2,099 research outputs found
Triangle singularity in the decays
We study the reaction and
find that the mechanism to produce this decay develops a triangle singularity
around ~MeV. The differential width
shows a rapid growth around the
invariant mass being 1515~MeV as a consequence of the triangle singularity of
this mechanism, which is directly tied to the nature of the and
as dynamically generated resonances from the interaction of
pseudoscalar mesons. The branching ratios obtained for the decays are of the order of , accessible in
present facilities, and we argue that their observation should provide relevant
information concerning the nature of the low-lying scalar mesons.Comment: 12 pages, 8 figures, published in EPJ
MixFairFace: Towards Ultimate Fairness via MixFair Adapter in Face Recognition
Although significant progress has been made in face recognition, demographic
bias still exists in face recognition systems. For instance, it usually happens
that the face recognition performance for a certain demographic group is lower
than the others. In this paper, we propose MixFairFace framework to improve the
fairness in face recognition models. First of all, we argue that the commonly
used attribute-based fairness metric is not appropriate for face recognition. A
face recognition system can only be considered fair while every person has a
close performance. Hence, we propose a new evaluation protocol to fairly
evaluate the fairness performance of different approaches. Different from
previous approaches that require sensitive attribute labels such as race and
gender for reducing the demographic bias, we aim at addressing the identity
bias in face representation, i.e., the performance inconsistency between
different identities, without the need for sensitive attribute labels. To this
end, we propose MixFair Adapter to determine and reduce the identity bias of
training samples. Our extensive experiments demonstrate that our MixFairFace
approach achieves state-of-the-art fairness performance on all benchmark
datasets.Comment: Accepted in AAAI-23; Code: https://github.com/fuenwang/MixFairFac
Signatures of the two poles in decay
We analyze theoretically the and decays to see the feasibility to check the double pole nature of
the axial-vector resonance predicted by the unitary extensions of
chiral perturbation theory (UChPT). Indeed, within UChPT the is
dynamically generated from the interaction of a vector and a pseudoscalar
meson, and two poles are obtained for the quantum numbers of this resonance.
The lower mass pole couples dominantly to and the higher mass pole to
, therefore we can expect that different reactions weighing differently
these channels in the production mechanisms enhance one or the other pole. We
show that the different final channels in weigh
differently both poles, and this is reflected in the shape of the final
vector-pseudoscalar invariant mass distributions. Therefore, we conclude that
these decays are suitable to distinguish experimentally the predicted double
pole of the resonance.Comment: 7 pages, 3 figure
A Comprehensive Analysis of Fermi Gamma-Ray Burst Data. IV. Spectral Lag and its Relation to E p Evolution
The spectral evolution and spectral lag behavior of 92 bright pulses from 84 gamma-ray bursts observed by the Fermi Gamma-ray Burst Monitor (GBM) telescope are studied. These pulses can be classified into hard-to-soft pulses (H2S; 64/92), H2S-dominated-tracking pulses (21/92), and other tracking pulses (7/92). We focus on the relationship between spectral evolution and spectral lags of H2S and H2S-dominated-tracking pulses. The main trend of spectral evolution (lag behavior) is estimated with ( ), where E p is the peak photon energy in the radiation spectrum, t + t 0 is the observer time relative to the beginning of pulse −t 0, and is the spectral lag of photons with energy E with respect to the energy band 8–25 keV. For H2S and H2S-dominated-tracking pulses, a weak correlation between and k E is found, where W is the pulse width. We also study the spectral lag behavior with peak time of pulses for 30 well-shaped pulses and estimate the main trend of the spectral lag behavior with . It is found that is correlated with k E . We perform simulations under a phenomenological model of spectral evolution, and find that these correlations are reproduced. We then conclude that spectral lags are closely related to spectral evolution within the pulse. The most natural explanation of these observations is that the emission is from the electrons in the same fluid unit at an emission site moving away from the central engine, as expected in the models invoking magnetic dissipation in a moderately high-σ outflow
A comprehensive analysis of Fermi Gamma-Ray Burst Data: IV. Spectral lag and Its Relation to Ep Evolution
The spectral evolution and spectral lag behavior of 92 bright pulses from 84
gamma-ray bursts (GRBs) observed by the Fermi GBM telescope are studied. These
pulses can be classified into hard-to-soft pulses (H2S, 64/92),
H2S-dominated-tracking pulses (21/92), and other tracking pulses (7/92). We
focus on the relationship between spectral evolution and spectral lags of H2S
and H2S-dominated-tracking pulses. %in hard-to-soft pulses (H2S, 64/92) and
H2S-dominating-tracking (21/92) pulses. The main trend of spectral evolution
(lag behavior) is estimated with
(), where is the peak photon
energy in the radiation spectrum, is the observer time relative to the
beginning of pulse , and is the spectral lag of photons
with energy with respect to the energy band - keV. For H2S and
H2S-dominated-tracking pulses, a weak correlation between
and is found, where is the pulse width. We also study the spectral
lag behavior with peak time of pulses for 30 well-shaped pulses
and estimate the main trend of the spectral lag behavior with . It is found that is correlated with
. We perform simulations under a phenomenological model of spectral
evolution, and find that these correlations are reproduced. We then conclude
that spectral lags are closely related to spectral evolution within the pulse.
The most natural explanation of these observations is that the emission is from
the electrons in the same fluid unit at an emission site moving away from the
central engine, as expected in the models invoking magnetic dissipation in a
moderately-high- outflow.Comment: 58 pages, 11 figures, 3 tables. ApJ in pres
The in the single Cabibbo-suppressed process
In this work, we have investigated the Cabibbo-suppressed process , by taking into account the intermediate scalar state
, which could be dynamically generated from the -wave
pseudoscalar-pseudoscalar interaction within the chiral unitary approach. We
have calculated the invariant mass distribution, and found that
there is a significant structure associated to the . We have also
roughly estimated the branching fraction . We encourage our experimental colleagues to measure the
process for searching for the state
signal in this reaction.Comment: 8 pages, 5 figure
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