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Ubirajara van KolckView profile

Professor

• Effective Field Theory
• Nuclear Physics
• Particle Physics
• +3 more

Ubirajara (Bira) van Kolck is a Professor in the Department of Physics at the University of Arizona and an Affiliate Professor at the Department of Physics, University of Washington. His research focuses on Effective Field Theories (EFTs), particularly their applications to nuclear-particle physics interfaces and molecular systems. He earned his Ph.D. in Physics from the University of Texas at Austin (1993). Research Interests : Effective Field Theory, nuclear forces, chiral symmetry, and low-energy nuclear interactions. His work bridges particle and nuclear physics, emphasizing controlled expansions in strongly interacting systems. Awards : Alfred P. Sloan Research Fellowship (200?), Outstanding Junior Investigator Award (U.S. Department of Energy), APS Fellow (2004). Teaching : Courses include Nuclear Physics (PHYS 551) and PHYS 261H. He emphasizes research-driven pedagogy, including undergraduate projects on quantum mechanics and renormalization. Service : Past-Chair of APS Topical Group on Few-Body Systems, editorial board member of Progress in Particle and Nuclear Physics . Organized major workshops on Effective Field Theories at Caltech and the Institute for Nuclear Theory. Labs/Groups : Involved with the Nuclear Theory Group at UW and the University of Arizona's Nuclear Physics Group. Key collaborations include the Cooler-CSB experiment and RIA Theory Working Group.

Amit BhoonahView profile

Researcher

• Particle Physics
• Astrophysics
• Dark Matter Research
• +3 more

Amit Bhoonah is a Researcher at the University of Pittsburgh's Department of Physics & Astronomy, affiliated with the Dietrich School. His work focuses on particle physics, astrophysics, and dark matter research, with a particular emphasis on ultralight dark matter, gravitational waves, and experimental detection methods. His research interests span theoretical and experimental domains, including dark photon models, axion physics, and the interplay between particle physics and cosmology. He has contributed to studies on gravitational wave signatures from dark sectors, neutrino mass mechanisms, and laboratory constraints using atomic systems. Notable publications include investigations into sub-MHz radio backgrounds from dark photons, axion detection via Rydberg atoms, and constraints on boson stars using x-ray/gamma-ray observations. His work bridges fundamental theory with cutting-edge experimental techniques, addressing questions about dark matter's nature and its interactions with ordinary matter. While no specific awards are listed, his active publication record reflects a focus on advancing dark matter detection and particle physics frontiers. Collaborative efforts are evident in co-authored works with researchers like Simran Nerval and Ningqiang Song. No advising roles or grants are explicitly mentioned in the provided texts.

• Particle Physics
• Astrophysical Neutrinos
• Beyond the Standard Model
• +3 more

Roger Moore is a Professor and Chair in the Department of Physics within the Faculty of Science at the University of Alberta. His research focuses on particle physics, particularly neutrinos and astrophysical phenomena beyond the Standard Model. He leads the IceCube Neutrino Experiment at the South Pole, co-chairs its trigger-filter board, and is involved in developing the Pacific Ocean Neutrino Experiment (P-ONE) with international collaborators. Education: BA (1992), MA (1996), and PhD (1996) from the University of Cambridge, UK. Postdoctoral work at PPARC (1996-1997) and Michigan State University (1997-2003). Joined UofA in 2003, advancing from Assistant to Full Professor by 2013. Research interests include high-energy neutrino interactions, searches for dark matter, quantum gravity effects, and neutrino emission from cosmic sources like galaxy clusters and X-ray binaries. Recent publications emphasize IceCube data analyses for transient neutrino emissions, sterile neutrinos, and multi-messenger astrophysics. Awards include the PPARC Postdoctoral Fellowship (1996-1997). His work contributed to the Higgs boson discovery via the ATLAS Experiment at CERN and continues with cutting-edge neutrino observatories like IceCube-Gen2 and P-ONE. Lab affiliations include IceCube Collaboration, P-ONE, and past contributions to ATLAS. His team develops advanced reconstruction algorithms and detector technologies for neutrino science.

