Dmitry Budker

Prof. Dr. Dmitry Budker

orcid
JGU, Helmholtz Institute Mainz, UC Berkeley

Research Focus & Metrics

Academic Career Length

34Years (1993-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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14 September 2008 in Nature Physics
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JTJ. M. Taylor
J. M. Taylor
PCP. Cappellaro
P. Cappellaro
LCL. Childress
L. Childress
LJL. Jiang
L. Jiang
Dmitry BudkerDmitry Budker
Dmitry Budker
MLM. D. Lukin
M. D. Lukin

1 April 2007 in Nature Physics
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Journal Article
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Dmitry BudkerDmitry Budker
Dmitry Budker
MRMichael Romalis
Michael Romalis

23 April 2013 in Nature Communications
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Journal Article
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NBN. Bar-Gill
N. Bar-Gill
LPL.M. Pham
L.M. Pham
AJA. Jarmola
A. Jarmola
Dmitry BudkerDmitry Budker
Dmitry Budker
RWR.L. Walsworth
R.L. Walsworth

17 February 2010 in Physical Review Letters
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Journal Article
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VAV. M. Acosta
V. M. Acosta
EBE. Bauch
E. Bauch
MLM. P. Ledbetter
M. P. Ledbetter
AWA. Waxman
A. Waxman
LBL.-S. Bouchard
L.-S. Bouchard
Dmitry BudkerDmitry Budker
Dmitry Budker
The temperature dependence of the magnetic-resonance spectra of nitrogen-vacancy (NV−) ensembles in the range of 280–330 K was studied. Four samples prepared under different conditions were analyzed with NV− concentrations ranging from 10 ppb to 15 ppm. For all samples, the axial zero-field splitting (ZFS) parameter D was found to vary significantly with temperature, T, as dD/dT=−74.2(7)  kHz/K. The transverse ZFS parameter E was nonzero (between 4 and 11 MHz) in all samples, and exhibited a temperature dependence of dE/(EdT)=−1.4(3)×10−4  K−1. The results might be accounted for by considering local thermal expansion. The temperature dependence of the ZFS parameters presents a significant challenge for diamond magnetometers and may ultimately limit their bandwidth and sensitivity.

20 November 2002 in Reviews of Modern Physics
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Dmitry BudkerDmitry Budker
Dmitry Budker
WGWojciech Gawlik
Wojciech Gawlik
DKD. F. Kimball
D. F. Kimball
SRS. M. Rochester
S. M. Rochester
VYV. V. Yashchuk
V. V. Yashchuk
AWA. Weis
A. Weis
The authors review the history, current status, physical mechanisms, experimental methods, and applications of nonlinear magneto-optical effects in atomic vapors. They begin by describing the pioneering work of Macaluso and Corbino over a century ago on linear magneto-optical effects (in which the properties of the medium do not depend on the light power) in the vicinity of atomic resonances. These effects are then contrasted with various nonlinear magneto-optical phenomena that have been studied both theoretically and experimentally since the late 1960s. In recent years, the field of nonlinear magneto-optics has experienced a revival of interest that has led to a number of developments, including the observation of ultranarrow (1-Hz) magneto-optical resonances, applications in sensitive magnetometry, nonlinear magneto-optical tomography, and the possibility of a search for parity- and time-reversal-invariance violation in atoms.

19 May 2014 in Physical Review X
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Dmitry BudkerDmitry Budker
Dmitry Budker
PGPeter W. Graham
Peter W. Graham
MLMicah Ledbetter
Micah Ledbetter
SRSurjeet Rajendran
Surjeet Rajendran
ASAlexander O. Sushkov
Alexander O. Sushkov
We propose an experiment to search for QCD axion and axionlike-particle dark matter. Nuclei that are interacting with the background axion dark matter acquire time-varying CP-odd nuclear moments such as an electric dipole moment. In analogy with nuclear magnetic resonance, these moments cause precession of nuclear spins in a material sample in the presence of an electric field. Precision magnetometry can be used to search for such precession. An initial phase of this experiment could cover many orders of magnitude in axionlike-particle parameter space beyond the current astrophysical and laboratory limits. And with established techniques, the proposed experimental scheme has sensitivity to QCD axion masses ma≲10−9  eV, corresponding to theoretically well-motivated axion decay constants fa≳1016  GeV. With further improvements, this experiment could ultimately cover the entire range of masses ma≲μ  eV, complementary to cavity searches.