Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/248
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dc.contributor.authorArora, Bindiya-
dc.date.accessioned2013-05-14T08:34:10Z-
dc.date.available2013-05-14T08:34:10Z-
dc.date.issued2012-
dc.identifier.citationPhys. Rev. A 85, 012506en_US
dc.identifier.urihttp://pra.aps.org/pdf/PRA/v85/i1/e012506en_US
dc.identifier.urihttp://arxiv.org/abs/1108.1639en_US
dc.descriptionOnly IISERM authors are available in the record.-
dc.description.abstractAppraising the projected $10^{-18}$ fractional uncertainty in the optical frequency standards using singly ionized ions, we estimate the black-body radiation (BBR) shifts due to the magnetic dipole (M1) and electric quadrupole (E2) multipoles of the magnetic and electric fields, respectively. Mul- tipolar scalar polarizabilities are determined for the singly ionized calcium (Ca$^+$) and strontium  (Sr$^+$) ions using the relativistic coupled-cluster method; though the theory can be exercised for any single ion clock proposal. The expected energy shifts for the respective clock transitions are estimated to be $4.38(3) \times 10^{-4}$ Hz for Ca$^+$ and $9.50(7) \times 10^{-5}$ Hz for Sr$^+$. These shifts are large enough and may be prerequisite for the frequency standards to achieve the foreseen  $10^{-18}$ precision goal.en_US
dc.language.isoenen_US
dc.publisherThe American Physical Societyen_US
dc.titleMultipolar Black Body Radiation Shifts for the Single Ion BASED Optical frequency standards,Clocksen_US
dc.typeArticleen_US
Appears in Collections:Research Articles

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