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Extragalactic Astronomy and Cosmology: An Introduction

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5. Active Galactic Nuclei<br />

186<br />

change substantially over the lifetime of the source,<br />

a total energy can be estimated from the luminosity<br />

<strong>and</strong> the minimum age,<br />

E 10 47 erg/s × 10 7 yr ∼ 3 × 10 61 erg , (5.8)<br />

however, the assumption of an essentially constant<br />

luminosity is not necessarily justified.<br />

• The luminosity of some AGNs varies by more than<br />

50% on time-scales of a day. From this variability<br />

time-scale, an upper limit for the spatial extent of<br />

the source can be determined, because the source<br />

luminosity can change substantially only on such<br />

time-scales where the source as a whole, or at least<br />

a major part of the emitting region, is in causal contact.<br />

Otherwise “one end” of the source does not<br />

know that the “other end” is about to vary. This<br />

yields a characteristic extent of the central source<br />

of R 1 lightday ∼ 3 × 10 15 cm.<br />

5.3.1 Why a Black Hole?<br />

We will now combine the aforementioned observations<br />

<strong>and</strong> derive from them that the basic energy production<br />

in AGNs has to be of a gravitational nature. To do this,<br />

we note that the most efficient “classical” method of energy<br />

production is nuclear fusion, as is taking place in<br />

stars. We will therefore make the provisional assumption<br />

(which will soon lead to a contradiction) that the<br />

energy production in AGNs is based on thermonuclear<br />

processes.<br />

By burning hydrogen into iron – the nucleus with the<br />

highest binding energy per nucleon – 8 MeV/nucleon<br />

are released, or 0.008 m p c 2 per nucleon. The maximum<br />

efficiency of nuclear fusion is therefore ɛ 0.8%,<br />

where ɛ is defined as the mass fraction of “fuel” that is<br />

converted into energy, according to<br />

E = ɛ mc 2 . (5.9)<br />

To generate the energy of E = 3 × 10 61 erg by nuclear<br />

fusion, a total mass m of fuel would be needed, where<br />

m is given by<br />

m = E<br />

ɛc ∼ 4 × 2 1042 g ∼ 2 × 10 9 M ⊙ , (5.10)<br />

where we used the energy estimate from (5.8). If the<br />

energy of an AGN was produced by nuclear fusion,<br />

burnt-out matter of mass m [more precisely, (1 − ɛ)m]<br />

must be present in the core of the AGN.<br />

However, the Schwarzschild radius of this mass is<br />

(see Sect. 3.5.1)<br />

r S = 2Gm<br />

c 2<br />

= 2GM ⊙<br />

c 2<br />

m<br />

M ⊙<br />

= 3 × 10 5 cm m M ⊙<br />

∼ 6 × 10 14 cm ,<br />

i.e., the Schwarzschild radius of the “nuclear cinder” is<br />

of the same order of magnitude as the above estimate of<br />

the extent of the central source. This argument demonstrates<br />

that gravitational effects must play a crucial role –<br />

the assumption of thermonuclear energy generation has<br />

been disproven because its efficiency ɛ is too low. The<br />

only known mechanism yielding larger ɛ is gravitational<br />

energy production.<br />

Through the infall of matter onto a central black hole,<br />

potential energy is converted into kinetic energy. If it is<br />

possible to convert part of this inward-directed kinetic<br />

energy into internal energy (heat) <strong>and</strong> subsequently emit<br />

this in the form of radiation, ɛ can be larger than that of<br />

thermonuclear processes. From the theory of accretion<br />

onto black holes, a maximum efficiency of ɛ ∼ 6% for<br />

accretion onto a non-rotating black hole (also called<br />

a Schwarzschild hole) is derived. A black hole with<br />

the maximum allowed angular momentum can have an<br />

efficiency of ɛ ∼ 29%.<br />

5.3.2 Accretion<br />

Due to its broad astrophysical relevance beyond the<br />

context of AGNs, we will consider the accretion process<br />

in somewhat more detail.<br />

The Principle of Accretion. Gas falling onto a compact<br />

object loses its potential energy, which is first converted<br />

into kinetic energy. If the infall is not prevented, the gas<br />

will fall into the black hole without being able to radiate<br />

this energy. In general one can expect that the gas has<br />

finite angular momentum. Thus it cannot fall straight<br />

onto the compact object, since this is prevented by the<br />

angular momentum barrier. Through friction with other<br />

gas particles <strong>and</strong> by the resulting momentum transfer,<br />

the gas will assemble in a disk oriented perpendicular to<br />

the direction of the angular momentum vector. The frictional<br />

forces in the gas are expected to be much smaller

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