What are Black Holes?
An object sits in space minding its own business. A rocket is fired from its
surface. What happens?
To escape from the surface of the object, the rocket must overcome
the pull of gravity.
The faster the rocket is propelled upward, the higher up it
will travel before it falls back to the object. There is a
critical speed beyond which the rocket will just escape the gravitational pull
of the object and escape to freedom.
This critical speed is known as the
escape speed = [2GM/R]1/2
(which is a measure of how strong gravity is at the surface of the object). Some examples
of escape speeds:
OBJECT | Escape Speed (km/s) |
Moon | 2 km/s |
Earth | 11.2 km/s |
Jupiter | 60 km/s |
Sun | 620 km/s |
White Dwarf | 6,900 km/s |
Neutron Star | 200,000 km/s |
Black Hole | c |
A black hole is an object from which the escape speed is
equal to c, the speed
of light. Consequently, light cannot escape from the object (and the object
appears black!)
Because the speed of light is the maximum speed at which
anything can travel through the Universe, this also
means that nothing can travel
fast enough to escape from a black hole.
i
Event Horizon
Question: What is the surface of a black hole?
According to Newton and Einstein, the strength of gravity
around an object doesn't depend upon how the material
is arranged inside of the object as long as the
distribution is
spherically symmetric. This means that the mass of the star
could, for example, either
be spread evenly thoughout the star's interior
or concentrated at the very
center of the star; we wouldn'be able to tell from the outside.
Question: How is the material distributed in a black hole?
It turns out that all of the mass of a black hole resides at
its very center (in a mathematical point); this point is referred
to as a singularity.
Note that a mathematical point has
no length, height, or width and thus has zero volume. So, if I cram
all the mass of the star into the singularity ===> the density of
material at the singularity is infinite. (This can lead to
interesting effects.)
Anyway, back to the surface of the black
hole. So what is meant by surface of a black hole?
Because all of the mass is contained in the singularity, we
define the surface of the black hole to be
the radius from which the escape speed is equal to
the speed of light,
c (recall the expression for the escape speed).
This surface is a natural
boundary; it separates our Universe into two parts:
- an inside part cut-off from the outside world in the sense
that an observer in the inside can only receive information from
the outside world; there is no way for an
observer on the inside
to send a message to someone on the outside.
- an observer on the outside can only send information to an
observer on the inside; the outside observer cannot
hope to get a response in return.
The imaginary surface that separates the Universe
into these regions is called the
Event Horizon.
The radius of the event horizon of a non-rotating black hole is
Rs =
3 x [M/MSun)] km .
Rs is referred to as the Schwarzschild Radius in honor of Karl
Schwarzschild, the first person to work out the theory of a non-rotating
black hole.
The Sun would have to shrink to
a radius of 3 km in
order to become a black hole. A 10 MSun
black hole would have a
radius of 3 x [10MSun/MSun]
km = 3 x [10] km = 30
km.
Question: What kinds of things can happen near the Event Horizon?
If a clock is dropped from infinity toward a black hole, the observer who
dropped the clock would see:
Interestingly, if an astronaut tagged along with the clock on its journey, the
astronaut would not
feel anything unusual about the trip (other than the
strong tidal forces). The astronaut simply falls toward the black hole,
pass through the event horizon, and then flow into the singularity. The
astronaut, however, sees interesting things. The black hole acts like a
lens leading to
several
effects.
Some Properties of Black Holes
- Cosmic Censorship
Nature always cloaks singularities with event horizons.
So, no matter what strange physics may occur near singularities, it
cannot reach back into our Universe.
- Black Holes Have No Hair
Black Holes are characterized by only their mass, spin, and
electrical charge. This is odd, as it says that it doesn't
matter if we make black holes out of elephants or gnats or old
socks, it is only the mass, charge, and spin that are
important. If I throw neutral material into a black hole, I do
not know if I threw in electron-positron pairs,
proton-anti-proton pairs, neutrons, neutrinos, ... . That is, we
lose information about our Universe as it passes into a black hole.
[Comment--if this information manages to sneak out into some other
universe
through some quirk, then the other universe would notice things
that occurred randomly and without warning (the notion of
cause
and effect breaks down). This is bad.]