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After nearly 11 years, I’ve finally decided to pull the plug on Usenet archive: Groupsrv.com.

The page you have requested no longer exists!

But don’t panic just yet!

I’ve coded this page in a way, that it’s monitoring each redirect & capturing data about the thread you’ve requested. Page you’ve requested is still available in Google’s Usenet Archive. You should be able to access it using following URL:

Event horizon / black holes and Schwarzschild metrics..

Note: I can’t guarantee that all Groupsrv.com pages can be found in Google Groups, but over 90% of the content should be there. If not, try the resources below!

Wikipedia:
Black hole! – to form a black hole The boundary of the is possible is called the event horizon . billionths of a kelvin for black holes of stellar mass
General relativity!Black holes and other compact objects notably the spherically symmetric Schwarzschild solution (used to describe a static black hole) and
Schwarzschild metric! – In Einstein ‘s theory of general relativity , the Schwarzschild metric (also known Schwarzschild black hole is called the event horizon , which is
Schwarzschild radius! – The Schwarzschild radius (sometimes historically referred to as the gravitational (Supermassive black holes up to 21 billion (2.1 × 10 10
Hawking radiation! – predicted to be released by black hole s, due to quantum effects near the event horizon . radiation than larger black holes and should

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