In+115−Yb+172 Coulomb Crystal Clock with 2.5×10−18 Systematic Uncertainty

IF 9 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Physical review letters Pub Date : 2025-01-16 DOI:10.1103/physrevlett.134.023201
H. N. Hausser, J. Keller, T. Nordmann, N. M. Bhatt, J. Kiethe, H. Liu, I. M. Richter, M. von Boehn, J. Rahm, S. Weyers, E. Benkler, B. Lipphardt, S. Dörscher, K. Stahl, J. Klose, C. Lisdat, M. Filzinger, N. Huntemann, E. Peik, T. E. Mehlstäubler
{"title":"In+115−Yb+172 Coulomb Crystal Clock with 2.5×10−18 Systematic Uncertainty","authors":"H. N. Hausser, J. Keller, T. Nordmann, N. M. Bhatt, J. Kiethe, H. Liu, I. M. Richter, M. von Boehn, J. Rahm, S. Weyers, E. Benkler, B. Lipphardt, S. Dörscher, K. Stahl, J. Klose, C. Lisdat, M. Filzinger, N. Huntemann, E. Peik, T. E. Mehlstäubler","doi":"10.1103/physrevlett.134.023201","DOIUrl":null,"url":null,"abstract":"We present a scalable mixed-species Coulomb crystal clock based on the S</a:mi></a:mrow>0</a:mn></a:mrow></a:msub></a:mrow>1</a:mn></a:mrow></a:mmultiscripts></a:mrow>↔</a:mo>P</a:mi></a:mrow>3</a:mn></a:mrow></a:mmultiscripts></a:mrow>0</a:mn></a:mrow></a:msub></a:mrow></a:math> transition in <d:math xmlns:d=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><d:mrow><d:mmultiscripts><d:mrow><d:msup><d:mrow><d:mi>In</d:mi></d:mrow><d:mrow><d:mo>+</d:mo></d:mrow></d:msup></d:mrow><d:mprescripts/><d:none/><d:mrow><d:mn>115</d:mn></d:mrow></d:mmultiscripts></d:mrow></d:math>. <f:math xmlns:f=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><f:mrow><f:mmultiscripts><f:mrow><f:msup><f:mrow><f:mi>Yb</f:mi></f:mrow><f:mrow><f:mo>+</f:mo></f:mrow></f:msup></f:mrow><f:mprescripts/><f:none/><f:mrow><f:mn>172</f:mn></f:mrow></f:mmultiscripts></f:mrow></f:math> ions are cotrapped and used for sympathetic cooling. Reproducible interrogation conditions for mixed-species Coulomb crystals are ensured by a conditional preparation sequence with permutation control. We demonstrate clock operation with a <h:math xmlns:h=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><h:mrow><h:mn>1</h:mn><h:msup><h:mrow><h:mi>In</h:mi></h:mrow><h:mrow><h:mo>+</h:mo></h:mrow></h:msup><h:mtext>−</h:mtext><h:mn>3</h:mn><h:msup><h:mrow><h:mi>Yb</h:mi></h:mrow><h:mrow><h:mo>+</h:mo></h:mrow></h:msup></h:mrow></h:math> crystal, achieving a relative systematic uncertainty of <j:math xmlns:j=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><j:mn>2.5</j:mn><j:mo>×</j:mo><j:msup><j:mn>10</j:mn><j:mrow><j:mo>−</j:mo><j:mn>18</j:mn></j:mrow></j:msup></j:math> and a relative frequency instability of <l:math xmlns:l=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><l:mrow><l:mn>1.6</l:mn><l:mo>×</l:mo><l:msup><l:mrow><l:mn>10</l:mn></l:mrow><l:mrow><l:mo>−</l:mo><l:mn>15</l:mn></l:mrow></l:msup><l:mo>/</l:mo><l:msqrt><l:mrow><l:mi>τ</l:mi><l:mo>/</l:mo><l:mn>1</l:mn><l:mtext> </l:mtext><l:mtext> </l:mtext><l:mi mathvariant=\"normal\">s</l:mi></l:mrow></l:msqrt></l:mrow></l:math>. We report on absolute frequency measurements with an uncertainty of <o:math xmlns:o=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><o:mn>1.3</o:mn><o:mo>×</o:mo><o:msup><o:mn>10</o:mn><o:mrow><o:mo>−</o:mo><o:mn>16</o:mn></o:mrow></o:msup></o:math> and optical frequency comparisons with clocks based on <q:math xmlns:q=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><q:mrow><q:mmultiscripts><q:mrow><q:msup><q:mrow><q:mi>Yb</q:mi></q:mrow><q:mrow><q:mo>+</q:mo></q:mrow></q:msup></q:mrow><q:mprescripts/><q:none/><q:mrow><q:mn>171</q:mn></q:mrow></q:mmultiscripts></q:mrow></q:math> (<s:math xmlns:s=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><s:mi>E</s:mi><s:mn>3</s:mn></s:math>) and <u:math xmlns:u=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><u:mrow><u:mmultiscripts><u:mrow><u:mi>Sr</u:mi></u:mrow><u:mprescripts/><u:none/><u:mrow><u:mn>87</u:mn></u:mrow></u:mmultiscripts></u:mrow></u:math>. With a fractional uncertainty of <w:math xmlns:w=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><w:mn>4.4</w:mn><w:mo>×</w:mo><w:msup><w:mn>10</w:mn><w:mrow><w:mo>−</w:mo><w:mn>18</w:mn></w:mrow></w:msup></w:math>, the