جست‌وجوی استاد و پژوهشگر

• Neutrino Physics
• Astroparticle Physics
• High-Energy Astrophysics
• +۳ مورد دیگر

Assistant Professor Juan Pablo Yáñez Garza is affiliated with the Department of Physics at the University of Alberta and the Arthur B. McDonald Canadian Astroparticle Physics Institute. His research focuses on neutrino physics, particularly neutrino oscillations, atmospheric neutrino production, and dark matter detection through experiments like IceCube and P-ONE. University of Alberta, Department of Physics (2018–present) Banting Postdoctoral Fellowship (2016–2018) Postdoctoral Fellow, DESY-Zeuthen (2014–2016) PhD, Experimental Physics, Humboldt Universität zu Berlin (2014) Yáñez Garza’s research explores fundamental questions in neutrino physics, including oscillation parameters, neutrinoless double beta decay, and the origins of ultra-high-energy cosmic rays. He develops advanced detection technologies such as novel photodetectors and acoustic positioning systems for large-scale experiments like IceCube and the Pacific Ocean Neutrino Experiment. Scientific awards include the Banting Postdoctoral Fellowship . His work spans collaborations with IceCube, SNO+, and VERITAS, focusing on multimessenger astronomy and indirect dark matter searches. Current projects involve refining neutrino interaction models, improving cosmic ray composition analysis, and deploying next-generation detectors for high-energy neutrino studies.

• Quantum Chromodynamics
• High Energy Physics
• Nuclear Theory
• +۵ مورد دیگر

Raju Venugopalan is a Distinguished Scientist in the Physics Department at Brookhaven National Laboratory (BNL) and an Adjunct Professor at Stony Brook University. He has held these positions since October 2022 and March 2009, respectively. Previously, he served as Group Leader of the BNL Nuclear Theory group from 2010-2015 and 2016-2021, and as a Senior Scientist at BNL from 2007-2022. His academic journey began with a B.S. from the University of Chicago in 1987 and a Ph.D. from Stony Brook University in 1992, followed by postdoctoral appointments at the University of Minnesota, University of Washington, and Niels Bohr Institute. Dr. Venugopalan's research focuses on Quantum Chromodynamics (QCD) at high energies, with particular emphasis on the Color Glass Condensate (CGC) effective theory, quark-gluon plasma (QGP) formation in heavy ion collisions, and the theoretical foundations of the Electron-Ion Collider (EIC). His work bridges theoretical nuclear physics with connections to cosmology, condensed matter physics, and ultracold atomic systems. He has pioneered numerical and analytical techniques in real-time classical-statistical field theory and co-invented the IP-Glasma model for heavy ion collisions. His publication record includes over 180 papers with approximately 29,000 citations on INSPIRE (35,000 on Google Scholar), with an H-index of 81 (INSPIRE) and 92 (Google Scholar). Since 2010, he has published over 95 papers cited approximately 14,000 times, placing him among the most highly cited theorists worldwide. His most cited paper has about 2,360 citations and is recognized as a Physical Review D 50th Anniversary Milestone paper. Humboldt Research Award (Humboldt Prize, 2016-) BNL Science & Technology Award (2018) Suffolk County NY Distinguished Asian American Award (2019) Co-author of Phys. Rev. D 50th Anniversary Milestone Paper (2020) Fellow of the American Physical Society (2007-) Dr. Venugopalan has been instrumental in the development of the Electron-Ion Collider, having organized the first eRHIC workshop at BNL in December 1999. Today, the EIC is an approved DOE project under construction at BNL, with first collisions expected in the early 2030s. He currently serves as Director of the BNL EIC Theory Institute. His service includes membership on the APS Committee on Scientific Meetings (2023-2025), co-PI of the DOE SURGE Topical theory collaboration (2022-2027), and editorial roles for Annals of Physics (2013-2024) and SciPost (2019-).

