11,799 research outputs found
Mass and Mean Velocity Dispersion Relations for Supermassive Black Holes in Galactic Bulges
Growing evidence indicate supermassive black holes (SMBHs) in the mass range
of lurking in central bulges of many
galaxies. Extensive observations reveal fairly tight power laws of
versus the mean stellar velocity dispersion of the host bulge. The
dynamic evolution of a bulge and the formation of a central SMBH should be
physically linked by various observational clues. In this contribution, we
reproduce the empirical power laws based on a self-similar
general polytropic quasi-static bulge evolution and a sensible criterion of
forming a SMBH surrounding the central density singularity of a general
singular polytropic sphere (SPS) \cite{loujiang2008}. Other properties of host
bulges and central SMBHs are also examined. Based on our model, we discuss the
intrinsic scatter of the relation and a scenario for the
evolution of SMBHs in different host bulges.Comment: 8 pages, 2 figures, accepted for publication in the Proceedings of
Science for VII Microquasar Workshop: Microquasars and Beyon
QCD radiative correction to color-octet inclusive production at B Factories
In nonrelativistic Quantum Chromodynamics (NRQCD), we study the
next-to-leading order (NLO) QCD radiative correction to the color-octet
inclusive production at B Factories. Compared with the leading-order
(LO) result, the NLO QCD corrections are found to enhance the short-distance
coefficients in the color-octet production by a factor of about 1.9. Moreover, the
peak at the endpoint in the energy distribution predicted at LO can be
smeared by the NLO corrections, but the major color-octet contribution still
comes from the large energy region of . By fitting the latest data of
observed by Belle, we
find that the values of color-octet matrix elements are much smaller than
expected earlier by using the naive velocity scaling rules or extracted from
fitting experimental data with LO calculations. As the most stringent
constraint by setting the color-singlet contribution to be zero in
, we get an upper limit of the
color-octet matrix element, at NLO in .Comment: 18 pages, 8 figure
Quantum algorithm for association rules mining
Association rules mining (ARM) is one of the most important problems in
knowledge discovery and data mining. Given a transaction database that has a
large number of transactions and items, the task of ARM is to acquire
consumption habits of customers by discovering the relationships between
itemsets (sets of items). In this paper, we address ARM in the quantum settings
and propose a quantum algorithm for the key part of ARM, finding out frequent
itemsets from the candidate itemsets and acquiring their supports.
Specifically, for the case in which there are frequent -itemsets
in the candidate -itemsets (), our
algorithm can efficiently mine these frequent -itemsets and estimate their
supports by using parallel amplitude estimation and amplitude amplification
with complexity ,
where is the error for estimating the supports. Compared with the
classical counterpart, classical sampling-based algorithm, whose complexity is
, our quantum algorithm
quadratically improves the dependence on both and in the
best case when and on alone in the worst
case when .Comment: 8 page
Engineering entangled microwave photon states via multiphoton interactions between two cavity fields and a superconducting qubit
It has been shown that there are not only transverse but also longitudinal
couplings between microwave fields and a superconducting qubit with broken
inversion symmetry of the potential energy. Using multiphoton processes induced
by longitudinal coupling fields and frequency matching conditions, we design a
universal algorithm to produce arbitrary superpositions of two-mode photon
states of microwave fields in two separated transmission line resonators, which
are coupled to a superconducting qubit. Based on our algorithm, we analyze the
generation of evenly-populated states and NOON states. Compared to other
proposals with only single-photon process, we provide an efficient way to
produce entangled microwave states when the interactions between
superconducting qubits and microwave fields are in the ultrastrong regime
A General Analysis of Wtb anomalous Couplings
We investigate new physics effects on the Wtb effective couplings in a
model-independent manner. The new physics effects are summarized as four
independent couplings , , and . Using
single-top-quark productions and W-helicity fraction measurements at the LHC
and Tevatron, we perform a global fit to impose constraints on top quark
effective couplings. We introduce a set of parameters , , and
to study the correlations among Wtb effective couplings. We show that (i)
improving the measurements of and is important in
constraining the correlation of and ; (ii)
and are anti-correlated, which is sensitive to all the
experiments; (iii) and are also anti-correlated, which is
sensitive to the W-helicity measurements; (iv) the correlation between
and is sensitive to the precision of , and
measurements. The effective Wtb couplings are studied in three kinds of
new physics models: models, vector-like
quark models and Littlest Higgs model with and without T-parity. The Wtb
couplings in the left-right model and the un-unified model are sensitive to the
ratio of gauge couplings when the new heavy gauge boson's mass () is
less than several hundred GeV, but the constraint is loose if TeV.
The Wtb couplings in vector-like quark models and the Littlest Higgs models are
sensitive to the mixing angles of new heavy particles and SM particles. We also
include the constraints of the oblique T-parameter and Zbb couplings which
impose much tighter constraints on the mixing angles. We show that the Wtb
coupling constraints become relevant if the precision of single top production
cross section measurements could be reduced to 1\% relative to the SM
predictions in future.Comment: Chin. Phys. C in pres
Scheme for suppressing atom expansion induced contrast loss in atom interferometers
The loss of contrast due to atom expansion induced non-perfect Raman pulse
area in atom interferometers is investigated systematically. Based on the
theoretical simulation, we find that the expansion of the atomic cloud results
in a decrease of the {\pi} pulse fidelity and a change of the {\pi} pulse
duration, which lead to a significant reduction in fringe contrast. We propose
a mitigation strategy of increasing the intensities of the second and third
Raman pulses. Simulation results show that the fringe contrast can be improved
by 13.6% in a typical atom interferometer gravimeter using this intensity
compensation strategy. We also evaluate the effects of this mitigation strategy
in the case of a lower atomic cloud temperature and a larger Raman beam size
under different Raman pulse time interval conditions. This mitigation strategy
has potential applications in increasing the sensitivity of atom
interferometer-based precision measuring, including precision measuring of the
gravity, gravity gradient, rotation, and magnetic field gradient, as well as
testing of the Einstein equivalence principle.Comment: 14 pages, 8 figure
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