Dark matter axion search using a Josephson Traveling wave parametric amplifier

C. Bartram; T. Braine; R. Cervantes; N. Crisosto; N. Du; G. Leum; P. Mohapatra; T. Nitta; L. J. Rosenberg; G. Rybka; J. Yang; John Clarke; I. Siddiqi; A. Agrawal; A. V. Dixit; M. H. Awida; A. S. Chou; M. Hollister; S. Knirck; A. Sonnenschein; W. Wester; J. R. Gleason; A. T. Hipp; S. Jois; P. Sikivie; N. S. Sullivan; D. B. Tanner; E. Lentz; R. Khatiwada; G. Carosi; C. Cisneros; N. Robertson; N. Woollett; L. D. Duffy; C. Boutan; M. Jones; B. H. Laroque; N. S. Oblath; M. S. Taubman; E. J. Daw; M. G. Perry; J. H. Buckley; C. Gaikwad; J. Hoffman; K. Murch; M. Goryachev; B. T. McAllister; A. Quiskamp; C. Thomson; M. E. Tobar; V. Bolkhovsky; G. Calusine; W. Oliver; K. Serniak

doi:10.1063/5.0122907

Dark matter axion search using a Josephson Traveling wave parametric amplifier

C. Bartram
, T. Braine
, R. Cervantes
, N. Crisosto
, N. Du
, G. Leum
, P. Mohapatra
, T. Nitta
, L. J. Rosenberg
, G. Rybka
, J. Yang
, John Clarke
, I. Siddiqi
, A. Agrawal
, A. V. Dixit
, M. H. Awida
, A. S. Chou
, M. Hollister
, S. Knirck
, A. Sonnenschein

W. Wester, J. R. Gleason, A. T. Hipp, S. Jois, P. Sikivie, N. S. Sullivan, D. B. Tanner, E. Lentz, R. Khatiwada, G. Carosi, C. Cisneros, N. Robertson, N. Woollett, L. D. Duffy, C. Boutan, M. Jones, B. H. Laroque, N. S. Oblath, M. S. Taubman, E. J. Daw, M. G. Perry, J. H. Buckley, C. Gaikwad, J. Hoffman, K. Murch, M. Goryachev, B. T. McAllister, A. Quiskamp, C. Thomson, M. E. Tobar, V. Bolkhovsky, G. Calusine, W. Oliver, K. Serniak

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67 Citations (Scopus)

Abstract

We describe the first implementation of a Josephson Traveling Wave Parametric Amplifier (JTWPA) in an axion dark matter search. The operation of the JTWPA for a period of about two weeks achieved sensitivity to axion-like particle dark matter with axion-photon couplings above 10-13 Ge V-1 over a narrow range of axion masses centered around 19.84 μeV by tuning the resonant frequency of the cavity over the frequency range of 4796.7-4799.5 MHz. The JTWPA was operated in the insert of the axion dark matter experiment as part of an independent receiver chain that was attached to a 0.56-l cavity. The ability of the JTWPA to deliver high gain over a wide (3 GHz) bandwidth has engendered interest from those aiming to perform broadband axion searches, a longstanding goal in this field.

Original language	English
Article number	044703
Journal	Review of Scientific Instruments
Volume	94
Issue number	4
DOIs	https://doi.org/10.1063/5.0122907
Publication status	Published - 1 Apr 2023

Funding

Funders	Funder number
ARC Australian Research Council	CE170100009, CE200100008

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10.1063/5.0122907

Cite this

Bartram, C., Braine, T., Cervantes, R., Crisosto, N., Du, N., Leum, G., Mohapatra, P., Nitta, T., Rosenberg, L. J., Rybka, G., Yang, J., Clarke, J., Siddiqi, I., Agrawal, A., Dixit, A. V., Awida, M. H., Chou, A. S., Hollister, M., Knirck, S., ... Serniak, K. (2023). Dark matter axion search using a Josephson Traveling wave parametric amplifier. Review of Scientific Instruments, 94(4), Article 044703. https://doi.org/10.1063/5.0122907