Csaba Balazsمشاهده پروفایل

استاد

• Theoretical Particle Physics
• Cosmology
• Dark Matter
• +۵ مورد دیگر

Professor Csaba Balazs at the School of Physics and Astronomy, Monash University, is a leading theoretical particle physicist investigating cosmic connections between elementary particles and the Universe's evolution. His work bridges CERN's Large Hadron Collider experiments with astrophysical observations to unravel dark matter, dark energy, and fundamental force unification. Research Pillars : Dark Matter & Energy, Supersymmetry, Gravitational Waves, Higgs Physics Key Collaborations : Cherenkov Telescope Array, GAMBIT Collaboration Scientific Achievements include developing frameworks for interpreting LHC data and advancing dark matter detection through multi-messenger astronomy. His 2019-2020 computational grants enabled large-scale simulations for particle-cosmology interplay. Publications span collider phenomenology, dark sector studies, and cosmological phase transitions. He serves as Scientific Coordinator for GAMBIT and organizes astroparticle workshops, while contributing to journals like Universe and Frontiers in Physics as editor/reviewer.

Raymond Freyمشاهده پروفایل

استاد

• Astrophysics
• Gravitational Waves
• Experimental High Energy Physics
• +۶ مورد دیگر

Raymond Frey is a Professor in the Department of Physics at the University of Oregon, part of the College of Arts and Sciences. He has been a key member of the UO faculty since 1989 and leads research in gravitational wave detection and astrophysics as part of the LIGO Scientific Collaboration. His group focuses on data analysis and characterizing non-astrophysical noise in LIGO detectors. Ph.D., University of California, Riverside, 1984 Joined University of Oregon: 1989 Former Head of Physics Department (2012–2018) Raymond Frey's research centers on experimental high energy physics and astrophysics, particularly the detection of gravitational waves from cataclysmic events such as black hole and neutron star mergers. His work contributes to opening the new field of gravitational wave astronomy. He specializes in identifying and mitigating environmental noise in LIGO data and in conducting triggered searches for gravitational wave signals associated with gamma-ray bursts and supernovae. The recent publications reflect a strong focus on multi-messenger astrophysics, especially the landmark detections of GW150914 and GW170817. These works span areas including signal detection, noise characterization, parameter estimation, and tests of general relativity, with a clear trajectory toward understanding compact object populations and the nature of dense matter. Scientific recognition includes being part of the LIGO team awarded Science Breakthrough of the Year in 2016 and 2017 . These honors celebrate the first direct detection of gravitational waves and the first observation of a binary neutron star merger with electromagnetic counterparts. Raymond Frey has advised numerous graduate students in physics, including Matthew Ball, Adrian Helmling-Cornell, Sudarshan Karki, Kara Merfeld, Philippe Nguyen, Jordan Palamos, Vinny Roma, and Paul Schale. His group has been supported by research grants from the National Science Foundation and other agencies funding LIGO-related work. He has taught a wide range of courses, from introductory physics and astronomy to advanced topics like mathematical methods and electronics. The UO LIGO group, which he co-leads, conducts research both at the LIGO Hanford Observatory and on campus, focusing on data analysis and detector characterization. The team regularly collaborates with international partners within the LIGO Scientific Collaboration and participates in major discovery efforts.

• Quantum Chromodynamics
• Nuclear Theory
• Neutron Star Physics
• +۳ مورد دیگر

David B. Blaschke is a Senior Lecturer at the University of Wroclaw, with affiliations at Helmholtz-Zentrum Dresden-Rossendorf (HZDR), CASUS, and other institutions. His research spans nuclear theory, quantum chromodynamics (QCD), astrophysics, and condensed matter physics. His work focuses on the thermodynamics of quark-hadron matter, QCD phase transitions, neutron star structure, and applications of non-Hermitian quantum mechanics. He investigates hybrid star phenomenology, primordial black hole formation, and particle spectra in heavy-ion collisions. The 15 most recent articles highlight trends in QCD matter under extreme conditions, neutron star equation of state, and cosmological implications of the QCD transition. His collaborations include institutions like Coimbra University, Rostock University, and DESY. Blaschke's research is published in journals such as Physical Review D, Universe, and Physics Letters B, with topics ranging from quark-gluon plasma to astrophysical observations of compact stars.

