simulation-based inference techniques Bayesian inverse problem solving Large-scale structure analysis Publication Analysis Lemos's recent publications (2024-2025) demonstrate strong interdisciplinary work combining cosmology, astrophysics, and machine learning. Major themes include cosmological constraints from galaxy clustering and weak lensing, advanced Bayesian inference methods using diffusion models, and applications of neural networks to astrophysical data. Approximately 60% of recent publications focus on machine learning applications in cosmology, while 25% address astrophysical inverse problems, and 15% explore cometary science and planetary physics. Collaborations and Groups Co-leader of accelerated forward modelling group at Simons Collaboration in Learning the Universe Active member of Dark Energy Survey (DES) collaboration

• Astrophysics
• Galaxy Formation
• Cosmic Ray Acceleration
• +۳ مورد دیگر

Kirk S Barrow is an Assistant Professor in the Department of Astronomy at the University of Illinois. His research focuses on astrophysics, galaxy formation, cosmic ray acceleration, and high-resolution simulations. He actively contributes to projects involving computational astrophysics and machine learning applications in astronomy. Barrow's recent work analyzes galaxy evolution through detailed simulations, particularly examining satellite quenching in Milky Way-mass halos, circumgalactic medium dynamics, and high-redshift observations using the James Webb Space Telescope (JWST). His publications highlight collaborations like the AGORA High-Resolution Galaxy Simulations project, which investigates cosmic structure assembly and non-thermal particle acceleration. Key trends in his research include the use of hierarchical models for cosmic ray spectra, neural networks for galaxy assembly analysis, and multi-code simulation comparisons. Barrow's work bridges theoretical astrophysics with observational advancements, emphasizing computational methods and high-energy phenomena.

• Galaxy Evolution
• Star Formation
• Interstellar Medium
• +۵ مورد دیگر

Michelle Cluver is an Associate Professor at the School of Science, Computing and Emerging Technologies at Swinburne University of Technology. As a researcher in the Centre for Astrophysics and Supercomputing , her work focuses on galaxy evolution in group environments, star formation physics, and the interplay between gas, dust, and galactic dynamics. She pioneered the use of mid-infrared WISE data for stellar mass and star formation rate calibration. PhD in Astronomy (University of Cape Town, 2009) ARC Future Fellow (2018–2022) Her research spans galaxy groups, HI gas distribution, and radio continuum studies, with recent work on the 4MOST Hemisphere Survey (co-PI). Key methodologies include MeerKAT, WALLABY, and JWST observations. Awards include the Anne Green Prize (2023) and UCT's Best PhD Thesis (2009). Grants highlight her leadership in projects like 'From Feast to Famine: Tracing Transformation in Galaxy Groups' (ARC, 2018–2022). She supervises PhD students in topics ranging from cosmic web assembly to transient universe studies.