We report on a direct search for scalar field dark matter using data from LIGO's third observing run. We analyze the coupling of size oscillations of the interferometer's beam splitter and arm test masses that may be caused by scalar field dark matter. Using new efficient search methods to maximize 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 up to four orders of magnitude in a frequency band from 10 to 180 Hz.

Göttel, A.s., Ejlli, A., Karan, K., Vermeulen, S.m., Aiello, L., Raymond, V., et al. (2024). Searching for Scalar Field Dark Matter with LIGO. PHYSICAL REVIEW LETTERS, 133(10) [10.1103/PhysRevLett.133.101001].

Searching for Scalar Field Dark Matter with LIGO

Lorenzo Aiello;
2024-01-01

Abstract

We report on a direct search for scalar field dark matter using data from LIGO's third observing run. We analyze the coupling of size oscillations of the interferometer's beam splitter and arm test masses that may be caused by scalar field dark matter. Using new efficient search methods to maximize 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 up to four orders of magnitude in a frequency band from 10 to 180 Hz.
2024
Pubblicato
Rilevanza internazionale
Articolo
Esperti anonimi
Settore PHYS-01/A - Fisica sperimentale delle interazioni fondamentali e applicazioni
English
Con Impact Factor ISI
dark matter; gravitational waves; LIGO
Göttel, A.s., Ejlli, A., Karan, K., Vermeulen, S.m., Aiello, L., Raymond, V., et al. (2024). Searching for Scalar Field Dark Matter with LIGO. PHYSICAL REVIEW LETTERS, 133(10) [10.1103/PhysRevLett.133.101001].
Göttel, As; Ejlli, A; Karan, K; Vermeulen, Sm; Aiello, L; Raymond, V; Grote, H
Articolo su rivista
File in questo prodotto:
File Dimensione Formato  
PhysRevLett.133.101001.pdf

accesso aperto

Tipologia: Versione Editoriale (PDF)
Licenza: Creative commons
Dimensione 887.98 kB
Formato Adobe PDF
887.98 kB Adobe PDF Visualizza/Apri

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/393012
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 0
  • ???jsp.display-item.citation.isi??? ND
social impact