2,884 research outputs found
Disorder effects on the quantum coherence of a many-boson system
The effects of disorders on the quantum coherence for many-bosons are studied
in a double well model. For the ground state, the disorder enhances the quantum
coherence. In the deep Mott regime, dynamical evolution reveals periodical
collapses and revivals of the quantum coherence which is robust against the
disorder. The average over variations in both the on-site energy and the
interaction reveals a beat phenomenon of the coherence-decoherence oscillation
in the temporal evolution.Comment: 4 figure
Top quark decays with flavor violation in the B-LSSM
The decays of top quark are extremely rare processes in the
standard model (SM). The predictions on the corresponding branching ratios in
the SM are too small to be detected in the future, hence any measurable signal
for the processes at the LHC is a smoking gun for new physics. In the extension
of minimal supersymmetric standard model with an additional local
gauge symmetry (B-LSSM), new gauge interaction and new flavor changing
interaction affect the theoretical evaluations on corresponding branching
ratios of those processes. In this work, we analyze those processes in the
B-LSSM, under a minimal flavor violating assumption for the soft breaking
terms. Considering the constraints from updated experimental data, the
numerical results imply ,
, and in our
chosen parameter space. Simultaneously, new gauge coupling constants
in the B-LSSM can also affect the numerical results of
.Comment: 20 pages, 4 figures, published in EPJC. arXiv admin note: substantial
text overlap with arXiv:1803.0990
Active backstepping control of combined projective synchronization among different nonlinear systems
In this article, the authors have studied combination projective synchronization using active backstepping method. The main contribution of this effort is realization of the projective
synchronization between two drive systems and one response system. We relax some limitations of previous work, where only combination complete synchronization has been investigated. According to Lyapunov stability theory and active backstepping design method, the corresponding controllers are designed to observe combination projective synchronization among three different classical chaotic systems, i.e. the Lorenz system, Rossler system and β¬ Chen system. The numerical simulation examples verify the effectiveness of the theoretical analysis. Combination projective synchronization has stronger anti-attack ability and antitranslated ability than the normal projective synchronization scheme realized by one drive and one response system in secure communication
Formation of episodic jets and associated flares from black hole accretion systems
Episodic ejections of blobs (episodic jets) are widely observed in black hole
sources and usually associated with flares. In this paper, by performing and
analyzing three dimensional general relativity magnetohydrodynamical numerical
simulations of accretion flows, we investigate their physical mechanisms. We
find that magnetic reconnection occurs in the accretion flow, likely due to the
turbulent motion and differential rotation of the accretion flow, resulting in
flares and formation of flux ropes. Flux ropes formed inside of 10-15
gravitational radii are found to mainly stay within the accretion flow, while
flux ropes formed beyond this radius are ejected outward by magnetic forces and
form the episodic jets. These results confirm the basic scenario proposed in
Yuan et al.(2009). Moreover, our simulations find that the predicted velocity
of the ejected blobs is in good consistency with observations of Sgr A*, M81,
and M87. The whole processes are found to occur quasi-periodically, with the
period being the orbital time at the radius where the flux rope is formed. The
predicted period of flares and ejections is consistent with those found from
the light curves or image of Sgr A*, M87, and PKS 1510-089. The possible
applications to protostellar accretion systems are discussed.Comment: 16 pages, 13 figures; accepted for publication in Ap
The properties of wind and jet from a super-Eddington accretion flow around a supermassive black hole
Wind and jet are important medium of AGN feedback thus it is crucial to
obtain their properties for the feedback study. In this paper we investigate
the properties of wind and jet launched from a super-Eddington accretion flow
around a supermassive black hole. For this aim, we have performed radiation
magnetohydrodynamical simulation of a magnetically arrested super-Eddington
accretion flows. We then have analyzed the simulation data by the ``virtual
particle trajectory'' approach and obtained the mass flux, poloidal and
toroidal velocities, and mass-flux-weighted momentum and energy fluxes of wind
and jet. The mass flux is found to be 2-6 times higher than that obtained based
on the time-averaged streamline method widely used in literature. Depending on
the black hole spin, the momentum flux of wind is found to be at least 2 times
larger than that of jet, while the total energy flux of jet is at most 3 times
larger than that of wind. These results are similar to the case of hot
accretion flows and imply that winds likely play a more important role than jet
in AGN feedback. The acceleration mechanism of wind and jet is analyzed and
found to be dominated by Lorentz force rather than radiation force.Comment: 13 pages, 13 figures; submitted to MNRA
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