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Jie Hu (University of Alberta)Poster
DEAP-3600 is a single-phase liquid argon (LAr) dark matter detector located 2 km underground at SNOLAB in Sudbury, Canada, searching for nuclear recoils from dark matter scattering in a 3.3-tonne LAr target. In 2019, the collaboration published a leading limit on the WIMP-nucleon spin-independent cross section, based on 231 exposure days. A new profile likelihood ratio analysis extends the...
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Dwaipayan RayPoster
Neutrinoless double-beta decay ($0\nu\beta\beta$) offers a way to probe for physics beyond the Standard Model. Observation of $0\nu\beta\beta$ will validate the Majorana nature of neutrinos, demonstrate violation of lepton number leading to an explanation of the observed baryon asymmetry in the universe, and probe new mass generation mechanisms up to the GUT scale. The planned nEXO experiment...
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Denaisha KraftPoster
While the Standard Model (SM) of particle physics has been successful in describing known fundamental particles and interactions, it is incomplete. The amount of charge-parity (CP) violation predicted within the SM is insufficient to explain the observed matter-antimatter asymmetry in the Universe. Additionally, possible deviations in the self-interactions of electroweak bosons motivate the...
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Peter Qin (SNOLAB)Poster
Rn-222 progeny produce unwanted background events in underground rare-event searches including those for dark matter and neutrinoless double beta decay. ZnS(Ag)-coated Lucas cells were used during the SNO experiment to evaluate Radon emanation into light water and continue to be used for ex-situ measurements of Radon concentration in SNO+ and at SNOLAB for materials assays. Support for current...
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Konstantin Stoychev (University of Guelph)Poster
The sudden onset of deformation in $A\approx100$ nuclei at $N=60$ has been described as a ground-state shape transition that has raised a lot of interest over the years from an experimental and theoretical point of view. This transition is most pronounced in the Zr and Sr isotopic chains where the low-energy excited-state structure shows significant signs of deformation developing at $N=60$,...
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Aeyla Webster (TRIUMF)Poster
The origin of the only stable fluorine isotope, $^{19}F$, has remained a longstanding question in nuclear astrophysics due to persistent discrepancies between observations and model-predicted abundances constrained by laboratory reaction rates and nuclear physics input. Recent work by Cristallo et al. highlighted that the reaction rate of $^{15}N(a,g)^{19}F$ – one of the key production...
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Abdennacer Hamdi (University of Regina)Poster
One of the long standing questions in the standard model of particle physics is the origin of nucleon mass, spin, and the charge and density spatial distributions within. In the theory of the strong interaction, the structure of the nucleon is described by form factors which can be accessed through hard exclusive meson production. The main focus of this study is to measure the form factor of...
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Taiki Shickele (TRIUMF/UBC)Poster
Sterile neutrinos appear in various extensions of the Standard Model and can help explain the origin of the observed active neutrino masses. Light sterile neutrinos in particular can contribute to the neutrinoless double-beta ($0\nu\beta\beta$) decay amplitude, providing an additional avenue to probe new physics, in addition to the established sensitivity of the process to the Majorana nature...
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Luan KoerichPoster
The Hyper-Kamiokande (Hyper-K) main detector is under construction and is planned to begin operation in 2027. The detector will consist of a cylindrical water tank measuring 68 metres in diameter and 72 metres in height, instrumented with 20,000 inward-facing 50-cm photomultiplier tubes (PMTs). To enhance calibration capabilities, 800 of the conventional PMTs will be replaced by multi-PMT...
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Artemis Tsantiri (University of Regina)Poster
Type I X-ray bursts are among the most frequent thermonuclear explosions we can observe, and can reveal important properties of accreting neutron star systems. Understanding their light curves requires detailed knowledge of the nuclear reactions that enable the transition from the hot CNO cycle towards explosive burning and the rp process. One such key breakout reaction is the 14O(α,p)17F...
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Desislava Kalaydjieva (University of Guelph)Poster
A sudden ground-state shape transition is known to occur sharply at $N=60$, accompanied by equally dramatic changes in the low-energy spectra of the nuclei with A$\approx\!$100. Detailed spectroscopic data on the $\gamma$ decay of $^{100}$Zr are essential for understanding this phase transition and the emergence of shape coexistence, predicted by recent Monte Carlo Shell Model (MCSM)...
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Diba Toyserkani (SNOLAB)Poster
The RadioActive isotope Measurement Program at SNOLAB (RAMPS) is designed to perform first direct measurement of long-lived nuclear decay processes. The pilot project focuses on performing the first direct measurement of the excited-state electron capture decay of Lutetium-176, a theoretically predicted yet experimentally unobserved nuclear transition. Understanding this highly suppressed...
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Emile Cantacuzene (University of Regina)Poster
As nuclei get richer in neutrons, the Q-value for beta-decay gets larger while the neutron separation energy decreases. Consequently, for large enough N/Z ratios, the daughter nucleus can decay by emitting one to several neutrons. Directly studying states above the neutron separation energy is an experimental challenge as it requires neutron detectors that have a good energy resolution while...
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