We invite members of our community, in particular new members, to an overview presentation about Wright Lab resources. The program includes introductions of Wright Lab technical and administrative staff, an overview of program activities for the Fall, a safety briefing for the community, and brief presentations about the facility’s resources.
Wright Lab will host two, identical 1-hour Environmental Health and Safety (EHS) Shop Orientations on Thursday, September 7 at 1 p.m. and Tuesday, September 12 at 2:30 p.m. The EHS shop orientation is offered each semester and is required to be taken once by anyone who would like to gain access and make use of the research and teaching shops at Wright Lab.
For more information on the shop facilities at Wright Lab see:
https://wlab.yale.edu/facilities
Wright Lab will host two, identical 1-hour Environmental Health and Safety (EHS) Shop Orientations on Thursday, September 7 at 1 p.m. and Tuesday, September 12 at 2:30 p.m. The EHS shop orientation is offered each semester and is required to be taken once by anyone who would like to gain access and make use of the research and teaching shops at Wright Lab.
For more information on the shop facilities at Wright Lab see:
https://wlab.yale.edu/facilities
Nuclear, particle and astrophysics are the themes of experiments hosted in underground labs. I will discuss, after motivated by fundamental questions, recent work done in Canfranc. Most of my talk will be concentrated on the exploration of neutrinos’ fundamental properties in nuclear and particle physics, astrophysics and cosmology, but I will also discuss current work on dark matter searches. Our cells are ionized by cosmic muons and radioactivity and I will briefly close with research on life processes in cosmic silence.
Inviting all members of the Wright Lab community to join us for an Ice Cream Social on Monday, August 28th at 2:00p.m. in the Wright Lab Vault.
Please join us to hear what our student researchers have been doing this summer.
AGENDA:
Forrest Hutchison (Charlie Baltay),”Magnitude Calibration of Supernovae from the LSQ/LCO Collaboration”
Florence Polak (David Rabinowitz),”Coadding QUEST Data in Search of Treasure in the Sky”
Selma Mazioud (Helen Caines),”Statistical Hadronization Model Calculations of Charm Hadron Production in Relativistic Heavy Ion Collisions at the LHC”
Joshua Kerner & Mary Zhang Remote (Helen Caines),”ePIC LFHCal R&D”
Astrophysical observation indicates that 68% of the Universe is made up of dark energy, 27% is dark matter, and the rest 5% is ordinary matter. Therefore, probing the dark components of the Universe is the most prominent subject in modern particle physics. One of the strong candidates of dark matter is the hypothetical particle called axions. The axion has been postulated to solve the strong-CP problem in quantum chromodynamics. The axion is also an ideal dark matter candidate who would have been produced during the Big Bang.
The axion represents both the most natural solution to the Strong-CP problem and a compelling candidate to constitute the dark matter of the Universe. The most sensitive experiments searching for axion dark matter are based on the resonant conversion of axions to photons within a microwave cavity permeated by a magnetic field.
Dark matter is the name that we give to the 85% of matter in the universe that interacts via gravity but negligibly with any of the other known forces. One compelling model for dark matter is the axion, as it simultaneously solves the existence of dark matter and the strong CP problem in QCD. Axions can interact with a strong magnetic field through the Primakoff effect, wherein the axion can spontaneously convert into a photon in the presence of a strong magnetic field.
BENEATH THE GREEN, THE QUANTUM
IN PARTNERSHIP WITH YALE QUANTUM INSTITUTE
