| dc.contributor.author | Jiang, Qing-Dong | |
| dc.contributor.author | Wilcek, Frank | |
| dc.date.accessioned | 2022-04-14T15:49:33Z | |
| dc.date.available | 2021-09-20T18:21:26Z | |
| dc.date.available | 2022-04-14T15:49:33Z | |
| dc.date.issued | 2019 | |
| dc.identifier.uri | https://hdl.handle.net/1721.1/132236.2 | |
| dc.description.abstract | © 2019 American Physical Society. Quantum fluctuations in vacuum can exert a dissipative force on moving objects, which is known as Casimir friction. Especially, a rotating particle in the vacuum will eventually slow down due to the dissipative Casimir friction. Here, we identify a dissipationless force by examining a rotating particle near a bi-isotropic media that generally breaks parity symmetry or/and time-reversal symmetry. The direction of the dissipationless vacuum force is always parallel with the rotating axis of the particle. We therefore call this dissipationless vacuum force the axial Casimir force. | en_US |
| dc.language.iso | en | |
| dc.publisher | American Physical Society (APS) | en_US |
| dc.relation.isversionof | 10.1103/PHYSREVB.99.165402 | en_US |
| dc.rights | Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. | en_US |
| dc.source | APS | en_US |
| dc.title | 5/11 - [DUPE] Axial Casimir force | en_US |
| dc.type | Article | en_US |
| dc.contributor.department | Massachusetts Institute of Technology. Center for Theoretical Physics | en_US |
| dc.eprint.version | Final published version | en_US |
| dc.type.uri | http://purl.org/eprint/type/JournalArticle | en_US |
| eprint.status | http://purl.org/eprint/status/PeerReviewed | en_US |
| dc.date.updated | 2020-03-02T12:48:01Z | |
| dspace.date.submission | 2020-03-02T12:48:04Z | |
| mit.license | PUBLISHER_POLICY | |
| mit.metadata.status | Publication Information Needed | en_US |
