Einstein Probe’s scientific opportunities in the field of active galactic nuclei
2018
Active galactic nuclei (AGNs) are accreting supermassive
black holes (SMBHs) that reside at the centers of galaxies and emit
excessive electromagnetic radiation, whose ultimate energy source
is the release of the gravitational potential energy of the accreted
matter in the form of thermal and radiation energy. Multi-timescale
and multi-band variability is a characteristic observational feature
of AGNs. In particular, X-ray variability is most worth noting because
of being intense and rapid, as well as carrying rich physical information
of the innermost region of the accretion disk. Therefore, AGN X-ray
variability has long been used as a probe for studying SMBHs. However,
at present, we still lack a very fundamental understanding of AGN
X-ray variability, whose origin and mechanisms remain largely unclear.
The Einstein Probe (EP) satellite has an unprecedented soft X-ray
survey capability, with a grasp (i.e., the product of detector effective
area and field of view) being one to two orders of magnitude larger
than previous similar satellites. EP is able to monitor hundreds of
bright AGNs in the whole sky with sampling intervals ranging from
100 s to years, and will thereby build an exceptional AGN variability
database. Accordingly, we propose to carry out AGN investigations
mainly in the following four aspects: comprehensive measurement of
the soft X-ray power spectral density for a large sample of bright
AGNs; systematic monitoring and study of the rare large-amplitude
AGN X-ray variability and flaring phenomenon; examination of long-term
spectral variability for a large sample of AGNs and monitoring of
their outbursts; and AGN/quasar survey. These unprecedented data will
facilitate our further understanding of many scientific questions,
such as the intense AGN X-ray variability and flaring phenomenon and
its mechanisms, the physical conditions, structures, dynamics, and
radiation processes of the AGN accretion disk, jet, and corona, as
well as the AGN cosmological evolution. Furthermore, given EP’s
capability of exploring a brand-new discovery space (large sky-area,
long-timescale, and systematic soft X-ray monitoring), we are likely
to discover some black hole accretion phenomena never seen before—the
complexity and diversity of the Universe are always beyond human imagination.
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