dorsal/arxiv
View SchemaPrecision spectroscopy and density-dependent frequency shifts in ultracold Sr
| Authors | Tetsuya Ido, Thomas H. Loftus, Martin M. Boyd, Andrew D. Ludlow, Kevin W. Holman, Jun Ye |
|---|---|
| Categories | |
| ArXiv ID | physics/0410110 |
| URL | https://arxiv.org/abs/physics/0410110 |
| DOI | 10.1103/PhysRevLett.94.153001 |
| Journal | Phys. Rev. Lett. 94, 153001 (2005) |
Abstract
By varying the density of an ultracold $^{88}$Sr sample from $10^9$ cm$^{-3}$ to $> 10^{12}$ cm$^{-3}$, we make the first definitive measurement of the density-related frequency shift and linewidth broadening of the $^1S_0$ - $^3P_1$ optical clock transition in an alkaline earth system. In addition, we report the most accurate measurement to date of the $^{88}$Sr $^1S_0 - ^3P_1$ optical clock transition frequency. Including a detailed analysis of systematic errors, the frequency is ($434 829 121 312 334 \pm 20_{stat} \pm 33_{sys}$) Hz.
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"abstract": "By varying the density of an ultracold $^{88}$Sr sample from $10^9$ cm$^{-3}$\nto $\u003e 10^{12}$ cm$^{-3}$, we make the first definitive measurement of the\ndensity-related frequency shift and linewidth broadening of the $^1S_0$ -\n$^3P_1$ optical clock transition in an alkaline earth system. In addition, we\nreport the most accurate measurement to date of the $^{88}$Sr $^1S_0 - ^3P_1$\noptical clock transition frequency. Including a detailed analysis of systematic\nerrors, the frequency is ($434 829 121 312 334 \\pm 20_{stat} \\pm 33_{sys}$) Hz.",
"arxiv_id": "physics/0410110",
"authors": [
"Tetsuya Ido",
"Thomas H. Loftus",
"Martin M. Boyd",
"Andrew D. Ludlow",
"Kevin W. Holman",
"Jun Ye"
],
"categories": [
"physics.atom-ph",
"physics.optics"
],
"doi": "10.1103/PhysRevLett.94.153001",
"journal_ref": "Phys. Rev. Lett. 94, 153001 (2005)",
"title": "Precision spectroscopy and density-dependent frequency shifts in ultracold Sr",
"url": "https://arxiv.org/abs/physics/0410110"
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