Welcome to the MAGIS100 web
What is MAGIS-100?
MAGIS-100 is a next-generation quantum sensor under construction at Fermilab that aims to explore fundamental physics with atom interferometry over a 100-meter baseline. This novel detector will search for ultralight dark matter, test quantum mechanics in new regimes, and serve as a technology pathfinder for future gravitational wave detectors in a previously unexplored frequency band. It combines techniques demonstrated in state-of-the-art 10-meter-scale atom interferometers with the latest technological advances of the world's best atomic clocks. MAGIS-100 will provide a development platform for a future kilometer-scale detector that would be sufficiently sensitive to detect gravitational waves from known sources. Here we present the science case for the MAGIS concept, review the operating principles of the detector, describe the instrument design, and study the detector systematics.
For more information, see
https://arxiv.org/abs/2104.02835
To access
MAGISLiverpoolWork and its subtopics you need to have a hep log in and be a member of
Magis100Group.
A start guide on how to use Foswiki
https://hep.ph.liv.ac.uk/twiki/System/WelcomeGuest
Latest News
New MAGIS-100 paper
https://arxiv.org/abs/2104.02835
Group Members
Jonathon Coleman (Academic Lead)
Kieran Bridges (Engineer)
Gedminas Elertas (Postdoc)
Sam Hindley (Research Student)
Leonie Hawkins (Research Student)
Henry Throssell (Research Student)
Kamran Hussain (Research Student)
Presentations and Papers
IntrestingPapers and
IntrestingPresentations;
Liverpool Work on MAGIS-100
MAGISLiverpoolWork
Vacuum Components
VacuumComponents
Optic Components
OpticComponents
Retro-reflection System - PZT controllers, actuators and feedback loop
RetroSystem
Procurement
QuotationOrders
Analysis
MathematicaCode
Source code for atomic source simulations:
https://github.com/TeamAtomECS/AtomECS
MAGIS100 Web Utilities