@article{8857f5de74444fdea771e6ca12821dec,

title = "Dark matter axion search using a Josephson Traveling wave parametric amplifier",

abstract = "We describe the first implementation of a Josephson Traveling Wave Parametric Amplifier (JTWPA) in an axion dark matter search. The operation of the JTWPA for a period of about two weeks achieved sensitivity to axion-like particle dark matter with axion-photon couplings above 10-13 Ge V-1 over a narrow range of axion masses centered around 19.84 μeV by tuning the resonant frequency of the cavity over the frequency range of 4796.7-4799.5 MHz. The JTWPA was operated in the insert of the axion dark matter experiment as part of an independent receiver chain that was attached to a 0.56-l cavity. The ability of the JTWPA to deliver high gain over a wide (3 GHz) bandwidth has engendered interest from those aiming to perform broadband axion searches, a longstanding goal in this field.",

author = "C. Bartram and T. Braine and R. Cervantes and N. Crisosto and N. Du and G. Leum and P. Mohapatra and T. Nitta and Rosenberg, \{L. J.\} and G. Rybka and J. Yang and John Clarke and I. Siddiqi and A. Agrawal and Dixit, \{A. V.\} and Awida, \{M. H.\} and Chou, \{A. S.\} and M. Hollister and S. Knirck and A. Sonnenschein and W. Wester and Gleason, \{J. R.\} and Hipp, \{A. T.\} and S. Jois and P. Sikivie and Sullivan, \{N. S.\} and Tanner, \{D. B.\} and E. Lentz and R. Khatiwada and G. Carosi and C. Cisneros and N. Robertson and N. Woollett and Duffy, \{L. D.\} and C. Boutan and M. Jones and Laroque, \{B. H.\} and Oblath, \{N. S.\} and Taubman, \{M. S.\} and Daw, \{E. J.\} and Perry, \{M. G.\} and Buckley, \{J. H.\} and C. Gaikwad and J. Hoffman and K. Murch and M. Goryachev and McAllister, \{B. T.\} and A. Quiskamp and C. Thomson and Tobar, \{M. E.\} and V. Bolkhovsky and G. Calusine and W. Oliver and K. Serniak",

note = "Funding Information: This work was supported by the U.S. Department of Energy through Grants Nos. DE-SC0009800, DESC0009723, DE-SC0010296, DE-SC0010280, DE-SC0011665, DEFG02-97ER41029, DEFG02-96ER40956, DEAC52-07NA27344, DEC03-76SF00098, and DE-SC0017987. Fermilab is a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. Additional support was provided by the Heising-Simons Foundation and the Lawrence Livermore National Laboratory and Pacific Northwest National Laboratory LDRD offices (LLNL Release No. LLNL-JRNL-825283). UWA was funded by the ARC Center of Excellence for Engineered Quantum Systems (Grant No. CE170100009) and Dark Matter Particle Physics (Grant No. CE200100008). Ben McAllister was funded by the Forrest Research Foundation. Tatsumi Nitta was supported by JSPS Overseas Research Fellowships No. 202060305. MIT Lincoln Laboratory acknowledges support from the Office of the Director of National Intelligence (ODNI), Intelligence Advanced Research Projects Activity (IARPA), under Air Force Contract No. FA8721-05-C-0002. The views and conclusions contained herein are those of the authors and should not be interpreted as necessarily representing the official policies or endorsements, either expressed or implied, of ODNI, IARPA, or the U.S. Government. Publisher Copyright: {\textcopyright} 2023 Author(s).",

year = "2023",

month = apr,

day = "1",

doi = "10.1063/5.0122907",

language = "English",

volume = "94",

journal = "Review of Scientific Instruments",

issn = "0034-6748",

publisher = "American Institute of Physics",

number = "4",

}

Bartram, C, Braine, T, Cervantes, R, Crisosto, N, Du, N, Leum, G, Mohapatra, P, Nitta, T, Rosenberg, LJ, Rybka, G, Yang, J, Clarke, J, Siddiqi, I, Agrawal, A, Dixit, AV, Awida, MH, Chou, AS, Hollister, M, Knirck, S, Sonnenschein, A, Wester, W, Gleason, JR, Hipp, AT, Jois, S, Sikivie, P, Sullivan, NS, Tanner, DB, Lentz, E, Khatiwada, R, Carosi, G, Cisneros, C, Robertson, N, Woollett, N, Duffy, LD, Boutan, C, Jones, M, Laroque, BH, Oblath, NS, Taubman, MS, Daw, EJ, Perry, MG, Buckley, JH, Gaikwad, C, Hoffman, J, Murch, K, Goryachev, M , McAllister, BT, Quiskamp, A, Thomson, C, Tobar, ME, Bolkhovsky, V, Calusine, G, Oliver, W & Serniak, K 2023, 'Dark matter axion search using a Josephson Traveling wave parametric amplifier', Review of Scientific Instruments, vol. 94, no. 4, 044703. https://doi.org/10.1063/5.0122907

TY - JOUR

T1 - Dark matter axion search using a Josephson Traveling wave parametric amplifier

AU - Bartram, C.

AU - Braine, T.

AU - Cervantes, R.

AU - Crisosto, N.

AU - Du, N.

AU - Leum, G.

AU - Mohapatra, P.

AU - Nitta, T.

AU - Rosenberg, L. J.

AU - Rybka, G.

