Black holes are increasingly taking center stage in modern astrophysics. Accretion onto these objects is an extremely efficient mechanism for extracting energy from mass—in principle, up to 30% of the accreting material's rest-mass energy is accessible. Largely for that reason, black holes have been implicated as the prime mover in many of the universe's most energetic phenomena, including active galactic nuclei, radio galaxies, and gamma-ray bursts. For example, an AGN, that is, an accreting black hole with a mass millions to billions of times greater than the solar mass (M ⊙) and situated at the center of its host galaxy, can have a power of 1040 W and outshine its host by a factor of thousands. AGNs and other exotic astrophysical systems provide natural laboratories for testing such fundamental physics as Lorentz invariance and general relativity. More surprising is the recent revelation that black holes seem to...
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1 August 2007
August 01 2007
Black holes and their environments Available to Purchase
Local spacetime geometry is not the only thing that black holes affect. They also profoundly influence galaxy formation and have an impact on scales as large as clusters of galaxies.
Jon M. Miller;
Jon M. Miller
1
University of Michigan
, Ann Arbor, US
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Christopher S. Reynolds
Christopher S. Reynolds
2
University of Maryland
, College Park, US
Search for other works by this author on:
Jon M. Miller
1
Christopher S. Reynolds
2
1
University of Michigan
, Ann Arbor, US
2
University of Maryland
, College Park, US
Physics Today 60 (8), 42–47 (2007);
Citation
Jon M. Miller, Christopher S. Reynolds; Black holes and their environments. Physics Today 1 August 2007; 60 (8): 42–47. https://doi.org/10.1063/1.2774097
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