Mariangela Lisantiمشاهده پروفایل

استاد

• Dark Matter
• Theoretical Particle Physics
• Astrophysics
• +۴ مورد دیگر

Mariangela Lisanti is a Professor of Physics at Princeton University, where she has been on the faculty since 2013 following her postdoctoral fellowship at the Princeton Center for Theoretical Science. Her work bridges theoretical particle physics, astrophysics, and data science to investigate fundamental questions about dark matter and cosmic structure. Education: B.A. in Physics from Harvard University (2005) Ph.D. in Physics from Stanford University (2010) Postdoctoral Fellowship at Princeton Center for Theoretical Science (2013) Lisanti's research centers on the Cold Dark Matter paradigm, examining how its variations manifest in galactic and sub-galactic scale observables through interdisciplinary approaches. Her group combines advanced numerical simulations with data analysis techniques to probe dark matter properties, leveraging computational methods to address challenges at the intersection of particle physics and cosmology. This work frequently incorporates machine learning and statistical modeling to interpret complex astrophysical datasets. Lisanti leads an active research group at Princeton University focused on designing and executing dedicated numerical simulations while developing novel data analysis frameworks. Though specific grant details aren't provided, her computational-intensive research implies substantial institutional and likely external funding support for high-performance computing resources and collaborative projects.

Salman Habibمشاهده پروفایل

پژوهشگر ارشد

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

Salman Habib serves as Division Director for the Computational Science Division at Argonne National Laboratory, with academic affiliations as Senior Associate of the Kavli Institute for Cosmological Physics at the University of Chicago and Senior Institute Fellow at the Northwestern Argonne Institute of Science and Engineering (a joint collaboration between Argonne and Northwestern University). Education: Undergraduate: Indian Institute of Technology, Delhi Ph.D.: University of Maryland (supervised by Bei-Lok Hu) Postdoctoral: University of British Columbia (with Bill Unruh) and Los Alamos National Laboratory His research spans cosmology, astrophysics, particle physics, quantum dynamics, and computational physics. With three decades of experience, he pioneered parallel supercomputing applications from 1990s Connection Machines to modern exascale systems. Current work focuses on advanced statistical methods and machine learning for cosmological inference using LSST and SPHEREx mission data. He actively contributes to the Legacy Survey of Space and Time Dark Energy Science Collaboration (LSST DESC) and NASA's SPHEREx science team. Students are explicitly welcomed to contact him for research opportunities.

Dmitry Budkerمشاهده پروفایل

استاد

• Experimental Atomic Physics
• Fundamental Interactions
• Symmetries
• +۳ مورد دیگر

Dmitry Budker is a Professor of Experimental Atomic Physics at Johannes Gutenberg University Mainz, affiliated with the Helmholtz Institute Mainz (HIM) and the GSI Helmholtz Center for Heavy Ion Research in Darmstadt. His research focuses on fundamental interactions and symmetries using atomic, molecular, and optical physics techniques, alongside developing optical sensors based on atomic vapor cells and zero/ultra-low field (ZULF) nuclear magnetic resonance. Education: 1963: Born in Russia. Studied physics at Novosibirsk State University, USSR, graduating with first-class honors. 1993: Earned PhD from the University of California, CA, USA. Budker's work spans precision measurements in atomic systems, quantum optics, and fundamental symmetry tests. His team's recent publications highlight advancements in parity violation studies, Bose-Einstein statistics validation, and constraints on fundamental constants' variation. His research group is actively involved in experimental atomic physics, optical sensor development, and ZULF NMR applications.

Jan Hamannمشاهده پروفایل

مدرس ارشد

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

Dr. Jan Hamann is a Senior Lecturer at the School of Physics , University of New South Wales, specializing in theoretical cosmology. His research focuses on analyzing high-precision astrophysical observations to study the universe's history, composition, and inflationary models. Education: PhD in Cosmology from Hamburg University (2007) Research Interests: Cosmic Microwave Background (CMB) analysis, inflationary features, dark matter (sterile neutrinos), cosmological parameter estimation, and machine learning applications to astrophysical data. Supervision: Primary supervisor for PhD students Yuqi Kang, Julius Wons, and Nathan Cohen; secondary supervisor for Kai Yi; and Honours supervisor for Jahanvi Maheshwari. Teaching: Courses include PHYS1241 Higher Physics 1B (Special) , PHYS4143 General Relativity , and PHYS3115 Particle Physics and the Early Universe . Recent publications (2024–2017) address CMB lensing, inflationary model optimization, sterile neutrino constraints, and machine learning techniques for cosmological data. He has contributed extensively to Planck mission analyses, particularly in CMB power spectra, isotropy tests, and inflationary parameter constraints.

