• Masses of Binary Black Hole Mergers
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  • Release time: 2022-04-20
  • detected frequency
  • emitted frequency
  • black hole binary merger
  • time dilation
  • mass gap
Video Introduction

Researchers show that masses of binary black hole mergers are overestimated, since a large gravitational redshift is not taken into account. Such a phenomenon occurs due to time dilation in a close neighborhood of any black hole. This fact allows us to explain a high mass gap between observed binary neutron stars and calculated binary black hole mergers. They also present other reasons why masses of black hole mergers are determined incorrectly. 

This video is adapted from 10.3390/galaxies10020052

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Křížek, M. Masses of Binary Black Hole Mergers. Encyclopedia. Available online: https://encyclopedia.pub/video/video_detail/290 (accessed on 05 July 2022).
Křížek M. Masses of Binary Black Hole Mergers. Encyclopedia. Available at: https://encyclopedia.pub/video/video_detail/290. Accessed July 05, 2022.
Křížek, Michal. "Masses of Binary Black Hole Mergers," Encyclopedia, https://encyclopedia.pub/video/video_detail/290 (accessed July 05, 2022).
Křížek, M. (2022, April 20). Masses of Binary Black Hole Mergers. In Encyclopedia. https://encyclopedia.pub/video/video_detail/290
Křížek, Michal. ''Masses of Binary Black Hole Mergers.'' Encyclopedia. Web. 20 April, 2022.
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