Rebecca SurmanView profile

Professor

• Nuclear Astrophysics
• Heavy Element Nucleosynthesis
• Neutron Star Mergers
• +2 more

Rebecca Surman is a Professor of Physics and Astronomy at the University of Notre Dame, specializing in nuclear astrophysics and heavy element nucleosynthesis. A Fellow of AAAS and APS, her research examines r-process element formation in neutron star mergers and supernovae. She received her PhD from UNC Chapel Hill and leads multiple NSF and DOE-funded projects. Research explores: Neutrino interactions in astrophysical environments Nuclear physics of exotic neutron-rich nuclei Kilonova light curve modeling R-process abundance patterns Honors include: AAAS and APS Fellowships Teaching prizes Major grants from NSF, DOE, and NEH Advises graduate students and postdocs in theoretical astrophysics and leads collaborative research networks including N3AS and NP3M.

Andrew MelatosView profile

Professor

• Gravitational Waves
• Neutron Stars
• Pulsar Timing
• +7 more

Andrew Melatos is a Professor in the School of Physics at the University of Melbourne, Australia. His research focuses on gravitational waves, neutron star astrophysics, superfluid dynamics, and interdisciplinary topics like econophysics and art-science collaboration. He has held senior roles in major collaborations such as OzGrav, LIGO, and the Texas Symposium Series. Melatos leads a dynamic research group producing cutting-edge work on pulsar glitches, magnetic mountains, and gravitational wave detection algorithms. His group has pioneered simulations of superfluid vortex avalanches and developed novel statistical methods for LIGO data analysis. Melatos has advised over 40 PhD and Master's students, many of whom now hold academic or industry leadership roles globally. His work bridges fundamental physics with applications in climate science, finance, and public outreach. Education: BSc (University Medal), University of Sydney (1988-1991) PhD in Physics, University of Sydney (1992-1995) Miller Fellow, UC Berkeley (1997-2000) Research Fellow, Caltech (1995-1997) Key Appointments: Chair, Texas Symposium Steering Committee (2006-2008) LIGO Scientific Collaboration Council (2014-present) Australia Telescope Time Assignment Committee (2002-2004) Research Themes: Melatos' work spans gravitational wave astrophysics, pulsar timing anomalies, superfluid turbulence in neutron stars, and interdisciplinary projects like econophysics modeling and art-science collaborations with visual artist Briony Barr. His group's recent breakthroughs include explaining pulsar glitch recovery via superfluid vortex dynamics and developing hidden Markov models for glitch detection. Publications & Impact: Over 15 key articles in areas like neutron star magnetospheres, LIGO signal processing, and econophysics. Notable collaborations include simulations of magnetic mountains and contributions to the historic 2017 gravitational wave-neutrino electromagnetic counterpart discovery.

• Gravitational Wave Physics
• General Relativity
• Astrophysics
• +4 more

Dr. David Rabeling is a Research Fellow at the Centre for Gravitational Astrophysics within the College of Science at the Australian National University. He is an active member of the LIGO Scientific Collaboration, contributing to numerous gravitational wave detection and analysis efforts. His work focuses on gravitational wave physics with emphasis on binary black hole and neutron star systems. Dr. Rabeling's research spans multiple areas of gravitational wave astronomy, including data analysis techniques for LIGO detectors, tests of general relativity using gravitational wave signals, and the study of binary compact object mergers. His work on the GW170817 event (the first observed binary neutron star merger) has been particularly significant, contributing to our understanding of neutron star properties, equation of state, and multi-messenger astronomy. He has developed expertise in gravitational wave signal processing, detector characterization, and the search for continuous and transient gravitational wave signals. His publication record demonstrates expertise in gravitational wave data analysis across multiple detector observing runs. A significant portion of his recent work focuses on the GW170817 event, examining it from multiple perspectives including tests of general relativity, neutron star equation of state constraints, and searches for electromagnetic counterparts. His research bridges theoretical predictions with observational gravitational wave data, contributing to our understanding of fundamental physics and astrophysical phenomena. As part of the Centre for Gravitational Astrophysics at ANU, Dr. Rabeling works within a team of researchers focused on gravitational wave detection and analysis. The Centre is part of the international LIGO Scientific Collaboration, giving him access to cutting-edge gravitational wave data and collaborative opportunities with researchers worldwide. His work contributes to Australia's growing role in gravitational wave astronomy and multi-messenger astrophysics.