• Gravitational Wave Astronomy
• Astrophysics
• Data Analysis
• +۳ مورد دیگر

Lilli Sun is a Research Fellow at the Centre for Gravitational Astrophysics within the Research School of Physics at the Australian National University. Her office is located in Physics North 1 76D, and she maintains an active research profile through her professional webpage at https://www.lingsun.org/. Dr. Sun's research focuses on gravitational wave astronomy, with expertise in data analysis techniques for the LIGO-Virgo-KAGRA collaboration. Her primary interests include the detection and analysis of gravitational waves from compact binary systems, neutron stars, and black holes. She has made significant contributions to major gravitational wave catalogs and multi-messenger astronomy efforts. Her publication record demonstrates expertise in advanced data analysis methods including hidden Markov models, cross-correlation techniques, and statistical inference approaches applied to gravitational wave data. Dr. Sun has been instrumental in numerous discoveries including binary black hole mergers, neutron star-black hole coalescences, and cosmological measurements using gravitational waves as 'standard sirens'. As an active member of the LIGO Scientific Collaboration, Dr. Sun contributes to multiple working groups focused on data analysis, detector characterization, and astrophysical interpretation of gravitational wave signals. Her work bridges theoretical astrophysics with practical data analysis challenges in one of the most exciting fields of modern physics.

Aaron Roodmanمشاهده پروفایل

استاد

• Observational Cosmology
• Dark Energy
• Large Optical Telescope Surveys
• +۵ مورد دیگر

Aaron Roodman is a Professor of Particle Physics and Astrophysics at Stanford's SLAC National Accelerator Laboratory, where he serves as the leader of the LSST Camera program and Deputy Director of the Rubin Observatory for construction. His research bridges experimental particle physics and observational cosmology, with significant contributions to understanding Dark Energy through large-scale astronomical surveys. Dr. Roodman received his B.S. with Honors in Physics from the California Institute of Technology in 1985 and his Ph.D. in Physics from the University of Chicago in 1991. His early career focused on experimental particle physics, studying differences between Matter and antiMatter for two decades before transitioning to astrophysics and cosmology. Roodman's research primarily centers on observational cosmology, with a focus on Dark Energy studies using data from large optical telescope surveys like the Dark Energy Survey. He has played a major role in the construction of the LSST Camera, the world's largest digital camera, for the Vera C. Rubin Observatory. His work combines advanced instrumentation development with cosmological analysis to probe fundamental questions about the universe's expansion and structure. His recent publications demonstrate a strong focus on large-scale cosmological surveys, particularly the Dark Energy Survey and the upcoming Legacy Survey of Space and Time (LSST). His research spans instrumental development for astronomical cameras, data analysis techniques for cosmological parameter estimation, and applications of machine learning to gravitational lensing and supernova cosmology. Fellow, American Physical Society, Division of Particles & Fields (2012) Professor Roodman actively mentors the next generation of scientists, serving as Doctoral Dissertation Advisor for Sydney Erickson and Theo Schutt, Doctoral Dissertation Reader for Sidney Mau and Guillem Megias i Homar, and Postdoctoral Research Mentor for Rebecca Chen. He has held significant leadership roles including Department Chair of Particle Physics & Astrophysics from 2015 to 2020. He leads major collaborative efforts including the LSST Camera program and is deeply involved with the Dark Energy Survey and Vera C. Rubin Observatory projects. His work brings together large international teams of scientists and engineers to advance our understanding of fundamental cosmic phenomena through cutting-edge observational techniques.

• Mathematical Physics
• General Relativity
• Cosmology
• +۳ مورد دیگر

Ali Kazım ÇAMLIBEL is an Assistant Professor at the Turkish-German University, Faculty of Engineering, Department of Electrical and Electronics Engineering. He completed his PhD and Master’s in Physics at Boğaziçi University, focusing on dark energy and cosmological models. His academic journey includes roles as Research Assistant at Boğaziçi University (2006) and Assistant Professor at Turkish-German University (2017–present). Doctorate: Boğaziçi University (2009–2016), Physics Master’s: Boğaziçi University (2006–2009), Physics Licence: Boğaziçi University (2000–2005), Physics His research spans mathematical physics, general relativity, and cosmology, with a focus on dark energy dynamics, supernova data analysis, and observational cosmology. He has also explored machine learning applications in cosmology, particularly in dark matter interactions and expansion history of the universe. Recent work includes phenomenological treatments of dark matter self-interactions (2025) and weak-field limits in modified gravity theories (2023). His publications analyze cosmological datasets, including Pantheon supernova data, and explore connections between dark matter, dark energy, and the universe’s expansion history. While his primary affiliation is with an Electrical and Electronics Engineering department, his research remains rooted in theoretical and observational cosmology.

