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

This video is adapted from 10.3390/galaxies10020052

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. 

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If you have any further questions, please contact Encyclopedia Editorial Office.
Křížek, M. Masses of Binary Black Hole Mergers. Encyclopedia. Available online: https://encyclopedia.pub/video/video_detail/290 (accessed on 15 November 2024).
Křížek M. Masses of Binary Black Hole Mergers. Encyclopedia. Available at: https://encyclopedia.pub/video/video_detail/290. Accessed November 15, 2024.
Křížek, Michal. "Masses of Binary Black Hole Mergers" Encyclopedia, https://encyclopedia.pub/video/video_detail/290 (accessed November 15, 2024).
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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