50th Annual Meeting of the APS Division of Atomic, Molecular and Optical Physics APS Meeting
Volume 64, Number 4
Monday–Friday, May 27–31, 2019;
Milwaukee, Wisconsin
Session W02: Hot Topics
10:30 AM–12:30 PM,
Friday, May 31, 2019
Wisconsin Center
Room: 101AB
Chair: John Bollinger, NIST Boulder
Abstract: W02.00003 : The challenge of a nuclear clock: Recent progress and perspectives
11:30 AM–12:00 PM
Preview Abstract
Abstract
Author:
Lars von der Wense
(Ludwig Maximilians Universität München)
A nuclear optical clock based on a single $^{229}$Th ion is expected to achieve a higher accuracy
than the best atomic clocks operational today [1]. Although already proposed back in 2003
[2], this nuclear clock has not yet become reality. The main obstacle that has so far hindered
the development of a nuclear clock was an unprecise knowledge of the energy value of a
nuclear excited state of the $^{229}$Th nucleus, generally known as the $^{229}$Th isomer. This metastable
nuclear excited state is the one of lowest energy in whole nuclear landscape and – with an
energy of less than 10 eV – in principle allows for direct nuclear laser excitation, which poses
a central requirement for the development of a nuclear clock.\\
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In the past few years significant progress toward the development of a nuclear clock has been
made: Starting with a first direct detection of the 229 Th isomer in 2016 based on its internal
conversion decay channel [3], the isomeric lifetime could be determined in 2017 [4], followed
by a first laser-spectroscopic characterization in 2018 [5]. Most recently a first energy
determination based on the isomer’s direct detection was successful, thereby constraining the
isomeric energy value to sufficient precision to determine the laser technology required in the
nuclear clock concept and paving the way for first nuclear laser spectroscopy experiments [6].\\
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In the presentation I will give an overview over the current status of the nuclear clock
development, with a particular focus on the most recent progress. Also the next required steps
will be detailed and future perspectives will be given.\\
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[1] C.J. Campbell et al., Phys. Rev. Lett. 108, 120802 (2012).
[2] E. Peik, C. Tamm, Eur. Phys. Lett. 61, 181 (2003).
[3] L. von der Wense et al., Nature 533, 47 (2016).
[4] B. Seiferle et al., Phys. Rev. Lett. 118, 042501 (2017).
[5] J. Thielking et al., Nature 556, 321 (2018).
[6] B. Seiferle et al., submitted for publication (2019)\\
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In collaboration with: Benedict Seiferle, Peter G. Thirolf