Polarized targets as dark matter detectors

Y. K. Semertzidis; G. Baum; P. Berglund; S. Bültmann; C. M. Dulya; P. Hautle; N. Hayashi; S. Ishimoto; A. Kishi; Y. Kisselev; D. Krämer; J. Kyynäräinen; J. M. Le Goff; A. Magnon; T. Niinikoski

doi:10.1016/0168-9002(94)01460-4

Polarized targets as dark matter detectors

Y. K. Semertzidis
, G. Baum
, P. Berglund
, S. Bültmann
, C. M. Dulya
, P. Hautle
, N. Hayashi
, S. Ishimoto
, A. Kishi
, Y. Kisselev
, D. Krämer
, J. Kyynäräinen
, J. M. Le Goff
, A. Magnon
, T. Niinikoski

Not published at VTT

Research output: Contribution to journal › Article › Scientific › peer-review

3 Citations (Scopus)

Abstract

The strong electron paramagnetic resonance (EPR) of polarized targets can be used to search for axions as dark matter candidates in the range of (1-100) GHz. Once the axions are absorbed they can provide the communications gate for spin thermal contact between different nuclei that were kept artificially at different temperatures. © 1995.

Original language	English
Pages (from-to)	122-123
Number of pages	2
Journal	Nuclear Instruments and Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume	356
Issue number	1
DOIs	https://doi.org/10.1016/0168-9002(94)01460-4
Publication status	Published - 1 Mar 1995
MoE publication type	A1 Journal article-refereed

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10.1016/0168-9002(94)01460-4

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Semertzidis, Y. K., Baum, G., Berglund, P., Bültmann, S., Dulya, C. M., Hautle, P., Hayashi, N., Ishimoto, S., Kishi, A., Kisselev, Y., Krämer, D., Kyynäräinen, J., Le Goff, J. M., Magnon, A., & Niinikoski, T. (1995). Polarized targets as dark matter detectors. Nuclear Instruments and Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 356(1), 122-123. https://doi.org/10.1016/0168-9002(94)01460-4

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title = "Polarized targets as dark matter detectors",

abstract = "The strong electron paramagnetic resonance (EPR) of polarized targets can be used to search for axions as dark matter candidates in the range of (1-100) GHz. Once the axions are absorbed they can provide the communications gate for spin thermal contact between different nuclei that were kept artificially at different temperatures. {\textcopyright} 1995.",

author = "Semertzidis, \{Y. K.\} and G. Baum and P. Berglund and S. B{\"u}ltmann and Dulya, \{C. M.\} and P. Hautle and N. Hayashi and S. Ishimoto and A. Kishi and Y. Kisselev and D. Kr{\"a}mer and J. Kyyn{\"a}r{\"a}inen and \{Le Goff\}, \{J. M.\} and A. Magnon and T. Niinikoski",

year = "1995",

month = mar,

day = "1",

doi = "10.1016/0168-9002(94)01460-4",

language = "English",

volume = "356",

pages = "122--123",

journal = "Nuclear Instruments and Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors and Associated Equipment",

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Semertzidis, YK, Baum, G, Berglund, P, Bültmann, S, Dulya, CM, Hautle, P, Hayashi, N, Ishimoto, S, Kishi, A, Kisselev, Y, Krämer, D, Kyynäräinen, J, Le Goff, JM, Magnon, A & Niinikoski, T 1995, 'Polarized targets as dark matter detectors', Nuclear Instruments and Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 356, no. 1, pp. 122-123. https://doi.org/10.1016/0168-9002(94)01460-4

TY - JOUR

T1 - Polarized targets as dark matter detectors

AU - Semertzidis, Y. K.

AU - Baum, G.

AU - Berglund, P.

AU - Bültmann, S.

AU - Dulya, C. M.

AU - Hautle, P.

AU - Hayashi, N.

AU - Ishimoto, S.

AU - Kishi, A.

AU - Kisselev, Y.

AU - Krämer, D.

AU - Kyynäräinen, J.

AU - Le Goff, J. M.

AU - Magnon, A.

AU - Niinikoski, T.

PY - 1995/3/1

Y1 - 1995/3/1

N2 - The strong electron paramagnetic resonance (EPR) of polarized targets can be used to search for axions as dark matter candidates in the range of (1-100) GHz. Once the axions are absorbed they can provide the communications gate for spin thermal contact between different nuclei that were kept artificially at different temperatures. © 1995.

AB - The strong electron paramagnetic resonance (EPR) of polarized targets can be used to search for axions as dark matter candidates in the range of (1-100) GHz. Once the axions are absorbed they can provide the communications gate for spin thermal contact between different nuclei that were kept artificially at different temperatures. © 1995.

UR - https://www.scopus.com/pages/publications/0011720727

U2 - 10.1016/0168-9002(94)01460-4

DO - 10.1016/0168-9002(94)01460-4

M3 - Article

AN - SCOPUS:0011720727

SN - 0168-9002

VL - 356

SP - 122

EP - 123

JO - Nuclear Instruments and Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

JF - Nuclear Instruments and Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

IS - 1

ER -

Polarized targets as dark matter detectors

Abstract

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