Nanoparticle Interferometer by Throw and Catch

Matter wave interferometry with increasingly larger masses could pave the way to understanding the nature of wavefunction collapse, the quantum to classical transition, or even how an object in a spatial superposition interacts with its gravitational field. In order to improve upon the current mass...

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Detalles Bibliográficos
Autores: Wardak, Jakub|||0000-0003-2348-1989, Georgescu, Tiberius, Gasbarri, Giulio|||0000-0001-9135-1719, Belenchia, Alessio|||0000-0002-0347-6763, Ulbricht, Hendrik
Tipo de recurso: artículo
Fecha de publicación:2024
País:España
Institución:Universitat Autònoma de Barcelona
Repositorio:Dipòsit Digital de Documents de la UAB
Idioma:inglés
OAI Identifier:oai:ddd.uab.cat:290850
Acceso en línea:https://ddd.uab.cat/record/290850
https://dx.doi.org/urn:doi:10.3390/atoms12020007
Access Level:acceso abierto
Palabra clave:Matter wave interferometry
Levitated optomechanics
Quantum superposition
Descripción
Sumario:Matter wave interferometry with increasingly larger masses could pave the way to understanding the nature of wavefunction collapse, the quantum to classical transition, or even how an object in a spatial superposition interacts with its gravitational field. In order to improve upon the current mass record, it is necessary to move into the nanoparticle regime. In this paper, we provide a design for a nanoparticle Talbot-Lau matter wave interferometer that circumvents the practical challenges of previously proposed designs. We present numerical estimates of the expected fringe patterns that such an interferometer would produce, considering all major sources of decoherence. We discuss the practical challenges involved in building such an experiment, as well as some preliminary experimental results to illustrate the proposed measurement scheme. We show that such a design is suitable for seeing interference fringes with (Formula presented.) amu SiO particles and that this design can be extended to even (Formula presented.) amu particles by using flight times below the typical Talbot time of the system.