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Black Holes: Physics, Structure, and Theory

1Introduction to Black Holes and Historical Context2Foundations of General Relativity3The Schwarzschild Solution4Geometry of Spacetime and Tidal Forces5Rotating Black Holes: The Kerr Metric6Black Hole Thermodynamics7Hawking Radiation and Quantum Effects8The Information Paradox9Formation and Astrophysical Evidence10Direct Imaging and Future Horizons
Formation and Astrophysical Evidence

M87* vs. Sagittarius A*

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We have imaged two distinct black holes. M87* is a giant, six-and-a-half-billion-solar-mass monster with a steady jet. Sgr A*, at our galaxy's center, is four-million-times the sun's mass but varies rapidly because its accretion flow is turbulent and clumpy.
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M87* and Sgr A*

M87*

  • Mass: ~6.5 billion solar masses
  • Location: Center of galaxy M87
  • Environment: Steady, bright jet
  • Variability: Slow (weeks/months)

Sgr A*

  • Mass: ~4 million solar masses
  • Location: Center of Milky Way
  • Environment: Fainter, variable accretion
  • Variability: Fast (minutes/hours)
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