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dc.contributor.authorF. Niyazen_US
dc.contributor.authorJ. Nunkaewen_US
dc.contributor.authorT. F. Gallagheren_US
dc.date.accessioned2019-08-05T04:43:17Z-
dc.date.available2019-08-05T04:43:17Z-
dc.date.issued2019-04-15en_US
dc.identifier.issn24699934en_US
dc.identifier.issn24699926en_US
dc.identifier.other2-s2.0-85064815436en_US
dc.identifier.other10.1103/PhysRevA.99.042507en_US
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85064815436&origin=inwarden_US
dc.identifier.urihttp://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.subjectPhysics and Astronomyen_US
dc.titleMicrowave spectroscopy of the Yb 6s(n+3)d→6sng, 6snh, and 6sni transitionsen_US
dc.typeJournalen_US
article.title.sourcetitlePhysical Review Aen_US
article.volume99en_US
article.stream.affiliationsUniversity of Virginiaen_US
article.stream.affiliationsChiang Mai Universityen_US
Appears in Collections:CMUL: Journal Articles

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