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Lect22
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... at the corners of a square of side L. The total potential energy of the masses is equal to –xGM2/L, where x equals ...
Black holes and the Structure of Space-Time
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... of stellar cores of GRB progenitors. This is problematic for solitary stars: • Evolutionary models of solitary massive stars show that even much weaker magnetic fields (Taylor-Spruit dynamo) result in too slow rotation – no collapsar disk (Heger et al. 2005) • Low metalicity may save the collapsar m ...
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... evidence of another planet near the Sun, which they named Vulcan. However, Vulcan didn’t exist. Einstein’s equations were able account for this. This was general relativity’s first success. i) Why hasn’t the precession been seen for the other planets? The relativistic precessions for Venus and Earth ...
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... as it moves away from a massive body. That is, it loses some energy as the gravitational field does work on it. This means that l must change. Since E goes down l gets bigger. • We have a RED shift! ...
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3x+6y=16 x+3y=5 - cloudfront.net
3x+6y=16 x+3y=5 - cloudfront.net

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Kerr metric

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