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Jillian's Guide to Black Holes: Forming - Types - Outside - Inside - Finding - References - WebsitesOnly the brave and the curious continue! I shall put forth such ideas as Schwarzschild's metric for spacetime and the Schwarzschild radius equation!I'm
kidding. They're not really that bad, but I feel the need to warn you
that I'm going to actually show two equations, and I know seeing equations
frightened me when I was surfing for black hole pages. No real math
here; I just think it's important to show 'em.
What the heck does this equation mean? It's for calculating the Schwarzschild radius of an object. What does that have to do with black holes? Well, when an object is compressed below its Schwarzschild Radius, an event horizon forms around it. Sound familiar? The event horizon of a black hole is just Rs = r. If you know the mass of an object, you can calculate its Rs. For a human it is 1.5 x 10-27 meters per kilogram (for comparison a proton is 10-15 meters). Very tiny! It's tough to make black holes out of small things!
What is the Schwarzschild metric?It
is Schwarzschild's solution to Eintstein's general relativity equation
set. The metric describes the shape of spacetime outside of matter.
Y'know, those cool curvey spacetime pictures in Scientific American.
Once you hit matter, be it some gas, a star, a planet, or a rock, this
metric no longer applies. The metric's kinda ... spherical. It looks
a lot like an equation made for rectangular coordinates transformed
into spherical coordinates, a standard calculus problem.
What does all that messy stuff mean?Well,
the ds factor tells you how space changes, what it all looks like. The
dt factor tells how time changes as spacetime changes. You can see that,
if r = Rs, dt would be zero. That is to say that at the even
horizon there would be no change in time. Makes sense; you can look
at the event horizon as being the place where time "stops." The dr factor
deals with how close to something you are. You'll notice that it "blows
up" when r = Rs; the Schwarzschild metric does not apply
beyond the event horizon. The d
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