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Detecting Superfluids, Exciting the Higgs Mode and Enhanced Cooling of Dimers in the BEC-BCS Crossover

dc.contributor.advisorKöhl, Michael
dc.contributor.authorEberz, Daniel
dc.date.accessioned2025-06-04T10:26:25Z
dc.date.available2025-06-04T10:26:25Z
dc.date.issued04.06.2025
dc.identifier.urihttps://hdl.handle.net/20.500.11811/13119
dc.description.abstractIn this thesis, the BEC-BCS crossover is experimentally investigated using a quantum simulator apparatus. We prepare a degenerate, interacting fermionic sample by cooling atoms in two of the lowest hyperfine states of 6Li in a crossed optical dipole trap. Interactions between the two states are controlled by means of a broad magnetic Feshbach resonance, and we adjust the samples' temperature and density by preciely tuning the trapping potential. This setup allows us to access and probe the entire BEC-BCS crossover.
A key property of the BEC-BCS crossover is the superfluid critical temperature, predicted to have a maximum on the BEC side of the strongly interacting regime. However, accurately measuring the critical temperature is challenging due to difficulties in determining a reliable temperature scale in the presence of strong interactions. In this thesis, we determine the critical temperature in the crossover with high accuracy by reconstructing the density distribution and incorporating interaction effects in the low-density wings when fitting to the virial expansion of the equation of state. This requires precise identification of the superfluid phase transition onset, for which we have developed two novel advanced image recognition techniques based on machine learning. Our improved methodology confirms, for the first time, an increase in the critical temperature from the BCS limit, extending beyond the unitarity point and approaching the BEC limit.
Crossing the superfluid phase transition is accompanied by spontaneous symmetry breaking, creating an energy landscape that supports two distinct excitation modes: the Goldstone and Higgs modes. Here, we probe the Higgs mode using two distinct excitation methods: a quench and a modulation of the interaction strength. This enables us to observe the Higgs mode throughout the crossover, revealing a gradual fading of the mode as it approaches the BEC regime, where particle-hole symmetry vanishes. Notably, we observe no temperature dependence of the Higgs mode, prompting further research.
Finally, we present a novel cooling method for a strongly interacting Fermi gas on the BEC side of the crossover, where a composite dimer bound state exists. By applying a modulation of the magnetic field at frequencies close to, but higher than the bound state energy, we selectively dissociate and remove high-energy dimers from the trap, thus realising evaporative cooling of the sample. This method does not require any changes to the trapping potential and facilitates staying in the efficient runaway regime. We demonstrate cooling for a wide range of interactions on the BEC side of the crossover, achieving high efficiencies that match or exceed all previously reported forced evaporation cooling near Feshbach resonances.
en
dc.language.isoeng
dc.rightsNamensnennung 4.0 International
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subjectQuantengas
dc.subjectSuprafluidität
dc.subjectPhasendiagramm
dc.subjectBEC-BCS crossover
dc.subjectEvaporation
dc.subjectKühlung
dc.subjectMaschinelles Lernen
dc.subjectDissoziation
dc.subjectQuantum gas
dc.subjectsuperfluidity
dc.subjectphase diagram
dc.subjectevaporation
dc.subjectcooling
dc.subjectmachine learning
dc.subjectdissociation
dc.subject.ddc530 Physik
dc.titleDetecting Superfluids, Exciting the Higgs Mode and Enhanced Cooling of Dimers in the BEC-BCS Crossover
dc.typeDissertation oder Habilitation
dc.identifier.doihttps://doi.org/10.48565/bonndoc-566
dc.publisher.nameUniversitäts- und Landesbibliothek Bonn
dc.publisher.locationBonn
dc.rights.accessRightsopenAccess
dc.identifier.urnhttps://nbn-resolving.org/urn:nbn:de:hbz:5-82594
dc.relation.doihttps://doi.org/10.1103/PhysRevLett.130.203401
dc.relation.doihttps://doi.org/10.1103/PhysRevA.108.063303
dc.relation.doihttps://doi.org/10.1103/PhysRevLett.133.150403
dc.relation.doihttps://doi.org/10.48550/arXiv.2410.10642
ulbbn.pubtypeErstveröffentlichung
ulbbnediss.affiliation.nameRheinische Friedrich-Wilhelms-Universität Bonn
ulbbnediss.affiliation.locationBonn
ulbbnediss.thesis.levelDissertation
ulbbnediss.dissID8259
ulbbnediss.date.accepted10.04.2025
ulbbnediss.instituteMathematisch-Naturwissenschaftliche Fakultät : Fachgruppe Physik/Astronomie / Physikalisches Institut (PI)
ulbbnediss.fakultaetMathematisch-Naturwissenschaftliche Fakultät
dc.contributor.coRefereeHofferberth, Sebastian
ulbbnediss.contributor.orcidhttps://orcid.org/0009-0001-7977-9795


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