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DC Field | Value | Language |
---|---|---|
dc.contributor.author | F. Niyaz | en_US |
dc.contributor.author | J. Nunkaew | en_US |
dc.contributor.author | T. F. Gallagher | en_US |
dc.date.accessioned | 2019-08-05T04:43:17Z | - |
dc.date.available | 2019-08-05T04:43:17Z | - |
dc.date.issued | 2019-04-15 | en_US |
dc.identifier.issn | 24699934 | en_US |
dc.identifier.issn | 24699926 | en_US |
dc.identifier.other | 2-s2.0-85064815436 | en_US |
dc.identifier.other | 10.1103/PhysRevA.99.042507 | en_US |
dc.identifier.uri | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85064815436&origin=inward | en_US |
dc.identifier.uri | http://cmuir.cmu.ac.th/jspui/handle/6653943832/65873 | - |
dc.description.abstract | © 2019 American Physical Society. Using a microwave and radio frequency resonance approach we observe the transitions of ytterbium from the 6s(n+3)d states to the 6snℓ states for 4≤ℓ≤6 and 28≤n≤33. The energies of the 6snℓ states of ℓ≥4 are determined from the observed intervals and the known values of the 6snd energies. We use a nonadiabatic core polarization model to analyze the energy levels to determine the dipole (αd) and quadrupole (αq) polarizabilities of the ground state of Yb+. We find the values αd=60.51(10)a03 and αq=672(28)a05. | en_US |
dc.subject | Physics and Astronomy | en_US |
dc.title | Microwave spectroscopy of the Yb 6s(n+3)d→6sng, 6snh, and 6sni transitions | en_US |
dc.type | Journal | en_US |
article.title.sourcetitle | Physical Review A | en_US |
article.volume | 99 | en_US |
article.stream.affiliations | University of Virginia | en_US |
article.stream.affiliations | Chiang Mai University | en_US |
Appears in Collections: | CMUL: Journal Articles |
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