2,099 research outputs found

    Triangle singularity in the J/ψK+Kf0(980)(a0(980))J/\psi \rightarrow K^+ K^- f_0(980)(a_0(980)) decays

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    We study the J/ψK+Kf0(980)(a0(980))J/\psi \rightarrow K^+ K^- f_0(980)(a_0(980)) reaction and find that the mechanism to produce this decay develops a triangle singularity around Minv(Kf0/Ka0)1515M_{\rm inv}(K^- f_0/K^- a_0) \approx 1515~MeV. The differential width dΓ/dMinv(Kf0/Ka0)d\Gamma / dM_{\rm inv}(K^- f_0/K^- a_0) 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 f0(980)f_0(980) and a0(980)a_0(980) as dynamically generated resonances from the interaction of pseudoscalar mesons. The branching ratios obtained for the J/ψK+Kf0(980)(a0(980))J/\psi \rightarrow K^+ K^- f_0(980)(a_0(980)) decays are of the order of 10510^{-5}, 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

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    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 K1(1270)K_1(1270) poles in D+νe+VPD^+\to \nu e^+ V P decay

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    We analyze theoretically the D+νe+ρKˉD^+\to \nu e^+ \rho \bar K and D+νe+KˉπD^+\to \nu e^+ \bar K^* \pi decays to see the feasibility to check the double pole nature of the axial-vector resonance K1(1270)K_1(1270) predicted by the unitary extensions of chiral perturbation theory (UChPT). Indeed, within UChPT the K1(1270)K_1(1270) 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 KπK^*\pi and the higher mass pole to ρK\rho K, 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 VPVP channels in D+νe+VPD^+\to \nu e^+ V P 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 K1(1270)K_1(1270) 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

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    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

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    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 logEpkElog(t+t0)\log E_p\propto k_E\log(t+t_0) (τ^kτ^logE{\hat{\tau}} \propto k_{\hat{\tau}}\log E), where EpE_p is the peak photon energy in the radiation spectrum, t+t0t+t_0 is the observer time relative to the beginning of pulse t0-t_0, and τ^{\hat{\tau}} is the spectral lag of photons with energy EE with respect to the energy band 88-2525 keV. For H2S and H2S-dominated-tracking pulses, a weak correlation between kτ^/Wk_{{\hat{\tau}}}/W and kEk_E is found, where WW is the pulse width. We also study the spectral lag behavior with peak time tpEt_{\rm p_E} of pulses for 30 well-shaped pulses and estimate the main trend of the spectral lag behavior with logtpEktplogE\log t_{\rm p_E}\propto k_{t_p}\log E. It is found that ktpk_{t_p} is correlated with kEk_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\sigma outflow.Comment: 58 pages, 11 figures, 3 tables. ApJ in pres

    The a0(980)a_0(980) in the single Cabibbo-suppressed process Λcπ0ηp\Lambda_c \to \pi^0\eta p

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    In this work, we have investigated the Cabibbo-suppressed process Λcπ0ηp\Lambda_c \to \pi^0\eta p, by taking into account the intermediate scalar state a0(980)a_0(980), which could be dynamically generated from the SS-wave pseudoscalar-pseudoscalar interaction within the chiral unitary approach. We have calculated the π0η\pi^0\eta invariant mass distribution, and found that there is a significant structure associated to the a0(980)a_0(980). We have also roughly estimated the branching fraction B(Λcπ0ηp)104\mathcal{B}(\Lambda_c \to \pi^0\eta p) \approx 10^{-4}. We encourage our experimental colleagues to measure the process Λcπ0ηp\Lambda_c \to \pi^0\eta p for searching for the state a0(980)a_0(980) signal in this reaction.Comment: 8 pages, 5 figure
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