This solution is the ``corner stone'' of GR. It is very simple (at least looks like), was found almost immediately after the GR had been formulated, was used for the first (classical) experimental tests of GR and is mentioned almost in every paper concerning gravity (up to the most recent ones).
It has 4 symmetries:
| 1 translation | (
|
| 3 rotations | (keeping |
It is most conveniently written in the spherical coordinates,
(or, more correctly, ``schwarzschild coordinates'',
because time coordinate is included), in which it takes the well-known form
It is interpreted as a gravitational field produced by some spherically symmetrical
configuration of matter of total mass
.
In solving the equations this
arises as a
constant of integration. It is given the meaning of mass because in the region where
gravitational field is weak (i.e. where metric is approximately that of Minkowski
space-time) the
-component of metric is related to the Newtonian gravitational
potential and we have:
Because the Newton's gravitational law is recovered, it is not a surprise that
investigation of motion along geodesics
in Schwarzschild space-time gives the known
planetary motion in the ``0'th order''. But more than that, the next order
corrections were found to provide the missing in Newtonian mechanics
for Mercury perihelion shift (the observed shift is
per century, from which
come from
interaction with other planets in the solar system; the discrepancy was obvious,
but could not be explained for a long time) and to predict (correctly) the
bending of light by the Sun. Not bad for such a simple-looking metric!
The metric behaves badly at
,
but it is only a coordinate singularity.
Indeed, curvature tensor for this solution is such that
,
but
,
and only
.
Thus the only ``place'' where curvature becomes singular is at
.
People also explicitly found transformations to other coordinates
(e.g. to the Kruskal-Szekeres coordinates),
which make the metric manifestly non-singular at the
hypersurface.
But it should be noted, that the only way to get rid of a coordinate singularity
is to make a singular coordinate transformation.
And still this hypersurface plays very important role. It is what is now called
the ``event horizon'', because of its ``one-way-membrane'' property:
all time-like geodesics (along which material objects can move) may cross it
only once, coming from exterior (
), so that anything which passes through
it has no chance to come back to ``this world''.
Thus, this solution describes a ``black hole'': not even light (and
therefore any information) can get out from ``under the horizon''; the only
way to observe it is via some indirect gravitational effects.
And this name is also correct from a different perspective: all this ``BH physics''
is really a ``hole'' in our understanding of Nature.
It is not simple to understand physically ``interior'' of the BH (the region
in space-time, corresponding to
in Schwarzschild coordinates).
The most important
point to notice is that there
is no longer a ``coordinate time'' and
is
no longer a ``radial coordinate'' (
and
components of the metric
flip their signs which in a sense flips the meaning of t and r). The symmetries
are still present in the interior, but
-independence cannot be interpreted
as ``staticity'' and ``spherical symmetry'' is not really a spherical symmetry.
Finally, the curvature singularity at
is called a ``central singularity'',
but it is not a singularity ``at the origin'' (see [1, p.154] for
clarification of this point).