Standard

Search for solar axions produced by Primakoff conversion using resonant absorption by 169Tm nuclei. / Derbin, A. V.; Bakhlanov, S. V.; Egorov, A. I.; Mitropol'sky, I. A.; Muratova, V. N.; Semenov, D. A.; Unzhakov, E. V.

In: Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Vol. 678, No. 2, 13.07.2009, p. 181-185.

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

Harvard

Derbin, AV, Bakhlanov, SV, Egorov, AI, Mitropol'sky, IA, Muratova, VN, Semenov, DA & Unzhakov, EV 2009, 'Search for solar axions produced by Primakoff conversion using resonant absorption by 169Tm nuclei', Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, vol. 678, no. 2, pp. 181-185. https://doi.org/10.1016/j.physletb.2009.06.016

APA

Derbin, A. V., Bakhlanov, S. V., Egorov, A. I., Mitropol'sky, I. A., Muratova, V. N., Semenov, D. A., & Unzhakov, E. V. (2009). Search for solar axions produced by Primakoff conversion using resonant absorption by 169Tm nuclei. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 678(2), 181-185. https://doi.org/10.1016/j.physletb.2009.06.016

Vancouver

Derbin AV, Bakhlanov SV, Egorov AI, Mitropol'sky IA, Muratova VN, Semenov DA et al. Search for solar axions produced by Primakoff conversion using resonant absorption by 169Tm nuclei. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics. 2009 Jul 13;678(2):181-185. https://doi.org/10.1016/j.physletb.2009.06.016

Author

Derbin, A. V. ; Bakhlanov, S. V. ; Egorov, A. I. ; Mitropol'sky, I. A. ; Muratova, V. N. ; Semenov, D. A. ; Unzhakov, E. V. / Search for solar axions produced by Primakoff conversion using resonant absorption by 169Tm nuclei. In: Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics. 2009 ; Vol. 678, No. 2. pp. 181-185.

BibTeX

@article{a42045d2d7834a7499f7859192979966,
title = "Search for solar axions produced by Primakoff conversion using resonant absorption by 169Tm nuclei",
abstract = "The search for resonant absorption of the Primakoff solar axions by 169Tm nuclei have been performed. Such an absorption should lead to the excitation of low-lying nuclear energy level: A + 169Tm → 169Tm* → 169Tm + γ (8.41 keV). The Si(Li) detector and 169Tm target placed inside the low-background setup were used for that purpose. As a result, a new restriction on the axion-photon coupling and axion mass was obtained: gA γ (GeV- 1) ṡ mA (eV) ≤ 1.36 × 10- 5 (90% c.l.). In model of hadronic axion this restriction corresponds to the upper limit on axion mass - mA ≤ 191 eV for 90% c.l.",
keywords = "Low background measurements, Solar axion",
author = "Derbin, {A. V.} and Bakhlanov, {S. V.} and Egorov, {A. I.} and Mitropol'sky, {I. A.} and Muratova, {V. N.} and Semenov, {D. A.} and Unzhakov, {E. V.}",
year = "2009",
month = jul,
day = "13",
doi = "10.1016/j.physletb.2009.06.016",
language = "English",
volume = "678",
pages = "181--185",
journal = "Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics",
issn = "0370-2693",
publisher = "Elsevier",
number = "2",

}

RIS

TY - JOUR

T1 - Search for solar axions produced by Primakoff conversion using resonant absorption by 169Tm nuclei

AU - Derbin, A. V.

AU - Bakhlanov, S. V.

AU - Egorov, A. I.

AU - Mitropol'sky, I. A.

AU - Muratova, V. N.

AU - Semenov, D. A.

AU - Unzhakov, E. V.

PY - 2009/7/13

Y1 - 2009/7/13

N2 - The search for resonant absorption of the Primakoff solar axions by 169Tm nuclei have been performed. Such an absorption should lead to the excitation of low-lying nuclear energy level: A + 169Tm → 169Tm* → 169Tm + γ (8.41 keV). The Si(Li) detector and 169Tm target placed inside the low-background setup were used for that purpose. As a result, a new restriction on the axion-photon coupling and axion mass was obtained: gA γ (GeV- 1) ṡ mA (eV) ≤ 1.36 × 10- 5 (90% c.l.). In model of hadronic axion this restriction corresponds to the upper limit on axion mass - mA ≤ 191 eV for 90% c.l.

AB - The search for resonant absorption of the Primakoff solar axions by 169Tm nuclei have been performed. Such an absorption should lead to the excitation of low-lying nuclear energy level: A + 169Tm → 169Tm* → 169Tm + γ (8.41 keV). The Si(Li) detector and 169Tm target placed inside the low-background setup were used for that purpose. As a result, a new restriction on the axion-photon coupling and axion mass was obtained: gA γ (GeV- 1) ṡ mA (eV) ≤ 1.36 × 10- 5 (90% c.l.). In model of hadronic axion this restriction corresponds to the upper limit on axion mass - mA ≤ 191 eV for 90% c.l.

KW - Low background measurements

KW - Solar axion

UR - http://www.scopus.com/inward/record.url?scp=67649216924&partnerID=8YFLogxK

U2 - 10.1016/j.physletb.2009.06.016

DO - 10.1016/j.physletb.2009.06.016

M3 - Article

AN - SCOPUS:67649216924

VL - 678

SP - 181

EP - 185

JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

SN - 0370-2693

IS - 2

ER -

ID: 42278598