former is—to our knowledge—the most accurate frequency ratio value reported to date. For the <y:math xmlns:y=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><y:mrow><y:mrow><y:mmultiscripts><y:mrow><y:msup><y:mrow><y:mi>In</y:mi></y:mrow><y:mrow><y:mo>+</y:mo></y:mrow></y:msup></y:mrow><y:mprescripts/><y:none/><y:mrow><y:mn>115</y:mn></y:mrow></y:mmultiscripts></y:mrow><y:mo>/</y:mo><y:mrow><y:mmultiscripts><y:mrow><y:mi>Sr</y:mi></y:mrow><y:mprescripts/><y:none/><y:mrow><y:mn>87</y:mn></y:mrow></y:mmultiscripts></y:mrow></y:mrow></y:math> ratio, we improve upon the best previous measurement by more than an order of magnitude. We also demonstrate operation with four In</ab:mi></ab:mrow>+</ab:mo></ab:mrow></ab:msup></ab:mrow>115</ab:mn></ab:mrow></ab:mmultiscripts></ab:mrow></ab:math> clock ions, which reduces the instability to <cb:math xmlns:cb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><cb:mrow><cb:mn>9.2</cb:mn><cb:mo>×</cb:mo><cb:msup><cb:mrow><cb:mn>10</cb:mn></cb:mrow><cb:mrow><cb:mo>−</cb:mo><cb:mn>16</cb:mn></cb:mrow></cb:msup><cb:mo>/</cb:mo><cb:msqrt><cb:mrow><cb:mi>τ</cb:mi><cb:mo>/</cb:mo><cb:mn>1</cb:mn><cb:mtext> </cb:mtext><cb:mtext> </cb:mtext><cb:mi mathvariant=\"normal\">s</cb:mi></cb:mrow></cb:msqrt></cb:mrow></cb:math>. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20069,"journal":{"name":"Physical review letters","volume":"30 1","pages":""},"PeriodicalIF":9.0000,"publicationDate":"2025-01-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical review letters","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/physrevlett.134.023201","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
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Abstract

We present a scalable mixed-species Coulomb crystal clock based on the S01↔P30 transition in In+115. Yb+172 ions are cotrapped and used for sympathetic cooling. Reproducible interrogation conditions for mixed-species Coulomb crystals are ensured by a conditional preparation sequence with permutation control. We demonstrate clock operation with a 1In+3Yb+ crystal, achieving a relative systematic uncertainty of 2.5×1018 and a relative frequency instability of 1.6×1015/τ/1 s. We report on absolute frequency measurements with an uncertainty of 1.3×1016 and optical frequency comparisons with clocks based on Yb+171 (E3) and Sr87. With a fractional uncertainty of 4.4×1018, the former is—to our knowledge—the most accurate frequency ratio value reported to date. For the In+115/Sr87 ratio, we improve upon the best previous measurement by more than an order of magnitude. We also demonstrate operation with four In+115 clock ions, which reduces the instability to 9.2×1016/τ/1 s. Published by the American Physical Society 2025
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在+115−Yb+172库仑晶体时钟2.5×10−18系统不确定度
我们提出了一个基于in +115中S01↔P30过渡的可扩展混合态库伦晶体时钟。Yb+172离子被捕获并用于交感冷却。通过有条件的排列控制制备序列,保证了混合种库仑晶体的再现性。我们演示了1 in +−3Yb+晶体的时钟操作,实现了2.5×10−18的相对系统不确定性和1.6×10−15/τ/ 1s的相对频率不稳定性。我们报告了不确定度为1.3×10−16的绝对频率测量和基于Yb+171 (E3)和Sr87的时钟的光频率比较。分数不确定性为4.4×10 - 18,据我们所知,前者是迄今为止报告的最准确的频率比值。对于In+115/Sr87的比值,我们比之前最好的测量结果提高了一个数量级以上。我们还演示了4个In+115时钟离子的操作,将不稳定性降低到9.2×10−16/τ/1 s。2025年由美国物理学会出版
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来源期刊
Physical review letters
Physical review letters 物理-物理:综合
CiteScore
16.50
自引率
7.00%
发文量
2673
审稿时长
2.2 months
期刊介绍: Physical review letters(PRL)covers the full range of applied, fundamental, and interdisciplinary physics research topics: General physics, including statistical and quantum mechanics and quantum information Gravitation, astrophysics, and cosmology Elementary particles and fields Nuclear physics Atomic, molecular, and optical physics Nonlinear dynamics, fluid dynamics, and classical optics Plasma and beam physics Condensed matter and materials physics Polymers, soft matter, biological, climate and interdisciplinary physics, including networks
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