Louise Skinnari
Searching for needles in the haystack at the LHC and beyond
Abstract:
The Large Hadron Collider (LHC) is the world’s most energetic particle accelerator complex, colliding protons at close to the speed of light. The LHC provides an extremely powerful tool to address fundamental questions about our Universe, including the nature of dark matter, the observed matter-antimatter asymmetry, and the origin of the large difference between the electroweak and Planck energy scales. The LHC is scheduled to be upgraded to its high luminosity counterpart (HL-LHC) in a few years. The HL-LHC will significantly increase the intensity of the proton collisions, in turn enabling the LHC experiments to collect immense data sets to measure properties of the Higgs boson is great detail, probe very rare Standard Model processes, and search for signs of new physics beyond the well-established Standard Model. The increase in intensity, although scientifically exciting, comes at the price of extremely challenging experimental data-taking conditions. These are particularly challenging for the real-time data filtering ('trigger') systems that are responsible for deciding which collision events to read out and store for later analysis. In this colloquium, I will discuss the motivation and physics potential of the high luminosity LHC upgrade, as well as some of the associated experimental challenges, in particular in the context of the CMS experiment's trigger system.
Katie Bouman
Seeing Beyond the Blur: Imaging Black Holes with Increasingly Strong Assumptions
Abstract:
At the heart of our Milky Way galaxy lies a supermassive black hole called Sagittarius A* that is evolving on the timescale of mere minutes. This talk will present the methods and procedures used to produce the first images of Sagittarius A* as well as discuss future directions we are taking to leverage machine learning to sharpen our view of the black hole, including mapping its evolving environment in 3D. It has been theorized for decades that a black hole will leave a "shadow" on a background of hot gas. However, due to its small size, traditional imaging approaches require an Earth-sized radio telescope. In this talk, I discuss techniques we have developed to photograph a black hole using the Event Horizon Telescope, a network of telescopes scattered across the globe. Recovering an image from this data requires solving an ill-posed inverse problem which necessitates the use of image priors to reduce the space of possible solutions. Although we have learned a lot from these initial images already, remaining scientific questions motivate us to improve this computational telescope to see black hole phenomena still invisible to us. In particular, we will discuss approaches we have developed to incorporate data-driven diffusion model priors into the imaging process to sharpen our view of the black hole and understand the sensitivity of the image to different underlying assumptions. Additionally, we will discuss how we have developed techniques that allow us to extract the evolving structure of our own Milky Way's black hole over the course of a night. In particular, we introduce Orbital Black Hole Tomography, which integrates known physics with a neural representation to map evolving flaring emission around the black hole in 3D for the first time.
Shu-Heng Shao
Non-invertible symmetries: From Ising Model to Pion Decay
Abstract:
I will discuss recent developments on a novel kind of global symmetry, the non-invertible symmetry. It is implemented by conserved operators that do not have an inverse, going outside the paradigm set by Wigner's theorem. I will start with the example in the Ising lattice model, and then discuss applications in pion decay and axion physics.
hosted by:Philip Harris
Ibles Olcina Samblas
New constraints on WIMP dark matter from the LUX-ZEPLIN (LZ) experiment
Abstract:
Dark matter detection experiments based on liquid xenon time projection chambers have been steadily increasing in sensitivity to the weakly interacting massive particle (WIMP) over the past two decades. The LZ experiment, employing a two-phase xenon time projection chamber containing 7,000 kilograms of liquid xenon, currently leads the way. Recently, the collaboration released new results from a combined analysis using data from the 2022 and 2024 science campaigns, amounting to a live exposure of 4.2 tonne-years. No evidence for an excess over expected backgrounds was found across all the test WIMP masses. The resulting limit on the spin-independent WIMP-nucleon cross section is world-leading for masses above 9 GeV/c2, surpassing previous best limits by about a factor of four. In this talk, I will describe the new results---including a new technique to actively tag background electronic recoils from Pb-214 beta decays, the observation of charge-suppressed two-neutrino double electron capture events from Xe-124 decays, and the bias mitigation technique called "salting"---and discuss what the future plans for the experiment are.
Jamie Rankin
From Interstellar Space to the Sun’s Embrace: Cosmic Ray Journeys through the Heliosphere
Abstract:
Over a century since their discovery, cosmic rays remain a compelling subject of inquiry in the fields of particle and space physics. These fully ionized atomic nuclei – comprised of practically all known elements of the periodic table – trace paths through the galaxy (and in some cases, from beyond) that cover vast spatial distances, and span over 14 decades in energy (~MeV to a few hundred EeV observed so far). Although origins at all scales are still not fully understood, the last decade has led to some especially critical breakthroughs in understanding, particularly related to their transport and acceleration. This talk focuses on key insights primarily gained from space-based observations of cosmic rays, ranging from ~MeV to ~TeV, whose trajectories get modified by the dynamics and presence of our own stellar astrosphere, the “heliosphere”. It will survey the key findings derived from in-situ measurements at various locations throughout the solar system – including those at record-setting distances near and far from the Sun – and venture beyond the cosmic rays themselves to emphasize what they reveal about how the Sun interacts with its surrounding interstellar environment, the size and structure of the heliosphere, and the physics of particle-plasma interactions applicable to many solar and astrophysical phenomena.
