The Evolution of the BL Lacertae Objects

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Abstract
The BL Lacertae population is set apart from the rest of the active galactic nuclei by a number of peculiar features, including remarkably little signs of cosmological evolution. We focus on this feature and take a hint from the observations to reconsider the extraction of the primary energy from a Kerr hole via the Blandford-Znajek (BZ) process; in fact, we stress how this can power the emitting jets of the BL Lac objects in a regime of low accretion. We show that the timescale for the BZ process to exhaust the rotational energy of the hole spans many gigayears in all such sources. We compute scales long and uniform enough to yield an intrinsically slow population evolution, giving rise to number counts of "Euclidean" or flatter shape; even longer timescales apply to the additional, analogous process involving the inner accretion disk directly. Such slow evolution takes place in ambients and at epochs (z1) where interactions of the host galaxies with companions become rare or weak. On the other hand, at higher z, we argue that frequent interactions of the hosts within groups enhanced, each for some 10−1 Gyr, the accretion rates and the emissions from the disks, attaining power levels that are typical of the radio-loud quasars. But such interactions were also likely to disorder the large-scale magnetic field in the disk and to decrease the angular momentum of the hole, thus limiting the lifetime of all BZ emissions to under a few gigayears. Then the stronger evolution of the flat-spectrum radio-loud quasars was driven, similar to the radio-quiet ones, by the interaction rate decreasing rapidly with z.

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