9,117 research outputs found
Anatomy of decays and effects of next-to-leading order contributions in the perturbative QCD factorization approach
In this paper, we will make systematic calculations for the branching ratios
and the CP-violating asymmetries of the twenty one decays
by employing the perturbative QCD (PQCD) factorization approach. Besides the
full leading-order (LO) contributions, all currently known next-to-leading
order (NLO) contributions are taken into account. We found numerically that:
(a) the NLO contributions can provide enhancement to the LO PQCD
predictions for and , or a reduction to
\calb(\bar{B}_s^0 \to \pi^{-} K^{*+}), and we confirmed that the inclusion of
the known NLO contributions can improve significantly the agreement between the
theory and those currently available experimental measurements, (b) the total
effects on the PQCD predictions for the relevant transition form
factors after the inclusion of the NLO twist-2 and twist-3 contributions is
generally small in magnitude: less than enhancement respect to the
leading order result, (c) for the "tree" dominated decay and the "color-suppressed-tree" decay ,
the big difference between the PQCD predictions for their branching ratios are
induced by different topological structure and by interference effects among
the decay amplitude and : constructive for the
first decay but destructive for the second one, and (d) for \bar{B}_s^0 \to
V(\eta, \etar) decays, the complex pattern of the PQCD predictions for their
branching ratios can be understood by rather different topological structures
and the interference effects between the decay amplitude \cala(V\eta_q) and
\cala(V\eta_s) due to the \eta-\etar mixing.Comment: 18 pages, 2 figures, 3 tables. Some modifications of the text.
Several new references are adde
Probing the physics of newly born magnetars through observation of superluminous supernovae
The central engines of some superluminous supernovae (SLSNe) are generally
suggested to be newly born fast rotating magnetars, which spin down mainly
through magnetic dipole radiation and gravitational wave emission. We calculate
the magnetar-powered SLSNe light curves (LCs) with the tilt angle evolution of
newly born magnetars involved. We show that, depending on the internal toroidal
magnetic fields , the initial spin periods , and
the radii of direct Urca (DU) cores of newly born magnetars, as
well as the critical temperature for neutron superfluidity,
bumps could appear in the SLSNe LCs after the maximum lights when the tilt
angles grow to . The value of determines the arising time
and the relative amplitude of a bump. The quantity can affect the
arising time and the luminosity of a bump, as well as the peak luminosity of a
LC. Moreover, it is interesting that a stronger will lead to
both a brighter peak and a brighter bump in a LC. While keeping other
quantities unchanged, the bump in the LC disappears for the magnetar with
smaller . We suggest that, once the SLSNe LCs with such kinds of
bumps are observed, by fitting these LCs with our model, not only
and of newly born magnetars but also the crucial physical
quantities , , and could be
determined. Nonobservation of SLSNe LCs with such kinds of bumps hitherto may
already put some (\textit{though very rough}) constraints on , , , and . Therefore, observation of
SLSNe LCs may provide a new approach to probe the physics of newly born
magnetars.Comment: 9 pages, 4 figures, to appear in PR
Transmission resonance in a composite plasmonic structure
The design, fabrication, and optical properties of a composite plasmonic
structure, a two-dimentional array of split-ring resonators inserted into
periodic square holes of a metal film, have been reported. A new type of
transmission resonance, which makes a significant difference from the
conventional peaks, has been suggested both theoretically and experimentally.
To understand this effect, a mechanism of ring- resonance induced dipole
emission is proposed.Comment: 14 pages, 4 figure
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