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dc.contributor.authorCassettari, Donatella
dc.contributor.authorMussardo, Giuseppe
dc.contributor.authorTrombettoni, Andrea
dc.date.accessioned2023-01-31T13:30:28Z
dc.date.available2023-01-31T13:30:28Z
dc.date.issued2023-01-31
dc.identifier282631517
dc.identifierc9abc92b-1162-4b55-999a-e4caf4303c0c
dc.identifier85178170905
dc.identifier.citationCassettari , D , Mussardo , G & Trombettoni , A 2023 , ' Holographic realization of the prime number quantum potential ' , PNAS Nexus , vol. 2 , no. 1 , pgac279 . https://doi.org/10.1093/pnasnexus/pgac279en
dc.identifier.issn2752-6542
dc.identifier.otherBibtex: 10.1093/pnasnexus/pgac279
dc.identifier.otherORCID: /0000-0003-3571-6642/work/128097280
dc.identifier.urihttps://hdl.handle.net/10023/26863
dc.description.abstractWe report the experimental realization of the prime number quantum potential VN(x), defined as the potential entering the single-particle Schrödinger Hamiltonian with eigenvalues given by the first N prime numbers. Using computer-generated holography, we create light intensity profiles suitable to optically trap ultracold atoms in these potentials for different N values. As a further application, we also implement a potential whose spectrum is given by the lucky numbers, a sequence of integers generated by a different sieve than the familiar Eratosthenes’s sieve used for the primes. Our results pave the way towards the realization of quantum potentials with arbitrary sequences of integers as energy levels and show, in perspective, the possibility to set up quantum systems for arithmetic manipulations or mathematical tests involving prime numbers.
dc.format.extent8
dc.format.extent2357622
dc.language.isoeng
dc.relation.ispartofPNAS Nexusen
dc.subjectQuantum devicesen
dc.subjectSchrödinger Hamiltonianen
dc.subjectOptical trapsen
dc.subjectPrime numbersen
dc.subjectQC Physicsen
dc.subjectQB Astronomyen
dc.subjectDASen
dc.subjectMCCen
dc.subject.lccQCen
dc.subject.lccQBen
dc.titleHolographic realization of the prime number quantum potentialen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. Condensed Matter Physicsen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1093/pnasnexus/pgac279
dc.description.statusPeer revieweden


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