551 research outputs found
Black Hole Spin Properties of 130 AGN
Supermassive black holes may be described by their mass and spin. When
supermassive black holes are active, the activity provides a probe of the state
of the black hole system. The spin of a hole can be estimated when the black
hole mass and beam power of the source are known for sources with powerful
outflows. Seventy-five sources for which both the black hole mass and beam
power could be obtained are identified and used to obtain estimates of black
hole spins. The 75 supermassive black holes studied include 52 FRII radio
galaxies and 23 FRII radio loud quasars with redshifts ranging from about zero
to two. The new values are combined with those obtained previously for 19 FRII
radio galaxies, 7 FRII radio loud quasars, and 29 radio sources associated with
CD galaxies to form samples of 71 FRII radio galaxies, 30 FRII quasars, and a
total sample of 130 spin values; all of the sources are associated with massive
elliptical galaxies. The new values obtained are similar to those obtained
earlier at similar redshift, and range from about 0.1 to 1 for FRII sources.
The overall results are consistent with those obtained previously: the spins
tend to decrease with decreasing redshift for the FRII sources studied. There
is a hint that the range of values of black hole spin at a given redshift is
larger for FRII quasars than for FRII radio galaxies. There is no indication of
a strong correlation between supermassive black hole mass and spin for the
supermassive black holes studied here. The relation between beam power and
black hole mass is obtained and used as a diagnostic of the outflows and the
dependence of the magnetic field strength on black hole mass.Comment: 12 pages, 12 figures, 5 table
Proposed dynamic phase difference method for the detection of tile debonding from the space shuttle orbiter
A noncontracting, semi-global, dynamic technique was developed for detecting loose tiles on the space shuttle orbiter. In laboratory tests on a single tile, the substrate was excited into lateral motion at a constant frequency and amplitude of 2g. The phase relationship between the motions of tile and substrate was examined by noncontacting probes in order to relate the dynamic properties of the tile SIP system to its fatigue history; by a visual technique using a stroboscope and split screen video monitor for practical application in the field. When the substrate is excited at an appropriate frequency (between 30 and 60 Hz), a good tile moves in phase and a loose tile out of phase with the substrate. The out of phase motion is readily observable in the form of a "beat" between the tile and a reference marker on the substrate
The Relationship Between Beam Power and Radio Power for Classical Double Radio Sources
Beam power is a fundamental parameter that describes, in part, the state of a
supermassive black hole system. Determining the beam powers of powerful
classical double radio sources requires substantial observing time, so it would
be useful to determine the relationship between beam power and radio power so
that radio power could be used as a proxy for beam power. A sample of 31
powerful classical double radio sources with previously determined beam and
radio powers are studied; the sources have redshifts between about 0.056 and
1.8. It is found that the relationship between beam power, Lj, and radio power,
P, is well described by Log(Lj) = 0.84 Log(P) + 2.15, where both L_j and P are
in units of 10^(44) erg/s. This indicates that beam power is converted to radio
power with an efficiency of about 0.7%. The ratio of beam power to radio power
is studied as a function of redshift; there is no significant evidence for
redshift evolution of this ratio over the redshift range studied. The
relationship is consistent with empirical results obtained by Cavagnolo et al.
(2010) for radio sources in gas rich environments, which are primarily FRI
sources, and with the theoretical predictions of Willott et al. (1999).Comment: 6 pages, 2 figures, 2 tables; accepted for publication in MNRA
Resonant Excitation of Graphene K-Phonon and Intra-Landau-Level Excitons in Magneto-Optical Spectroscopy
Precise infrared magnetotransmission experiments have been performed in
magnetic fields up to 32 T on a series of multilayer epitaxial graphene
samples. We observe changes in the spectral features and broadening of the main
cyclotron transition when the incoming photon energy is in resonance with the
lowest Landau level separation and the energy of a K point optical phonon. We
have developed a theory that explains and quantitatively reproduces the
frequency and magnetic field dependence of the phenomenon as the absorption of
a photon together with the simultaneous creation of an intervalley,
intra-Landau-level exciton, and a K phonon.Comment: Main manuscript (5 pages); Supplementary Material (18 pages
Moire bands in twisted double-layer graphene
A moire pattern is formed when two copies of a periodic pattern are overlaid
with a relative twist. We address the electronic structure of a twisted
two-layer graphene system, showing that in its continuum Dirac model the moire
pattern periodicity leads to moire Bloch bands. The two layers become more
strongly coupled and the Dirac velocity crosses zero several times as the twist
angle is reduced. For a discrete set of magic angles the velocity vanishes, the
lowest moire band flattens, and the Dirac-point density-of-states and the
counterflow conductivity are strongly enhanced
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