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Detection of Black Holes01:10

Detection of Black Holes

Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
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X-ray Imaging01:24

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German physicist Wilhelm Röntgen (1845–1923) was experimenting with electrical current when he discovered that a mysterious and invisible "ray" would pass through his flesh but leave an outline of his bones on a screen coated with a metal compound. In 1895, Röntgen made the first durable record of the internal parts of a living human: an "X-ray" image (as it came to be called) of his wife’s hand. Scientists worldwide quickly began their own experiments with X-rays, and by 1900, X-ray was widely...

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Related Experiment Video

Updated: Jun 21, 2026

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera
06:28

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera

Published on: January 30, 2020

Robust identification of isotropic diffuse gamma rays from galactic dark matter.

Jennifer M Siegal-Gaskins1, Vasiliki Pavlidou

  • 1Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, Ohio 43210, USA.

Physical Review Letters
|August 8, 2009
PubMed
Summary

Scientists propose a new method to detect dark matter signals. Analyzing the energy dependence of the angular power spectrum could help identify gamma rays from Galactic dark matter substructure using the Fermi Gamma-ray Space Telescope.

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Area of Science:

  • Astrophysics
  • Particle Physics
  • Cosmology

Background:

  • Dark matter annihilation in Galactic substructure creates diffuse gamma-ray emission.
  • This signal is difficult to distinguish from the extragalactic gamma-ray background.
  • The Fermi Gamma-ray Space Telescope observes gamma rays in an accessible energy range.

Purpose of the Study:

  • To develop a method for disentangling Galactic dark matter signals from background noise.
  • To identify gamma rays originating from Galactic dark matter substructure.

Main Methods:

  • Analyzing the energy dependence of the angular power spectrum of gamma-ray emissions.
  • Utilizing data from the Fermi Gamma-ray Space Telescope.

Main Results:

  • The energy dependence of the angular power spectrum can be used to identify Galactic dark matter signals.
  • A modest contribution of Galactic dark matter to the observed emission is sufficient for detection.

Conclusions:

  • The proposed method offers a promising approach to detect dark matter.
  • This technique could confirm the presence and distribution of dark matter in Galactic substructure.