| dc.contributor.author | Kawasaki, Akio | |
| dc.date.accessioned | 2015-10-13T12:03:01Z | |
| dc.date.available | 2015-10-13T12:03:01Z | |
| dc.date.issued | 2015-10 | |
| dc.date.submitted | 2015-07 | |
| dc.identifier.issn | 1050-2947 | |
| dc.identifier.issn | 1094-1622 | |
| dc.identifier.uri | http://hdl.handle.net/1721.1/99215 | |
| dc.description.abstract | The magic wavelength for an optical lattice for hydrogen atoms that cancels the lowest order ac Stark shift of the 1S-2S transition is calculated to be 513 nm. The magnitudes of the ac Stark shift ΔE = −119 Hz/(kW/cm[superscript 2]) and the slope dΔE/dν = −2.77 Hz/(GHz kW/cm[superscript 2]) at the magic wavelength suggest that a stable and narrow-line-width trapping laser is necessary to achieve a deep enough optical lattice to confine hydrogen atoms in a way that gives a small enough light shift for the precision spectroscopy of the 1S-2S transition. | en_US |
| dc.description.sponsorship | United States. Defense Advanced Research Projects Agency | en_US |
| dc.description.sponsorship | National Science Foundation (U.S.) | en_US |
| dc.publisher | American Physical Society | en_US |
| dc.relation.isversionof | http://dx.doi.org/10.1103/PhysRevA.92.042507 | 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 | American Physical Society | en_US |
| dc.title | Magic wavelength for the hydrogen 1S-2S transition | en_US |
| dc.type | Article | en_US |
| dc.identifier.citation | Kawasaki, Akio. "Magic wavelength for the hydrogen 1S-2S transition." Phys. Rev. A 92, 042507 (October 2015). © 2015 American Physical Society | en_US |
| dc.contributor.department | Massachusetts Institute of Technology. Department of Physics | en_US |
| dc.contributor.department | Massachusetts Institute of Technology. Research Laboratory of Electronics | en_US |
| dc.contributor.department | MIT-Harvard Center for Ultracold Atoms | en_US |
| dc.contributor.mitauthor | Kawasaki, Akio | en_US |
| dc.relation.journal | Physical Review A | 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 | 2015-10-12T22:00:13Z | |
| dc.language.rfc3066 | en | |
| dc.rights.holder | American Physical Society | |
| dspace.orderedauthors | Kawasaki, Akio | en_US |
| dc.identifier.orcid | https://orcid.org/0000-0001-8353-8903 | |
| mit.license | PUBLISHER_POLICY | en_US |
| mit.metadata.status | Complete | |
