2,980 research outputs found
Representation of SO(3) Group by a Maximally Entangled State
A representation of the SO(3) group is mapped into a maximally entangled two
qubit state according to literatures. To show the evolution of the entangled
state, a model is set up on an maximally entangled electron pair, two electrons
of which pass independently through a rotating magnetic field. It is found that
the evolution path of the entangled state in the SO(3) sphere breaks an odd or
even number of times, corresponding to the double connectedness of the SO(3)
group. An odd number of breaks leads to an additional phase to the
entangled state, but an even number of breaks does not. A scheme to trace the
evolution of the entangled state is proposed by means of entangled photon pairs
and Kerr medium, allowing observation of the additional phase.Comment: 4 pages, 3 figure
Rapid "Turn-on" of type 1 AGN in a quiescent early type galaxy SDSS1115+0544
We present a detailed study of a transient in the center of SDSS1115+0544
based on the extensive UV, optical, mid-IR light curves (LC) and spectra over
1200 days. The host galaxy is a quiescent early type galaxy at = 0.0899
with a blackhole mass of . The transient underwent a 2.5
magnitude brightening over days, reaching a peak -band luminosity
(extinction corrected) of magnitude, then fading 0.5 magnitude over 200
days, settling into a plateau of days. Following the optical brightening
are the significant mid-IR flares at and m, with a peak time
delay of days. The mid-IR LCs are explained as the echo of UV photons
by a dust medium with a radius of cm, consistent with of 0.58 inferred from the spectra. This event is very energetic with an
extinction corrected erg s. Optical
spectra over 400 days in the plateau phase revealed newly formed broad
H emission with a FWHM of km s and narrow
coronal lines such as [Fe VII], [Ne V]. This flare also has a steeply rising UV
continuum, detected by multi-epoch data at to days post
optical peak. The broad Balmer lines and the UV continuum do not show
significant temporal variations. The slow evolving LCs over 1200 days, the
constant Balmer lines and UV continuum at late-times rule out TDE and SN IIn as
the physical model for this event. We propose that this event is a `turn-on'
AGN, transitioning from a quiescent state to a type 1 AGN with a sub-Eddington
accretion rate of /yr. This change occurred on a very short time
scale of days. The discovery of such a rapid `turn-on' AGN
poses challenges to accretion disk theories and may indicate such event is not
extremely rare.Comment: Comments are welcome. Emails to the first author. Accepted for
publication in Ap
Multifunctional in vivo vascular imaging using near-infrared II fluorescence
In vivo real-time epifluorescence imaging of mouse hindlimb vasculatures in
the second near-infrared region (NIR-II, 1.1~1.4 microns) is performed using
single-walled carbon nanotubes (SWNTs) as fluorophores. Both high spatial
resolution (~30 microns) and temporal resolution (<200 ms/frame) for small
vessel imaging are achieved 1-3 mm deep in the tissue owing to the beneficial
NIR-II optical window that affords deep anatomical penetration and low
scattering. This spatial resolution is unattainable by traditional NIR imaging
(NIR-I, 0.75~0.9 microns) or microscopic computed tomography (micro-CT), while
the temporal resolution far exceeds scanning microscopic imaging techniques.
Arterial and venous vessels are unambiguously differentiated using a dynamic
contrast-enhanced NIR-II imaging technique based on their distinct
hemodynamics. Further, the deep tissue penetration, high spatial and temporal
resolution of NIR-II imaging allow for precise quantifications of blood
velocity in both normal and ischemic femoral arteries, which are beyond the
capability of ultrasonography at lower blood velocity.Comment: 33 pages, 5 main text figures, 6 supporting figures and 2 tables;
Published online at Nature Medicine, 201
Darboux transformation for two component derivative nonlinear Schr\"odinger equation
In this paper, we consider the two component derivative nonlinear
Schr\"{o}dinger equation and present a simple Darboux transformation for it. By
iterating this Darboux transformation, we construct a compact representation
for the soliton solutions.Comment: 12 pages, 2 figure
Projected wave functions for fractionalized phases of quantum spin systems
Gutzwiller projection allows a construction of an assortment of variational
wave functions for strongly correlated systems. For quantum spin S=1/2 models,
Gutzwiller-projected wave functions have resonating-valence-bond structure and
may represent states with fractional quantum numbers for the excitations. Using
insights obtained from field-theoretical descriptions of fractionalization in
two dimensions, we construct candidate wave functions of fractionalized states
by projecting specific superconducting states. We explicitly demonstrate the
presence of topological order in these states.Comment: 10 pages, 3 figure
Fractionalization in an Easy-axis Kagome Antiferromagnet
We study an antiferromagnetic spin-1/2 model with up to third
nearest-neighbor couplings on the Kagome lattice in the easy-axis limit, and
show that its low-energy dynamics are governed by a four site XY ring exchange
Hamiltonian. Simple ``vortex pairing'' arguments suggest that the model
sustains a novel fractionalized phase, which we confirm by exactly solving a
modification of the Hamiltonian including a further four-site interaction. In
this limit, the system is a featureless ``spin liquid'', with gaps to all
excitations, in particular: deconfined S^z=1/2 bosonic ``spinons'' and Ising
vortices or ``visons''. We use an Ising duality transformation to express vison
correlators as non-local strings in terms of the spin operators, and calculate
the string correlators using the ground state wavefunction of the modified
Hamiltonian. Remarkably, this wavefunction is exactly given by a kind of
Gutzwiller projection of an XY ferromagnet. Finally, we show that the
deconfined spin liquid state persists over a finite range as the additional
four-spin interaction is reduced, and study the effect of this reduction on the
dynamics of spinons and visons.Comment: best in color but readable in B+
The emission positions of kHz QPOs and Kerr spacetime influence
Based the Alfven wave oscillation model (AWOM) and relativistic precession
model (RPM) for twin kHz QPOs, we estimate the emission positions of most
detected kHz QPOs to be at r=18+-3 km (R/15km) except Cir X-1 at r = 30\+-5 km
(R/15km). For the proposed Keplerian frequency as an upper limit to kHz QPO,
the spin effects in Kerr Spacetime are discussed, which have about a 5% (2%)
modification for that of the Schwarzchild case for the spin frequency of 1000
(400) Hz.The application to the four typical QPO sources, Cir X-1, Sco X-1, SAX
J1808.4-3658 and XTE 1807-294, is mentioned.Comment: Science China, Physics, Mechanics & Astronomy, 2010, 53, NO.
Singularly Perturbed Monotone Systems and an Application to Double Phosphorylation Cycles
The theory of monotone dynamical systems has been found very useful in the
modeling of some gene, protein, and signaling networks. In monotone systems,
every net feedback loop is positive. On the other hand, negative feedback loops
are important features of many systems, since they are required for adaptation
and precision. This paper shows that, provided that these negative loops act at
a comparatively fast time scale, the main dynamical property of (strongly)
monotone systems, convergence to steady states, is still valid. An application
is worked out to a double-phosphorylation ``futile cycle'' motif which plays a
central role in eukaryotic cell signaling.Comment: 21 pages, 3 figures, corrected typos, references remove
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