• Gravitational Waves
• Physics
• Gravitational and Subatomic Physics
• +4 more

Sarah Caudill is a Researcher in the Gravitational and Subatomic Physics (GRASP) group within the Faculty of Science at Utrecht University. Her work focuses on gravitational wave astronomy, particularly in analyzing data from the LIGO, Virgo, and KAGRA detectors. She is an active contributor to major gravitational wave collaborations and has co-authored numerous significant publications in the field. Dr. Caudill's research spans multiple areas of gravitational wave physics, with a particular emphasis on data analysis techniques, detector characterization, and the search for various gravitational wave sources. Her work contributes to our understanding of compact binary systems, neutron stars, black holes, and other astrophysical phenomena detectable through gravitational waves. She has made significant contributions to the development of analysis methods for gravitational wave detection, including machine learning approaches and novel signal processing techniques. The recent publications by Dr. Caudill demonstrate a strong focus on improving gravitational wave detection capabilities, developing advanced analysis methods, and searching for diverse gravitational wave sources. Her work spans from detector characterization to the analysis of specific astrophysical events, showing both breadth and depth in gravitational wave research. Current trends in her research include the application of machine learning to gravitational wave data analysis, the development of more efficient waveform generation methods, and the search for exotic gravitational wave sources such as cosmic strings. Dr. Caudill has been involved in major gravitational wave discovery efforts, contributing to catalogs of detected events and analyses of detector performance. Her work helps advance the field of gravitational wave astronomy and contributes to our understanding of the universe through this new observational window.

• Particle and high energy physics
• Nuclear and plasma physics
• Astronomical sciences
• +4 more

Paolo Gondolo is a Professor in the Department of Physics & Astronomy at the University of Utah, where he has held appointments since 2009. His research spans particle physics, cosmology, and astrophysics, with a focus on dark matter, dark energy, and compact objects like gravastars. He earned his PhD in Physics from the University of California, Los Angeles in 1991 and has previously served as Associate Professor (2006–2009) and Assistant Professor at the University of Utah (2003–2006) and Case Western Reserve University (2000–2003). PhD, Physics, University of California, Los Angeles (1991) His research interests include Dark Matter , Primordial Black Holes , Gravitational Waves , Dark Energy , and High-Energy Astrophysics . He has pioneered theoretical frameworks for dark stars powered by dark matter annihilation and studied the interplay between cosmic structures and fundamental physics. His recent publications highlight gravitational wave signatures from preheating instabilities, dark matter phenomenology in nuclear scattering, and exotic compact objects like gravastars. These works integrate Cosmology , General Relativity , and Particle Physics . APS Fellowship (2006) for contributions to particle and astrophysical research Gondolo leads the Phun with Physics Outreach Program (founded 2006), engaging K-12 students in Utah through interactive science education. He also serves on the National Science Foundation Site Visit Team (2024) and teaches courses such as Intro To Particle Phycs and Quantum Field Theory I (2023).

