Accreting Black Holes and Neutron Stars
On the most efficient and energetic power plants in the Universe
I am involved in studying the probably most extreme
objects: black holes and neutron stars that attract matter
from their surroundings. The complexity and extent of this
field requires us to collaborate amongst different
research institutes and to connect different
astrophysical disciplines in a
strongly interdisciplinary manner. My research has
been funded by all sub-divisions of
the "Netherlands
Research School for Astronomy" (NOVA) and
the DLR. The
bottom part of this page is rather technical. Here, I want
to bridge to the general public and let everyone access the
fascinating science we are pushing forward. With these
information on hand, it will be easier to understand the
condensed information presented further below.
Black holes and neutron stars gather a lot of mass at
very little space. Both can result from the
collapse of a massive star at the end of its
lifetime. During such a collapse, several processes that
would keep matter in shape are overcome and a super-dense
configuration of matter is formed. Neutron stars can be
said to be the last stable (and most dense) configuration of
matter known. They are about as massive as our sun but
measure only tens of kilometers in diameter. In other cases,
massive stars collapse all the way to black holes.
In black holes, the entire mass is found in one
"singularity". The "size" of a black hole is pure
definition and not the size of any structure - it is the
(gravitational) radius at which nothing, not even light can
escape the steep trough of space-time formed by the
super-dense black hole. We call both neutron stars and black
holes "compact objects".
When we neglect time, an analogy of space is a
stretched sheet. Now, let's compare two objects of the same
mass: a heavy marble (the black hole) and porous Dutch bread
(our sun). The marble will curve the sheet deeper than the
bread. Still, both will curve the sheet the same way towards
its outer edge. A lighter marble thrown onto the sheet will
therefore draw circles the same way around both central
objects. Curvature of space is exactly what causes
gravitational attraction. Likewise, Earth will orbit our sun
the same way it would orbit a black hole of the same
mass. The story changes only when an observer approaches the
black hole very closely and experiences the localized and
much deeper (and steeper) curvature of space-time (our sheet
plus time as fourth dimension). Black holes therefore only
have a very small area of influence. Here, all the
fascinating effects come to play. Light, for example, has to
follow space-time just as a marble on a curved sheet. Close
to a black hole, light from your flashlight may come back to
you and you may also see yourself from behind. But be aware
of the extreme tidal forces that will stretch everything
like a spaghetti. The steeper the sheet (or space) is
curved, the stronger the tidal force.
Only the environment of black holes (and neutron stars)
makes them the most efficient and energetic power plants
in the universe. Everything that formed anywhere in the
Universe has angular momentum and follows trajectories
around a center of mass. If there is matter close to a black
hole with angular momentum, it will thus spiral around the
heavy central mass just like planets around their central
star(s). This is true for black holes at all sizes and
masses. Matter around the largest black holes of millions to
billions of solar masses forms the centers of huge galaxies
like our Milky Way. Matter around stellar-sized black holes
may have originated from gas remaining after the explosion
of the foregoing massive star.
Very close to the black hole, gas is assumed to be very
dense. Friction can lead to an outward transport of angular
momentum and therefore the formation of a disk. This disk can
continuously feed the inner object with mass. Einstein's
famous equation predicts that this mass is proportional to
energy. During the "accretion of matter", this
gravitational energy is released via radiation across
the electromagnetic spectrum and strong outflows of
matter. The efficiency at which radiation is produced
exceeds nuclear fusion by a factor of more than 14 and we
can certainly call it the most efficient process to produce
energy across the Universe. On Earth, however, we have
limited possibilities to squeeze the energy contained in
pure mass. For example, we burn it (one of our biggest
problems), throw it somewhere, try to extract the kinetic
energy carried by winds, or let reactions do their
thing.
Accretion onto compact objects is an ubiquitous
process in the Universe at all mass scales. It is a
process of gradual in-spiral and not the consequence of
black holes sucking in their environment in
free-fall. Galaxies, where their central black hole happens
to accrete matter and thus releases heaps of energy, are
called "Active Galaxies". Our Milky Way is not an Active
Galaxy. Note that, on smaller scales, neutron stars can also
attract matter from their surroundings. For them, this
process can not last forever. After accumulating a certain
mass, an explosion is triggered that may lead to the
formation of a black hole. Black holes, however,
can merge and accrete matter over cosmological time
scales and reach extreme masses. Merging black holes
(and neutron stars) were just recently found by detecting
gravitational wave signals from these mergers with Earth
itself as detector material.
My research focuses on a better understanding of
compact objects as cosmic power plants. To do so, me and my
colleagues try to picture the invisible. The size of a
supermassive black hole inside a distant galaxy is
comparable to the size of a bacterium on the moon, which is
much smaller than the best telescope could resolve. We
therefore use some tricks. We study all forms of the
released energy to infer the energizing processes very
close to the black hole. We observe the light being
emitted from these systems from the lowest to the highest
energies (from the radio to the gamma-rays). The energy
dependency of the light encodes valuable information on the
processes we try to understand. Matter that is thrown out
of these systems (the "exhaust"), however, can be observed
and imaged in many cases. The most extreme of these outflows
are "jets". They emerge from the centers of Active
Galaxies and the environment of stellar-sized black holes
inside galaxies. Jets are remaining focused at extremely
large distances. They accelerate matter to nearly the speed
of light, which also produces radiation. We can for example
observe their strong radio light with large radio antennas
on Earth.