1,640 research outputs found
Practical decoy-state measurement-device-independent quantum key distribution
Measurement-device-independent quantum key distribution (MDI-QKD) is immune
to all the detection attacks; thus when it is combined with the decoy-state
method, the final key is unconditionally secure, even if a practical weak
coherent source is used by Alice and Bob. However, until now, the analysis of
decoy-state MDI-QKD with a weak coherent source is incomplete. In this paper,
we derive, with only vacuum+weak decoy state, some tight formulas to estimate
the lower bound of yield and the upper bound of error rate for the fraction of
signals in which both Alice and Bob send a single-photon pulse to the untrusted
third party Charlie. The numerical simulations show that our method with only
vacuum+weak decoy state can asymptotically approach the theoretical limit of
the infinite number of decoy states. Furthermore, the statistical fluctuation
due to the finite length of date is also considered based on the standard
statistical analysis.Comment: 5 pages, 3 figure
Unbiased Correction Relations for Galaxy Cluster properties Derived from Chandra and XMM-Newton
We use a sample of 62 clusters of galaxies to investigate the discrepancies
of gas temperature and total mass within r500 between XMM-Newton and Chandra
data. Comparisons of the properties show that: (1) Both the de-projected and
projected temperatures determined by Chandra are higher than those of
XMM-Newton and there is a good linear relation for the de-projected
temperature. (2) The Chandra mass is much higher than XMM-Newton mass with a
bias of 0.15. To explore the reasons for the discrepancy in mass, we
recalculate the Chandra mass (expressed as M_c) by modifying its temperature
with the de-projected temperature relation. The results show that M_c is more
close to the XMM-Newton mass with the bias reducing to 0.02. Moreover, M_c are
corrected with the r500 measured by XMM-Newton and the intrinsic scatter is
significantly improved with the value reducing from 0.20 to 0.12. These mean
that the temperature bias may be the main factor causing the mass bias. At
last, we find that M_c is consistent with the corresponding XMM-Newton mass
derived directly from our mass relation at a given Chandra mass. Thus, the
de-projected temperature and mass relations can provide unbiased corrections
for galaxy cluster properties derived from Chandra and XMM-Newton.Comment: accepted for publication in Ap
Exploring behaviors of partonic matter forming in early stage of and nucleus-nucleus collisions at ultra-relativistic energies
The parton yield, (pseudo)rapidity distribution, and transverse momentum
distribution in partonic matter assumed forming in the early stage of and
nucleus-nucleus collisions at RHIC energy (=200 GeV) and LHC
energy (=5.5 TeV for nucleus-nucleus, 5.5 and/or 14 TeV for
) are comparatively investigated with parton and hadron cascade model
PACIAE. It turned out that the different parton and anti-parton spectra
approach to be similar with reaction energy increasing from RHIC to LHC. We
have argued that if the partonic matter forming in Au+Au collisions at RHIC
energy is strongly interacting quark-gluon plasma, the one forming in Pb+Pb
collisions at LHC energy might approach the real (free) quark-gluon plasma.Comment: 6 pages, 6 figure
Centrality dependence of forward-backward multiplicity correlation in Au+Au collisions at =200 GeV
We have studied the centrality dependence of charged particle
forward-backward multiplicity correlation strength in Au+Au collisions at
=200 GeV with a parton and hadron cascade model, PACIAE, based
on PYTHIA. The calculated results are compared with the STAR data. The
experimentally observed correlation strength characters: (1) the approximately
flat pseudorapidity dependence in central collisions and (2) the monotonous
decrease with decreasing centrality are well reproduced. However the
theoretical results are bigger than the STAR data for the peripheral
collisions. A discussion is given for the comparison among the different models
and STAR data.Comment: 5pages,4figure
A classical postselected weak amplification scheme via thermal light cross-Kerr effect
In common sense, postselected weak amplification must be related to
destructive interference effect of the meter system, and a single photon exerts
no effect on thermal field via cross-phasemodulation (XPM) interaction. In this
Letter we present, for the first time, a thermal light cross-Kerr effect.
Through analysis, we reveal two unexpected results: i) postselection and weak
amplification can be explained at a classical level without destructive
interference, and ii) weak amplification and weak value are not one thing.
After postselection a new mixed light can be generated which is nonclassical.
