Getting there! DUNE with two 17kt LAr TPC Far Detector (FD1-FD2) modules, a Near Detector Complex and a Neutrino Beam with an intensity of 1.2 MW is well on its way to start physics in 2028 at SURF (SD). Mass Ordering and sensitivity to Maximal CPV - the initial goals of the flagship Long-Baseline (LBL) Neutrino Program - are within reach. The time has come to define a strategy to achieve the ambitious ultimate precision in the LBL physics goals and possibly further expand the DUNE science scope into the low-energy domain of rare underground physics and BSM searches.
Spouses And Partners
At sufficiently high temperatures and pressures, QCD matter becomes a hot and dense deconfined medium known as the Quark Gluon Plasma (QGP). Collisions of relativistic heavy-ions are used to recreate the QGP, providing a rich laboratory for exploring the mysteries of the strong interaction. The intrinsic and dynamic properties of the QGP are probed with jets, narrow cones of particles resulting from the scattering of quarks and gluons with a high momentum transfer.
In heavy-ion collisions, the fragmentation pattern of a high-energy jet is modified by its interactions with the quark-gluon plasma (QGP). Jet substructure observables, i.e. observables build out of the jet constituents, are thus expected to be sensitive to properties of the medium such as its temperature, length or transport coefficients. So far, experimental measurements at RHIC and the LHC have revealed a narrowing of the jet core with respect to proton-proton collisions.
Neutrinos decoupled in the early moments of the Big Bang are believed to be the second most abundant particle in the Universe. PTOLEMY is an experiment for detecting relic neutrinos captured on tritium targets. The challenges of ultra-cold neutrino detection have led to new advances in material technologies, RF detection, TES micro-calorimetry, and a transverse drift electromagnetic spectrometer. In this talk, I will present the current status and prospects of PTOLEMY.
High energy (> TeV) neutrinos are unique messengers to the distant, high-energy universe. As chargeless and weakly interacting particles, neutrinos arrive undeflected and unattenuated from cosmic distances, giving us key insights to the properties of astrophysical accelerators at the highest redshifts. In this talk, I will discuss the ongoing work of the IceCube Neutrino Observatory to detect and study extraterrestrial neutrinos across a broad range in energies, from TeV to EeV.
The gluon distribution function grows with lower and lower momentum fraction x very fast. As the total scattering cross section is bound by quantum mechanics, the raise of the gluon density has to be tamed, which is explained by gluon recombination under the color glass condensate (CGC) framework. A definitive discovery of nonlinear effects in QCD and as such the saturation regime would significantly improve our understanding of the nucleon structure and of nuclear interactions at high energy.
The neutrino mass scale plays a crucial role in both particle physics and cosmology, yet this scale is unknown. The neutrino masses distort the tritium beta-decay spectrum due to energy conservation. By measuring the tritium spectrum, KATRIN has placed the most precise model-independent limit on the neutrino mass scale, to date (mβ<0.8 eV). Cyclotron Radiation Emission Spectroscopy (CRES), a technique pioneered by Project 8, has the potential to advance beyond KATRIN’s design sensitivity.
sPHENIX is a new Relativistic Heavy Ion Collider (RHIC) detector under construction at Brookhaven National Laboratory required to complete RHIC’s scientific mission of probing the inner workings of Quark-Gluon Plasma. For that reason, sPHENIX will make precision measurements of jets, heavy flavor, and upsilon production. These measurements are possible due to the large hermetic acceptance, huge data rate, hadronic calorimetry, precision tracking of the sPHENIX detector.
This talk will discuss sPHENIX readiness for operations, its physics program, and construction status.
Understanding what our material world is made of has been an ultimate question for humankind for as long as our existence. Yet modern science and technology have enabled us to “see” objects at vastly different scales, from stars in distant galaxies to atomic particles, the fundamental origin of these matter and their strong interactions are far from understood. One of the most intriguing questions, the color confinement, is of particular interest, where quarks and gluons are forever clumped in the form of hadrons.
The Standard Model of particle physics describes fundamental forces in the universe – electromagnetic, weak and strong interactions. The strong interactions between quarks and gluons via color charges is described by Quantum Chromodynamics (QCD). High-energy particle accelerators enable precision studies of the Standard Model and beyond and, in particular, answering fundamental open questions in QCD, concerning the processes underlying complex particle formation and the nature of emergent QCD. Hadrons are composite color neutral states that comprise much of the visible world around us.