• Astrophysics
• Gravitational Wave Astronomy
• Radio Astronomy
• +3 more

Iris de Ruiter is a postdoctoral researcher at the University of Sydney, affiliated with the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav). Her work focuses on analyzing ASKAP radio telescope data to identify exotic transients from compact objects like white dwarfs, neutron stars, and black holes. She develops software to detect these phenomena and conducts multi-wavelength follow-up studies to understand their physical properties and evolutionary processes. Additionally, she contributes to electromagnetic follow-up efforts for gravitational wave events, aiming to detect radio emissions from neutron star mergers. Her research bridges observational astronomy with theoretical astrophysics, emphasizing the interplay between radio transient detection and gravitational wave science. Key projects include studying binary systems and high-energy ejecta from cosmic mergers. No specific awards or formal student advisement roles are detailed in the provided information.

Ling SunView profile

Research Fellow

• Gravitational Wave Physics
• Neutron Stars
• Black Holes
• +3 more

Ling Sun is a Research Fellow at the Australian National University's Centre for Gravitational Astrophysics. Their work focuses on gravitational wave physics, neutron stars, black holes, and advanced detector technologies. They contribute to the LIGO and Virgo collaborations, specializing in data analysis for transient events and continuous wave searches. Research interests include gravitational wave detection methodologies, calibration uncertainties, and the interface between fundamental physics and observational astrophysics. They lead projects on ultralight boson searches and black hole spectroscopy, leveraging next-generation detector networks like Cosmic Explorer. Recent work emphasizes improving detector sensitivity through quantum noise suppression and exploring cosmological implications via Hubble constant measurements. Collaborations span global teams analyzing multi-messenger data from supernovae, magnetars, and fast radio bursts. Ling Sun co-leads the ANU team in the ARC Centre of Excellence for Gravitational Wave Discovery, advancing theoretical frameworks for exotic compact objects and gravitational wave signal interpretation.

Philip ChangView profile

Professor

• Theoretical Astrophysics
• Cosmology
• Supernovae
• +4 more

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.

Thomas CorbittView profile

Professor

• Experimental General Relativity
• Quantum Optomechanics
• Gravitational Wave Detection
• +2 more

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.

Øystein ElgarøyView profile

Professor

• Cosmology
• Astrophysics
• Dark Matter
• +4 more

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
• Cosmology
• Gravitational Wave Astronomy
• +3 more

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.

Zeynep DemiragliView profile

Associate Professor

• Particle Physics
• Dark Matter
• Higgs Physics
• +3 more

Zeynep Demiragli is an Associate Professor at Boston University, where she contributes to the Compact Muon Solenoid (CMS) experiment at CERN's Large Hadron Collider (LHC). Her research focuses on dark matter detection, Higgs boson physics, and advancing CMS detector technologies. She currently leads the development of Advanced Telecom Computer Architecture-based Data, Trigger, and Control (DTC) boards for the CMS inner tracker system as part of the High Luminosity LHC (HL-LHC) upgrade, ensuring efficient pixel data readout for critical physics analyses. Her work includes probing dark matter interactions in proton-proton collisions and analyzing missing transverse momentum signals. As convener of the CMS jet and missing transverse momentum physics group, she coordinates algorithm development and performance monitoring for object reconstruction. She is deeply involved in HL-LHC preparations, emphasizing detector robustness under high-luminosity conditions. Zeynep's research interests span experimental particle physics, high-energy collider dynamics, and the Standard Model's extensions. She explores phenomena like light-by-light scattering and axion-like particles in ultraperipheral collisions. Her contributions to WH production studies and top quark pair polarization also highlight her expertise in precision measurements. Her recent articles emphasize dark matter searches, Higgs boson decays, and detector optimization. Collaborations with the BU Electronics Design Facility and leadership in jet physics groups underscore her technical and organizational roles. No scientific awards were explicitly mentioned, but her work contributes significantly to foundational physics advancements. Her advising and grants activities are not detailed in the provided texts. She is affiliated with the CMS experiment team, HL-LHC upgrade initiatives, and the APOLLO ATCA blades project. Her lab involvement includes pixel detector testing and hardware development at Boston University's facilities.