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:
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!
Schwarzschild metric! – called the event horizon, which is situated at the Schwarzschild radius, often called the radius of a black hole. Any non-rotating and non-charged mass
Schwarzschild radius! – hence the name "black hole". Black holes can be classified based on their Schwarzschild radius, or equivalently, by their density. Black holes with very high
Black hole! – form a black hole. The boundary of the region from which no escape is possible is called the event horizon. Although crossing the event horizon has enormous
General relativity! – gravitational collapse, and the objects known today as black holes. In the same year, the first steps towards generalizing Schwarzschild‘s solution to electrically
De Sitter–Schwarzschild metric! – black hole event horizons and also cosmological horizons. The de Sitter–Schwarzschild solution is the simplest solution which has both. The metric of