Long-Baseline Atom Interferometry
Abstrak
Long-baseline atom interferometry is a promising technique for probing various aspects of fundamental physics, astrophysics and cosmology, including searches for ultralight dark matter (ULDM) and for gravitational waves (GWs) in the frequency range around 1~Hz that is not covered by present and planned detectors using laser interferometry. The MAGIS detector is under construction at Fermilab, as is the MIGA detector in France. The PX46 access shaft to the LHC has been identified as a very suitable site for an atom interferometer of height $\sim 100$m, sites at the Boulby mine in the UK and the Canfranc Laboratory are also under investigation, and possible sites for km-class detectors have been suggested. The Terrestrial Very-Long-Baseline Atom Interferometry (TVLBAI) Proto-Collaboration proposes a coordinated programme of interferometers of increasing baselines.
Topik & Kata Kunci
Penulis (53)
Antun Balaz
Diego Blas
Oliver Buchmueller
Sergio Calatroni
Laurentiu-Ioan Caramete
David Cerdeno
Maria Luisa Chiofalo
Fabio Di Pumpo
Goran Djordjevic
John Ellis
Pierre Fayet
Chris Foot
Naceur Gaaloul
Susan Gardner
Barry M Garraway
Alexandre Gauguet
Enno Giese
Jason M. Hogan
Onur Hosten
Alex Kehagias
Eva Kilian
Tim Kovachy
Carlos Lacasta
Marek Lewicki
Elias Lopez Asamar
J. Luis Lopez-Gonzalez
Nathan Lundblad
Michele Maggiore
Christopher McCabe
John McFerran
Gaetano Mileti
Peter Millington
Gavin W. Morley
Senad Odzak
Chris Overstreet
Krzysztof Pawlowski
Emanuele Pelucchi
Johann Rafelski
Albert Roura
Marianna S. Safronova
Florian Schreck
Olga Sergijenko
Yeshpal Singh
Marcelle Soares-Santos
Nikolaos Stergioulas
Guglielmo M. Tino
J. N. Tinsley
Hendrik Ulbricht
Maurits van der Grinten
Ville Vaskonen
Wolf von Klitzing
Andre Xuereb
Emmanuel Zambrini Cruzeiro
Akses Cepat
- Tahun Terbit
- 2025
- Bahasa
- en
- Sumber Database
- arXiv
- Akses
- Open Access ✓