GRASIAN: shaping and characterization of the cold hydrogen and deuterium beams for the forthcoming first demonstration of gravitational quantum states of atoms.


Journal

The European physical journal. D, Atomic, molecular, and optical physics
ISSN: 1434-6079
Titre abrégé: Eur Phys J D At Mol Opt Phys
Pays: Germany
ID NLM: 101762148

Informations de publication

Date de publication:
2024
Historique:
received: 22 07 2024
accepted: 16 09 2024
medline: 1 11 2024
pubmed: 1 11 2024
entrez: 1 11 2024
Statut: ppublish

Résumé

A low energy particle confined by a horizontal reflective surface and gravity settles in gravitationally bound quantum states. These gravitational quantum states (GQS) were so far only observed with neutrons. However, the existence of GQS is predicted also for atoms. The GRASIAN collaboration pursues the first observation of GQS of atoms, using a cryogenic hydrogen beam. This endeavor is motivated by the higher densities, which can be expected from hydrogen compared to neutrons, the easier access, the fact that GQS were never observed with atoms and the accessibility to hypothetical short-range interactions. In addition to enabling gravitational quantum spectroscopy, such a cryogenic hydrogen beam with very low vertical velocity components-a few cm

Identifiants

pubmed: 39483954
doi: 10.1140/epjd/s10053-024-00916-5
pii: 916
pmc: PMC11522151
doi:

Types de publication

Journal Article

Langues

eng

Pagination

132

Informations de copyright

© The Author(s) 2024.

Auteurs

Carina Killian (C)

Stefan Meyer Institute for Subatomic Physics, Austrian Academy of Sciences, Dominikanerbastei 16, 1010 Vienna, Austria.

Philipp Blumer (P)

Institute for Particle Physics and Astrophysics, ETH, 8093 Zurich, Switzerland.

Paolo Crivelli (P)

Institute for Particle Physics and Astrophysics, ETH, 8093 Zurich, Switzerland.

Otto Hanski (O)

Department of Physics and Astronomy, University of Turku, 20014 Turku, Finland.

Daniel Kloppenburg (D)

Stefan Meyer Institute for Subatomic Physics, Austrian Academy of Sciences, Dominikanerbastei 16, 1010 Vienna, Austria.

François Nez (F)

Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-PSL Université, Collège de France, 75252 Paris, France.

Valery Nesvizhevsky (V)

Institut Max von Laue - Paul Langevin, 71 avenue des Martyrs, 38042 Grenoble, France.

Serge Reynaud (S)

Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-PSL Université, Collège de France, 75252 Paris, France.

Katharina Schreiner (K)

Institute for Particle Physics and Astrophysics, ETH, 8093 Zurich, Switzerland.
Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-PSL Université, Collège de France, 75252 Paris, France.
Institut Max von Laue - Paul Langevin, 71 avenue des Martyrs, 38042 Grenoble, France.
University of Vienna, Vienna Doctoral School in Physics, Universitätsring 1, 1010 Vienna, Austria.

Martin Simon (M)

Stefan Meyer Institute for Subatomic Physics, Austrian Academy of Sciences, Dominikanerbastei 16, 1010 Vienna, Austria.

Sergey Vasiliev (S)

Department of Physics and Astronomy, University of Turku, 20014 Turku, Finland.

Eberhard Widmann (E)

Stefan Meyer Institute for Subatomic Physics, Austrian Academy of Sciences, Dominikanerbastei 16, 1010 Vienna, Austria.

Pauline Yzombard (P)

Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-PSL Université, Collège de France, 75252 Paris, France.

Classifications MeSH