日本語
 
Help Privacy Policy ポリシー/免責事項
  詳細検索ブラウズ

アイテム詳細


公開

学術論文

Searching for scalar field dark matter with LIGO

MPS-Authors

Ejlli ,  Aldo
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons231107

Karan,  Kanioar
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

External Resource
There are no locators available
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
フルテキスト (公開)

2401.18076.pdf
(プレプリント), 2MB

PhysRevLett.133.101001.pdf
(出版社版), 888KB

付随資料 (公開)
There is no public supplementary material available
引用

Göttel, A. S., Ejlli, A., Karan, K., Vermeulen, S. M., Aiello, L., Raymond, V., & Grote, H. (2024). Searching for scalar field dark matter with LIGO. Physical Review Letters, 133(10):. doi:10.1103/PhysRevLett.133.101001.


引用: https://hdl.handle.net/21.11116/0000-000F-DF9D-6
要旨
We report on a direct search for scalar field dark matter using data from
LIGO's third observing run. We analyse the coupling of size oscillations of the
interferometer's beamsplitter and arm test masses that may be caused by scalar
field dark matter. Using new efficient search methods to maximise sensitivity
for signatures of such oscillations, we set new upper limits for the coupling
constants of scalar field dark matter as a function of its mass, which improve
upon bounds from previous direct searches by several orders of magnitude in a
frequency band from 10 Hz to 180 Hz.