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dc.contributor.author | van Wyk, Pieter | en |
dc.contributor.author | Tajima, Hiroyuki | en |
dc.contributor.author | Inotani, Daisuke | en |
dc.contributor.author | Ohnishi, Akira | en |
dc.contributor.author | Ohashi, Yoji | en |
dc.contributor.alternative | 大西, 明 | ja |
dc.date.accessioned | 2018-08-06T04:51:07Z | - |
dc.date.available | 2018-08-06T04:51:07Z | - |
dc.date.issued | 2018-01 | - |
dc.identifier.issn | 2469-9926 | - |
dc.identifier.uri | http://hdl.handle.net/2433/233198 | - |
dc.description.abstract | We propose a theoretical idea to use an ultracold Fermi gas as a quantum simulator for the study of the low-density region of a neutron-star interior. Our idea is different from the standard quantum simulator that heads for perfect replication of another system, such as the Hubbard model discussed in high-Tc cuprates. Instead, we use the similarity between two systems and theoretically make up for the difference between them. That is, (1) we first show that the strong-coupling theory developed by Nozières and Schmitt–Rink (NSR) can quantitatively explain the recent experiment on the equation of state (EoS) in a ⁶Li superfluid Fermi gas in the BCS (Bardeen–Cooper–Schrieffer) unitary limit far below the superfluid phase-transition temperature Tc. This region is considered to be very similar to the low-density region (crust regime) of a neutron star (where a nearly unitary s-wave neutron superfluid is expected). (2) We then theoretically compensate the difference that, while the effective range reff is negligibly small in a superfluid ⁶Li Fermi gas, it cannot be ignored (reff = 207 fm) in a neutron star, by extending the NSR theory to include effects of reff. The calculated EoS when reff = 2.7 fm is shown to agree well with the previous neutron-star EoS in the low-density region predicted in nuclear physics. Our idea indicates that an ultracold atomic gas may more flexibly be used as a quantum simulator for the study of other complicated quantum many-body systems, when we use not only the experimental high tunability, but also the recent theoretical development in this field. Since it is difficult to directly observe a neutron-star interior, our idea would provide a useful approach to the exploration for this mysterious astronomical object. | en |
dc.format.mimetype | application/pdf | - |
dc.language.iso | eng | - |
dc.publisher | American Physical Society (APS) | en |
dc.rights | ©2018 American Physical Society. | en |
dc.title | Superfluid Fermi atomic gas as a quantum simulator for the study of the neutron-star equation of state in the low-density region | en |
dc.type | journal article | - |
dc.type.niitype | Journal Article | - |
dc.identifier.jtitle | Physical Review A | en |
dc.identifier.volume | 97 | - |
dc.identifier.issue | 1 | - |
dc.relation.doi | 10.1103/PhysRevA.97.013601 | - |
dc.textversion | publisher | - |
dc.identifier.artnum | 013601 | - |
dc.address | Department of Physics, Keio University | en |
dc.address | Nishina Center, RIKEN | en |
dc.address | Department of Physics, Keio University | en |
dc.address | Yukawa Institute for Theoretical Physics, Kyoto University | en |
dc.address | Department of Physics, Keio University | en |
dcterms.accessRights | open access | - |
datacite.awardNumber | 16K05503 | - |
datacite.awardNumber | 15K00178 | - |
datacite.awardNumber | 15H00840 | - |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName.alternative | Japan Society for the Promotion of Science (JSPS) | en |
jpcoar.funderName.alternative | Japan Society for the Promotion of Science (JSPS) | en |
jpcoar.funderName.alternative | Japan Society for the Promotion of Science (JSPS) | en |
出現コレクション: | 学術雑誌掲載論文等 |
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