Roger Rusack
Measuring the Higgs Boson mass
Abstract: Since the Higgs boson was first observed in the early data collected at the LHC there have been a sequence of measurements of the mass by both the CMS and ATLAS collaborations that have become more and more precise as more data are collected. While the mass of the Higgs boson, is not predicted by the standard model of particle physics, once the mass is known its couplings to other elementary particles are known. Precision measurements of its mass are further motivated by its connection to the stability of the electroweak vacuum and to the self-consistency of the electroweak fit. In my talk I will discuss how the mass is measured in both the ZZ* and the gamma-gamma decay channels by the two experiments and discuss an analysis the CMS Collaboration is performing to the achieve the most precise measurement so far of the Higgs boson mass.
Kenneth Long
The precise measurement of the W boson mass with the CMS detector at the CERN LHC
Abstract: Particle masses and the coupling strengths of the forces are fundamentally experimental parameters that must be measured and input into the standard model of particle physics (SM). While the SM does not predict their values, it does predict precise relationships between them. Physics beyond the standard model can change these relationships through the effects of virtual particle quantum loops, thus making it of paramount importance to measure these parameters with the highest possible precision. While the mass of the Z boson is known to the remarkable precision of nearly 20 parts per million, thanks to the CERN LEP experimental program, the W boson mass is known much less precisely. Furthermore, the most precise measurement of the W boson mass, performed by the CDF Collaboration at Fermilab in 2022, is in significant tension with the standard model expectation from indirect measurements. Recently, the CMS Collaboration at the LHC has performed its first measurement of the W boson mass. The measurement is based on a sample of W boson events decaying to a muon and a neutrino, with the results obtained via a highly granular maximum likelihood fit to the kinematic distributions of the muons. The significant in situ constraints of theoretical inputs and their corresponding uncertainties provided by this novel approach, together with an accurate determination of the experimental effects, lead to a very precise W boson mass measurement, 80360.2 +/- 9.9 MeV. The result is in agreement with the standard model prediction and in tension with the measurement of the CDF Collaboration. I will discuss the measurement procedure and the experimental and theoretical advancements that enabled this striking result.
Zoltan Ligeti
Flavor: from the November revolution to the FCC
Abstract: Flavor physics, the study of what distinguishes the fermion generations, was instrumental in establishing the standard model of particle physics (SM). It continues to provide some of the strongest constraints on extensions of the SM, and will likely be important in elucidating the structure of new phenomena hopefully discovered at the LHC or future colliders. I will discuss some recent topics of interest due to hints of possible deviations from the SM, as well as examples of the expected increases in discovery potential in the coming decades.
Julia Gonski
A Collider for the Future of High Energy Physics
Abstract: High energy particle colliders have been a cornerstone of fundamental physics research for decades, providing increasingly stringent evidence of the Standard Model and enabling key discoveries. Outstanding goals for the field, such as precision characterization of the Higgs boson, probing the dark sector, and exploring the unknown, require a plan to ensure that the successes of collider physics don’t end with the Large Hadron Collider around 2040. The 2023 US P5 report lays the groundwork for future collider planning, prioritizing an off-shore “Higgs factory” followed by a multi-TeV discovery machine. The Future Circular Collider (FCC), proposed to be hosted at CERN with international collaboration, offers a combined program for both of these priorities. The P5 process, FCC program, and ongoing work will be discussed alongside related topics of alternate collider designs and accelerator/detector R&D, together laying out a bright and exciting future for our understanding of the fundamental universe.
Alfonso Garcia
News from the Mediterranean Abyss: Latest Findings from KM3NeT Neutrino Telescopes
Abstract: The KM3NeT collaboration is constructing two Cherenkov detectors deep in the Mediterranean Sea: ARCA, situated off the Sicilian coast, aims to detect high-energy astrophysical neutrinos, and ORCA, located 40 km off-shore Toulon, designed to study atmospheric neutrino oscillations. Despite currently operating in partial configurations, both detectors have collected over a year of data, yielding exciting initial physics results. In this seminar, I will present the latest findings from these detectors, highlighting a remarkable high-energy event observed in ARCA last year.
Dean Lee
Emergent physics from nuclear lattice simulations
Abstract: The talk starts with an introduction to nuclear lattice effective field theory. After this, several recent results are presented such as the emergent geometry and duality of the carbon nucleus, wavefunction matching for solving many-body problems, calculations of nuclear charge radii, nuclear structure for initial states of relativistic ion collisions, and nuclear thermodynamics. The last part of the talk is a discussion of new results on multimodal superfluidity, with theoretical and experimental evidence for quartet superfluidity and simultaneous spin-singlet (S-wave) and spin-triplet (P-wave) superfluidity in neutrons.
