GRASIAN: Shaping and characterization of the cold hydrogen and deuterium beams for the forthcoming first demonstration of gravitational quantum states of atoms
Carina Killian, Philipp Blumer, Paolo Crivelli, Daniel Kloppenburg, Francois Nez, Valery Nesvizhevsky, Serge Reynaud, Katharina Schreiner, Martin Simon, Sergey Vasiliev, Eberhard Widmann, Pauline Yzombard
{"title":"GRASIAN: Shaping and characterization of the cold hydrogen and deuterium beams for the forthcoming first demonstration of gravitational quantum states of atoms","authors":"Carina Killian, Philipp Blumer, Paolo Crivelli, Daniel Kloppenburg, Francois Nez, Valery Nesvizhevsky, Serge Reynaud, Katharina Schreiner, Martin Simon, Sergey Vasiliev, Eberhard Widmann, Pauline Yzombard","doi":"arxiv-2407.15443","DOIUrl":null,"url":null,"abstract":"A low energy particle confined by a horizontal reflective surface and gravity\nsettles in gravitationally bound quantum states. These gravitational quantum\nstates (GQS) were so far only observed with neutrons. However, the existence of\nGQS is predicted also for atoms. The GRASIAN collaboration pursues the first\nobservation of GQS of atoms, using a cryogenic hydrogen beam. This endeavor is\nmotivated by the higher densities, which can be expected from hydrogen compared\nto neutrons, the easier access, the fact, that GQS were never observed with\natoms and the accessibility to hypothetical short range interactions. In\naddition to enabling gravitational quantum spectroscopy, such a cryogenic\nhydrogen beam with very low vertical velocity components - a few cm s$^{-1}$,\ncan be used for precision optical and microwave spectroscopy. In this article,\nwe report on our methods developed to reduce background and to detect atoms\nwith a low horizontal velocity, which are needed for such an experiment. Our\nrecent measurement results on the collimation of the hydrogen beam to 2 mm, the\nreduction of background and improvement of signal-to-noise and finally our\nfirst detection of atoms with velocities < 72 m s$^{-1}$ are presented.\nFurthermore, we show calculations, estimating the feasibility of the planned\nexperiment and simulations which confirm that we can select vertical velocity\ncomponents in the order of cm s$^{-1}$.","PeriodicalId":501039,"journal":{"name":"arXiv - PHYS - Atomic Physics","volume":"67 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-07-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Atomic Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2407.15443","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
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 s$^{-1}$,
can be used for precision optical and microwave spectroscopy. In this article,
we report on our methods developed to reduce background and to detect atoms
with a low horizontal velocity, which are needed for such an experiment. Our
recent measurement results on the collimation of the hydrogen beam to 2 mm, the
reduction of background and improvement of signal-to-noise and finally our
first detection of atoms with velocities < 72 m s$^{-1}$ are presented.
Furthermore, we show calculations, estimating the feasibility of the planned
experiment and simulations which confirm that we can select vertical velocity
components in the order of cm s$^{-1}$.