Wright Lab All Hands Meeting, Karsten Heeger, Yale, "CUPID Update"
The Wright Lab community is invited to a weekly meeting on Mondays at 9:30 a.m. in WL-216 to hear about and discuss what is going on at the lab.
The Wright Lab community is invited to a weekly meeting on Mondays at 9:30 a.m. in WL-216 to hear about and discuss what is going on at the lab.
The Wright Lab community is invited to a weekly meeting on Mondays at 9:30 a.m. in WL-216 to hear about and discuss what is going on at the lab.
The Wright Lab community is invited to a weekly meeting on Mondays at 9:30 a.m. in WL-216 to hear about and discuss what is going on at the lab.
The Wright Lab community is invited to a weekly meeting on Mondays at 9:30 a.m. in WL-216 to hear about and discuss what is going on at the lab.
The Wright Lab community is invited to a weekly meeting on Mondays at 9:30 a.m. in WL-216 to hear about and discuss what is going on at the lab.
The Wright Lab community is invited to a weekly meeting on Mondays at 9:30 a.m. in WL-216 to hear about and discuss what is going on at the lab.
The Wright Lab community is invited to a weekly meeting on Mondays at 9:30 a.m. in WL-216 to hear about and discuss what is going on at the lab.
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.
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.
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.