Over the last twenty-five years, or so, there has been
considerable controversy concerning what might really happen inside
the horizon of a ``black hole,'' and also whether or not the
Cauchy horizon that (usually) lies inside there is actually a stable
piece of the geometry or would disappear [becoming changed into a
singularity (?)] in a more physical situation than the one envisioned
in the black-hole geometry, where we are ignoring all conceivable
"back-reaction" on the metric due to the "test" particles.
Recall that the (outer) horizon is a place where the rr-component
of the metric vanishes. Inside that horizon the former radial
tangent vector becomes timelike. The "Cauchy horizon" is basically
the place inside that horizon where that tangent vector again vanishes,
and then again becomes spacelike after one has passed through this
(second) horizon.
This page lists some references, sorted a very little bit by type.
The references vary from published journal articles through simply
online, electronic files. Some of the journal articles may also
be accessed online; try and see.
Click here to mail your comments and suggestions concerning the Homepage |
Click here to go to Finley's own Home Page |
Click here
to go to the Physics and Astronomy Department Home Page. |