AU - Yang, J.

AU - Clarke, John

AU - Siddiqi, I.

AU - Agrawal, A.

AU - Dixit, A. V.

AU - Awida, M. H.

AU - Chou, A. S.

AU - Hollister, M.

AU - Knirck, S.

AU - Sonnenschein, A.

AU - Wester, W.

AU - Gleason, J. R.

AU - Hipp, A. T.

AU - Jois, S.

AU - Sikivie, P.

AU - Sullivan, N. S.

AU - Tanner, D. B.

AU - Lentz, E.

AU - Khatiwada, R.

AU - Carosi, G.

AU - Cisneros, C.

AU - Robertson, N.

AU - Woollett, N.

AU - Duffy, L. D.

AU - Boutan, C.

AU - Jones, M.

AU - Laroque, B. H.

AU - Oblath, N. S.

AU - Taubman, M. S.

AU - Daw, E. J.

AU - Perry, M. G.

AU - Buckley, J. H.

AU - Gaikwad, C.

AU - Hoffman, J.

AU - Murch, K.

AU - Goryachev, M.

AU - McAllister, B. T.

AU - Quiskamp, A.

AU - Thomson, C.

AU - Tobar, M. E.

AU - Bolkhovsky, V.

AU - Calusine, G.

AU - Oliver, W.

AU - Serniak, K.

N1 - Funding Information: This work was supported by the U.S. Department of Energy through Grants Nos. DE-SC0009800, DESC0009723, DE-SC0010296, DE-SC0010280, DE-SC0011665, DEFG02-97ER41029, DEFG02-96ER40956, DEAC52-07NA27344, DEC03-76SF00098, and DE-SC0017987. Fermilab is a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. Additional support was provided by the Heising-Simons Foundation and the Lawrence Livermore National Laboratory and Pacific Northwest National Laboratory LDRD offices (LLNL Release No. LLNL-JRNL-825283). UWA was funded by the ARC Center of Excellence for Engineered Quantum Systems (Grant No. CE170100009) and Dark Matter Particle Physics (Grant No. CE200100008). Ben McAllister was funded by the Forrest Research Foundation. Tatsumi Nitta was supported by JSPS Overseas Research Fellowships No. 202060305. MIT Lincoln Laboratory acknowledges support from the Office of the Director of National Intelligence (ODNI), Intelligence Advanced Research Projects Activity (IARPA), under Air Force Contract No. FA8721-05-C-0002. The views and conclusions contained herein are those of the authors and should not be interpreted as necessarily representing the official policies or endorsements, either expressed or implied, of ODNI, IARPA, or the U.S. Government. Publisher Copyright: © 2023 Author(s).

PY - 2023/4/1

Y1 - 2023/4/1

N2 - We describe the first implementation of a Josephson Traveling Wave Parametric Amplifier (JTWPA) in an axion dark matter search. The operation of the JTWPA for a period of about two weeks achieved sensitivity to axion-like particle dark matter with axion-photon couplings above 10-13 Ge V-1 over a narrow range of axion masses centered around 19.84 μeV by tuning the resonant frequency of the cavity over the frequency range of 4796.7-4799.5 MHz. The JTWPA was operated in the insert of the axion dark matter experiment as part of an independent receiver chain that was attached to a 0.56-l cavity. The ability of the JTWPA to deliver high gain over a wide (3 GHz) bandwidth has engendered interest from those aiming to perform broadband axion searches, a longstanding goal in this field.

AB - We describe the first implementation of a Josephson Traveling Wave Parametric Amplifier (JTWPA) in an axion dark matter search. The operation of the JTWPA for a period of about two weeks achieved sensitivity to axion-like particle dark matter with axion-photon couplings above 10-13 Ge V-1 over a narrow range of axion masses centered around 19.84 μeV by tuning the resonant frequency of the cavity over the frequency range of 4796.7-4799.5 MHz. The JTWPA was operated in the insert of the axion dark matter experiment as part of an independent receiver chain that was attached to a 0.56-l cavity. The ability of the JTWPA to deliver high gain over a wide (3 GHz) bandwidth has engendered interest from those aiming to perform broadband axion searches, a longstanding goal in this field.

UR - https://www.scopus.com/pages/publications/85153317106

U2 - 10.1063/5.0122907

DO - 10.1063/5.0122907

M3 - Article

C2 - 38081262

AN - SCOPUS:85153317106

SN - 0034-6748

VL - 94

JO - Review of Scientific Instruments

JF - Review of Scientific Instruments

IS - 4

M1 - 044703

ER -

Dark matter axion search using a Josephson Traveling wave parametric amplifier

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ARC Centre of Excellence for Engineered Quantum Systems (EQuS 2017)

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