![]() |
First photo of a black hole |
Einstein’s general theory of relativity allows for the existence of objects with infinite density (singularities). There are two types:
1.
Black holes,
accumulations of matter in a null volume, either at the center of a galaxy, or
as the result of a supernova explosion.
2.
The universe, at its initial moment (the Big
Bang).
A star like the sun is in equilibrium because the gravitational attraction, which tends to make it contract, is equal to the expansion caused by the nuclear reactions taking place inside the star. When a star much larger than the sun exhausts its nuclear fuel (first hydrogen, then helium, then other elements), as there are no longer nuclear reactions to stop the contraction, the star implodes. When the implosion rebounds, the star throws large quantities of matter into space: a supernova explosion, which for some time makes the star brighter than a whole galaxy. But there is always a remainder of matter, which gives rise to a new type of object.
If the mass of the remainder of the star is within
certain limits, the implosion stops because the strong nuclear interaction
causes a repulsion between the elementary particles (neutrons) that ultimately
make up the star. The result is a neutron
star, a pulsar. But if the mass of the remainder is even greater
(more than 3 or 4 times greater than the mass of the sun), the attraction of
gravity would overcome the strong nuclear interaction, the implosion cannot be
stopped, and the result is a black
hole, a singularity, with all the mass of the remainder of the star
concentrated in a null volume. Therefore, although its mass is always finite,
the density (mass/volume) would be infinite.
![]() |
Karl Schwarzchild |
At a certain distance from the center of a black
hole (the Schwarzschild radius) the escape velocity (the speed that a body must to
escape the attraction of a gravitational mass) is equal to the speed of light.
Since neither matter nor energy can move faster, that means that anything
closer than that distance to the center of the black hole cannot escape from
it. Not even light can escape from the inside of a black hole. That is
precisely why John Wheeler proposed the name black hole for these objects in 1967, which was reportedly
suggested to him by one of his students. The spherical surface whose center is
the center of the black hole and whose radius is the Schwarzschild radius is
called the event horizon
of the black hole.
We know that physicists always try to avoid
infinities whenever they appear in their equations. Einstein, for example, was
against the idea that black holes (they were not called that at the time, but Schwarzschild
singularities)
have infinite density. Various theories have subsequently been proposed, some
indistinguishable from general relativity under normal conditions, to try to
eliminate singularities. I talked about one of them in another
post.
![]() |
Roger Penrose |
One of the ways to try and solve the infinite
density problem was by trying to find solutions to Einstein’s equations under
conditions that would not lead to singularities; for example, by making the
black hole rotate, or have an electric charge, or by trying to show that under
the most general possible conditions the singularity would not appear. But in
the late 1960s, Roger Penrose and Stephen Hawking showed that singularities do
appear, whatever the initial conditions. In turn, their theorems proved that
Einstein’s equation leads without any possible escape to the fact that the
universe began at the Big
Bang. In 2020,
Penrose received the Nobel Prize in physics for this reason (Hawking had
already died).
Is there a way to escape infinite density? Yes. We
know (I have said it several times in these posts) that general relativity can
only be applied since 5×10-44 seconds after the Big Bang. Before that time (the Planck time) the universe was so small that the other great
physical theory, quantum theory, must also be applied. This theory is usually
applied to very small objects. The problem is that we do not have a theory of quantum gravity, which combines general relativity with quantum
theory. There have been several attempts to construct such a theory, but so far
no one has succeeded. Until we have it, we do not know what could have happened
in the first fraction of a second after the Big Bang, and we also do not know what exactly happens at
the center of a black hole, where the same theory would have to be applied.
Meanwhile, some say that it is not true that black
holes have infinite density. What they do is divide the mass inside the black
hole (remember that mass is always finite) by the volume of the sphere
contained inside the event horizon, the radius of which is the distance to the
center of the black hole from the point where the escape velocity equals the
speed of light: the distance at which not even light can escape from the black
hole. That volume is never infinite either. The quotient of a finite number between another
finite number different from zero is always finite. Consequently, they claim that the gigantic supermassive black holes
at the center of galaxies have a density lower than that of water. But this is
cheating, because it assumes that the density inside the black hole is
constant, which no theory allows us to assert. We should not confuse the
average density of the sphere contained inside the event horizon with the
density of the compressed matter inside the black hole. For now, we cannot
avoid the possibility that this matter occupies a volume equal to zero, as
predicted by Einstein’s equations.
Thematic Thread about Standard Cosmology: Previous Next
Manuel Alfonseca
No comments:
Post a Comment