4.6 Article

Constraining the photon coupling of ultra-light dark-matter axion-like particles by polarization variations of parsec-scale jets in active galaxies

出版社

IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2019/02/059

关键词

particle physics; cosmology connection; cosmology of theories beyond the SM

资金

  1. NASA-Fermi GI grants [NNX08AV67G, NNX12A087G, NNX15AU76G]
  2. Russian Foundation for Basic Research [17-02-00197]
  3. government of the Russian Federation [05.Y09.21.0018]
  4. Alexander von Humboldt foundation
  5. Academy of Finland [274477, 284495, 312496]
  6. Russian Science Foundation [18-12-00258]
  7. Russian Science Foundation [18-12-00258] Funding Source: Russian Science Foundation
  8. NASA [94461, NNX08AV67G] Funding Source: Federal RePORTER
  9. Academy of Finland (AKA) [312496] Funding Source: Academy of Finland (AKA)

向作者/读者索取更多资源

Dark matter may consist of axion-like particles with ultra-low masses. Two-photon interactions of these particles affect the polarization of radiation propagating through the dark matter. Coherent oscillations of the Bose condensate of the particles induce periodic changes in the plane of polarisation of emission passing through the condensate. We estimate this effect and analyze MOJAVE VLBA polarization observations of bright downstream features in the parsec-scale jets of active galaxies. Through the non-observation of periodic changes in the polarization angle, we are able to constrain the photon coupling of the ultra-light dark-matter axion-like particles at the level of less than or similar to 10(-12) GeV-1 for masses between similar to 5 x 10(-23) eV and similar to 1.2 x 10(-21) eV.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.6
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据