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.

в: Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Том 678, № 2, 13.07.2009, стр. 181-185.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

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, Том. 678, № 2, стр. 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 и пр. 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 Июль 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. в: Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics. 2009 ; Том 678, № 2. стр. 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