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Ground-state electromagnetically-induced-transparency cooling of Yb + 171 ions in a polychromatic field. / Krysenko, D. S.; Prudnikov, O. N.; Taichenachev, A. V. et al.

In: Physical Review A, Vol. 108, No. 4, 043114, 10.2023.

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@article{9267d9acc0d044a58fd349a2f6202fb3,
title = "Ground-state electromagnetically-induced-transparency cooling of Yb + 171 ions in a polychromatic field",
abstract = "We propose a scheme of deep laser cooling of Yb+171, which is based on the effect of electromagnetically induced transparency (EIT) in a polychromatic field with three frequency components resonant with optical transitions of the S1/22→P1/22 line. The deep cooling down to the ground motional state in a trap allows for a significant suppression of the second-order Doppler shift in the frequency standard. Moreover, in our scheme, there is no need to use a magnetic field, which is required for Doppler cooling of Yb+171 in a field with a two frequency component. Cooling without the use of a magnetic field is important for the deep suppression of quadratic Zeeman shifts of clock transitions due to an uncontrolled residual magnetic field.",
author = "Krysenko, {D. S.} and Prudnikov, {O. N.} and Taichenachev, {A. V.} and Yudin, {V. I.} and Chepurov, {S. V.} and Bagaev, {S. N.}",
note = "The research was supported by the Russian Science Foundation (Project No. 23-22-00198). The work of A.V.T. was supported by the Russian Science Foundation (Project No. 23-12-00182), and V.I.Y. was supported by the Ministry of Science and Higher Education of the Russian Federation (Project No. FSUS-2020-0036).",
year = "2023",
month = oct,
doi = "10.1103/PhysRevA.108.043114",
language = "English",
volume = "108",
journal = "Physical Review A",
issn = "2469-9926",
publisher = "American Physical Society",
number = "4",

}

RIS

TY - JOUR

T1 - Ground-state electromagnetically-induced-transparency cooling of Yb + 171 ions in a polychromatic field

AU - Krysenko, D. S.

AU - Prudnikov, O. N.

AU - Taichenachev, A. V.

AU - Yudin, V. I.

AU - Chepurov, S. V.

AU - Bagaev, S. N.

N1 - The research was supported by the Russian Science Foundation (Project No. 23-22-00198). The work of A.V.T. was supported by the Russian Science Foundation (Project No. 23-12-00182), and V.I.Y. was supported by the Ministry of Science and Higher Education of the Russian Federation (Project No. FSUS-2020-0036).

PY - 2023/10

Y1 - 2023/10

N2 - We propose a scheme of deep laser cooling of Yb+171, which is based on the effect of electromagnetically induced transparency (EIT) in a polychromatic field with three frequency components resonant with optical transitions of the S1/22→P1/22 line. The deep cooling down to the ground motional state in a trap allows for a significant suppression of the second-order Doppler shift in the frequency standard. Moreover, in our scheme, there is no need to use a magnetic field, which is required for Doppler cooling of Yb+171 in a field with a two frequency component. Cooling without the use of a magnetic field is important for the deep suppression of quadratic Zeeman shifts of clock transitions due to an uncontrolled residual magnetic field.

AB - We propose a scheme of deep laser cooling of Yb+171, which is based on the effect of electromagnetically induced transparency (EIT) in a polychromatic field with three frequency components resonant with optical transitions of the S1/22→P1/22 line. The deep cooling down to the ground motional state in a trap allows for a significant suppression of the second-order Doppler shift in the frequency standard. Moreover, in our scheme, there is no need to use a magnetic field, which is required for Doppler cooling of Yb+171 in a field with a two frequency component. Cooling without the use of a magnetic field is important for the deep suppression of quadratic Zeeman shifts of clock transitions due to an uncontrolled residual magnetic field.

UR - https://www.scopus.com/record/display.uri?eid=2-s2.0-85176389673&origin=inward&txGid=ac76775685e0cb1b032bcddb41c5033e

UR - https://www.mendeley.com/catalogue/7623ed07-aa42-3e33-b132-3590abae73b3/

U2 - 10.1103/PhysRevA.108.043114

DO - 10.1103/PhysRevA.108.043114

M3 - Article

VL - 108

JO - Physical Review A

JF - Physical Review A

SN - 2469-9926

IS - 4

M1 - 043114

ER -

ID: 59284429