Page 52 - A Brief History of Time - Stephen Hawking

A Brief History of Time - Stephen Hawking... Chapter 6
have some evidence that there is a much larger black hole, with a mass of about a hundred thousand times that of the
sun, at the center of our galaxy. Stars in the galaxy that come too near this black hole will be torn apart by the
difference in the gravitational forces on their near and far sides. Their remains and gas that is thrown off other stars, will
fall toward the black hole. As in the case of Cygnus X-l, the gas will spiral inward and will heat up, though not as much
as in that case. It will not get hot enough to emit X rays, but it could account for the very compact source of radio waves
and infrared rays that is observed at the galactic center.

It is thought that similar but even larger black holes, with masses of about a hundred million times the mass of the sun,
occur at the centers of quasars. For example, observations with the Hubble telescope of the galaxy known as M87
reveal that it contains a disk of gas 130 light-years across rotating about a central object two thousand million times the
mass of the sun. This can only be a black hole. Matter falling into such a supermassive black hole would provide the
only source of power great enough to explain the enormous amounts of energy that these objects are emitting. As the
matter spirals into the black hole, it would make the black hole rotate in the same direction, causing it to develop a
magnetic field rather like that of the earth. Very high-energy particles would be generated near the black hole by the
in-falling matter. The magnetic field would be so strong that it could focus these particles into jets ejected outward along
the axis of rotation of the black hole, that is, in the directions of its north and south poles. Such jets are indeed observed
in a number of galaxies and quasars. One can also consider the possibility that there might be black holes with masses
much less than that of the sun. Such black holes could not be formed by gravitational collapse, because their masses
are below the Chandrasekhar mass limit: stars of this low mass can support themselves against the force of gravity
even when they have exhausted their nuclear fuel. Low-mass black holes could form only if matter was compressed to
enormous densities by very large external pressures. Such conditions could occur in a very big hydrogen bomb: the
physicist John Wheeler once calculated that if one took all the heavy water in all the oceans of the world, one could
build a hydrogen bomb that would compress matter at the center so much that a black hole would be created. (Of
course, there would be no one left to observe it!) A more practical possibility is that such low-mass black holes might
have been formed in the high temperatures and pressures of the very early universe. Black holes would have been
formed only if the early universe had not been perfectly smooth and uniform, because only a small region that was
denser than average could be compressed in this way to form a black hole. But we know that there must have been
some irregularities, because otherwise the matter in the universe would still be perfectly uniformly distributed at the
present epoch, instead of being clumped together in stars and galaxies.

Whether the irregularities required to account for stars and galaxies would have led to the formation of a significant
number of “primordial” black holes clearly depends on the details of the conditions in the early universe. So if we could
determine how many primordial black holes there are now, we would learn a lot about the very early stages of the
universe. Primordial black holes with masses more than a thousand million tons (the mass of a large mountain) could
be detected only by their gravitational influence on other, visible matter or on the expansion of the universe. However,
as we shall learn in the next chapter, black holes are not really black after all: they glow like a hot body, and the smaller
they are, the more they glow. So, paradoxically, smaller black holes might actually turn out to be easier to detect than
large ones!

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