• Astrophysics
• Cosmology
• Galaxy Formation and Evolution
• +۳ مورد دیگر

Viola Gelli is a Research Fellow at the Niels Bohr Institute, University of Copenhagen, specializing in the Cosmic Dawn Center (DAWN) where she investigates galaxy formation during the universe's first billion years. Her work combines James Webb Space Telescope (JWST) observations with theoretical modeling to study high-redshift phenomena including Population III galaxies and early star formation processes. Her research focuses on astrophysical processes at cosmic dawn, particularly bursty star formation, metallicity evolution in primordial galaxies, and feedback mechanisms from supernovae. She employs multi-wavelength JWST data to analyze galaxy clustering, stellar populations, and chemical enrichment in the reionization era, often developing novel statistical approaches for interpreting sparse high-z observations. Analysis of her eight recent publications reveals a cohesive research program centered on JWST's capabilities to probe the epoch of first galaxies. Her work consistently addresses how stellar feedback shapes early galaxy evolution, with particular emphasis on quenching mechanisms, metal-pollution signatures, and connections between high-z systems and local galaxy analogs. No scientific awards were documented in the available institutional materials. Gelli actively contributes to major international collaborations including the Lighter BEACON JWST survey consortium, where her expertise in pure-parallel imaging analysis informs survey design and data interpretation. Her research methodology integrates observational constraints with cosmological simulations to model galaxy formation under extreme high-redshift conditions. As a core member of the Cosmic Dawn Center, she participates in this Danish National Research Foundation-funded initiative that unites theoretical and observational efforts across multiple institutions to decode the physics of cosmic dawn through coordinated JWST programs and simulation campaigns.

• Astrophysics
• Cosmology
• Supernovae
• +۳ مورد دیگر

Radoslaw Jan Wojtak is an Associate Professor at the Niels Bohr Institute , University of Copenhagen, affiliated with the DARK Cosmology Centre. His research focuses on cosmological applications of supernovae and gravitational lensing, particularly addressing the Hubble constant tension through multi-messenger observations and statistical modeling. Institution: University of Copenhagen Research Unit: Niels Bohr Institute / DARK Email: radek.wojtak@nbi.ku.dk As a leading researcher in transient astrophysics, he develops Bayesian hierarchical models for Type Ia supernovae and investigates kilonovae as alternative distance indicators. His work leverages LSST and Hubble Space Telescope data to constrain cosmological parameters through strongly lensed supernova systems. His recent publications analyze: γ-ray attenuation methods for H₀ measurement Extinction models in Cepheid calibration galaxies LSST lensing detection techniques Expanding photosphere method for kilonovae Current collaborations span institutions in 15+ countries, with research outputs generating media coverage and social media engagement. No formal awards or student advisement details are publicly documented in the scraped materials.

• Theoretical Physics
• Cosmology
• Particle Physics
• +۳ مورد دیگر

Guido D'Amico serves as an Associate Professor in the Department of Mathematical, Physical and Computer Sciences at the University of Parma. His teaching portfolio includes advanced courses such as Advanced General Relativity (for Master's in Physics), Theory of Fundamental Interactions (Master's level), and foundational Physics courses for Engineering undergraduates, reflecting a strong commitment to both theoretical and applied physics education. Dr. D'Amico's research centers on theoretical cosmology with emphases on: Effective Field Theory applications to Large-Scale Structure (LSS) Primordial non-Gaussianities and inflationary models Dark energy and modified gravity Analysis of galaxy clustering data from surveys like BOSS and Euclid Computational methods for cosmological parameter estimation His work bridges high-energy theory and observational cosmology to address fundamental questions about the universe's evolution. His recent publications (2023-2025) demonstrate a focused trajectory in refining EFTofLSS for precision cosmology. Key themes include: Modeling nonlinear scales in galaxy clustering Constraints on quintessence and dark energy Primordial non-Gaussianity bounds from galaxy data Development of emulators and statistical methods for LSS analysis Contributions to the Euclid mission's cosmological pipelines These efforts position him at the forefront of extracting cosmological insights from next-generation surveys. No scientific awards were documented in the source materials. Information regarding graduate student mentorship, research funding, or laboratory affiliations was not provided in the available texts.