This scheme can be realized via electromagnetically-induced transparency.Comment: Comments are welcome. 6 pages, 11 figure
Complete deterministic multi-electron Greenberger-Horne-Zeilinger state analyzer for quantum communication
We present a scheme for the multi-electron Greenberger-Horne-Zeilinger (GHZ)
state analyzer, resorting to an interface between the polarization of a probe
photon and the spin of an electron in a quantum dot embedded in a microcavity.
All the multi-spin GHZ states can be completely discriminated by using
single-photon detectors and linear optical elements. Our scheme has some
features. First, it is a complete GHZ-state analyzer for multi-electron spin
systems. Second, the initial entangled states remain after being identified and
they can be used for a successive task. Third, the electron qubits are static
and the photons play a role of a medium for information transfer, which has a
good application in quantum repeater in which the electron qubits are used to
store the information and the photon qubits are used to transfer the
information between others.Comment: 6 page, 3 figures, 1 tabl
A good mass proxy for galaxy clusters with XMM-Newton
We use a sample of 39 galaxy clusters at redshift z < 0.1 observed by
XMM-Newton to investigate the relations between X-ray observables and total
mass. Based on central cooling time and central temperature drop, the clusters
in this sample are divided into two groups: 25 cool core clusters and 14
non-cool core clusters, respectively. We study the scaling relations of
Lbol-M500, M500-T, M500-Mg and M500-YX, and also the influences of cool core on
these relations. The results show that the M500-YX relation has a slope close
to the standard self-similar value, has the smallest scatter and does not vary
with the cluster sample. Moreover, the M500-YX relation is not affected by the
cool core. Thus, the parameter of YX may be the best mass indicator.Comment: ApJ Accepted, 25 pages, 7 figure
Hacking on decoy-state quantum key distribution system with partial phase randomization
Quantum key distribution (QKD) provides means for unconditional secure key
transmission between two distant parties. However, in practical
implementations, it suffers from quantum hacking due to device imperfections.
Here we propose a hybrid measurement attack, with only linear optics, homodyne
detection, and single photon detection, to the widely used vacuum+weak decoy
state QKD system when the phase of source is partially randomized. Our analysis
shows that, in some parameter regimes, the proposed attack would result in an
entanglement breaking channel but still be able to trick the legitimate users
to believe they have transmitted secure keys. That is, the eavesdropper is able
to steal all the key information without discovered by the users. Thus, our
proposal reveals that partial phase randomization is not sufficient to
guarantee the security of phase-encoding QKD systems with weak coherent states.Comment: 12 pages,4 figure
The scaling relation and its difference between cool-core and non-cool-core clusters
We construct a sample of 70 clusters using data from XMM-Newton and Planck to
investigate the scaling relation and the
cool-core influences on the relation. is calculated by
accurate de-projected temperature and electron number density profiles derived
from XMM-Newton. is the latest Planck data restricted to
our precise X-ray size . To study the cool-core influences
on scaling relation, we apply two criteria,
limits of central cooling time and classic mass deposition rate, to distinguish
cool-core clusters (CCCs) from non-cool-core clusters (NCCCs). We also use
from other papers, which are derived from different
methods, to confirm our results.
The intercept and slope of the scaling
relation are , . The intrinsic scatter is
. The ratio of \mbox{} is , which is perfectly agreed with unity.
Discrepancies of scaling relation between
CCCs and NCCCs are found in observation. They are independent of cool-core
classification criteria and calculation methods, although
discrepancies are more significant under the classification criteria of classic
mass deposition rate. The intrinsic scatter of CCCs (0.04) is quite small
compared to that of NCCCs (0.27). The ratio of for CCCs is , suggesting that CCCs' may
overestimate SZ signal. By contrast, the ratio of for NCCCs is , which indicates that NCCCs' may underestimate SZ signal.Comment: 16 pages, 5 figures, accepted by RA
Study on possible molecular states composed of () and () within the Bethe-Salpeter framework
observed by the LHCb collaboration is confirmed as a pentaquark
and its structure, production, and decay behaviors attract great attention from
theorists and experimentalists. Since its mass is very close to sum of
and masses, it is naturally tempted to be considered as a
molecular state composed of and . Moreover, is
observed in the channel with final state, requiring that isospin
conservation is an isospin-1/2 eigenstate. In literature, several
groups used various models to estimate its spectrum. We systematically study
the pentaquarks within the framework of the Bethe-Salpeter equation; thus
is an excellent target because of the available data. We calculate
the spectrum of in terms of the Bethe-Salpter equations and further
study its decay modes. Some predictions on other possible pentaquark states
that can be tested in future experiments are made.Comment: 24 pages, 3 firures, accepted by PR
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