15,264 research outputs found

    Covariant chiral nucleon-nucleon contact Lagrangian up to order O(q4)\mathcal{O}(q^4)

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    We adopt a covariant version of the naive dimensional analysis and construct the chiral two-nucleon contact Lagrangian constrained by Lorentz, parity, charge conjugation, hermitian conjugation, and chiral symmetries. We show that at O(q0)\mathcal{O}(q^0), O(q2)\mathcal{O}(q^2), O(q4)\mathcal{O}(q^4), where qq denotes a generic small quantity, there are 4, 13, and 23 terms, respectively. We find that by performing 1/mN1/m_N expansions, the covariant Lagrangian reduces to the conventional non-relativistic one, which includes 2, 7, and 15 terms at each corresponding order.Comment: 9 page

    An Improved Roe Scheme for All Mach-Number Flows Simultaneously Curing Known Problems

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    Roe scheme is known for its good performance in moderate-Mach-number flows. However, this scheme and its extended versions suffers from many disastrous problems, such as non-physical behavior, global cut-off, and checkerboard problems, for incompressible flows; and shock instability, expansion shock, and positively non-conservative problems for hypersonic flows. In this paper, non-physical behavior problem, checkerboard problem, and main reason of shock instability problem are due to that the Roe scheme cannot identify multi-dimensional incompressible and compressible flows when normal Mach number on the cell face tends to zero, and then leads to incorrect cross modifications. Positively non-conservative problem is also identified as another important reason for shock instability. Therefore, Mach number and an assistant pressure-density-varying detector are introduced into the Roe scheme to judge compressibility, positivity condition is satisfied by a simple modification with minimal numerical dissipation increases and even with possible decreases in numerical dissipation, the mechanism of the preconditioned Roe scheme is introduced to suppress checkerboard problem, and modified entropy fix and the rotated Riemann solver is combined with complementary advantages as an assistant improvement for better robust. Based on above improvements and previous developments for global cut-off and expansion shock problems, an improvement Roe scheme for all Mach-number flow (Roe-AM) is proposed to simultaneously overcome nearly all well-known drawbacks of the classical Roe scheme. The Roe-AM scheme is simple, easy to implement, computationally low-cost, robust, good extensibility, and free of empirical parameters essentially, with increasing minimal numerical dissipation

    Charge density waves and phonon-electron coupling in ZrTe3_3 investigated by Raman spectroscopy and first-principles calculations

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    Charge-density-wave (CDW) order has long been interpreted as arising from a Fermi-surface instability in the parent metallic phase. While phonon-electron coupling has been suggested to influence the formation of CDW order in quasi-two-dimensional (quasi-2D) systems, the presumed dominant importance of Fermi-surface nesting remains largely unquestioned in quasi-1D systems. Here we show that phonon-electron coupling is also important for the CDW formation in a model quasi-1D system ZrTe3_3. Our joint experimental and computational study reveals that particular lattice vibrational patterns possess exceedingly strong coupling to the conduction electrons, and are directly linked to the lattice distortions associated with the CDW order. The dependence of the coupling matrix elements on electron momentum further dictates the opening of (partial) electronic gaps in the CDW phase. Since lattice distortions and electronic gaps are the defining signatures of CDW order, our result demonstrates that the conventional wisdom based on Fermi-surface geometry needs to be substantially supplemented by phonon-electron coupling even in the simplest quasi-1D case. As prerequisites for the CDW formation, the highly anisotropic electronic structure and strong phonon-electron coupling in ZrTe3_3 give rise to a distinct Raman scattering effect, namely, measured phonon linewidths depend on the direction of momentum transfer in the scattering process.Comment: 23 pages, 9 figure

    WWΞ³/ZWW\gamma/Z production in the Randall-Sundrum model at LHC and CLIC

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    We study the W+Wβˆ’Ξ³(Z)W^+W^-\gamma(Z) productions at both the CERN Large Hadron Collider (LHC) and the Compact Linear Collider (CLIC) in the framework of the Randall-Sundrum (RS) model. The impacts of the virtual RS Kaluza-Klein (KK) graviton on these processes are studied and compared with the standard model (SM) background. We present the integrated and differential cross sections in both the RS model and the SM. The results show that the relative RS discrepancies at the CLIC differ from those at the LHC, particularly in the transverse momentum and rapidity distributions. We also find that the RS signature performance, as a result of the resonance character of the RS KK-graviton spectrum, is distinctively unlike that in the large extra dimensions model. We conclude that the CLIC with unprecedented precision and high center-of-mass energy has a potential advantage over the LHC in exploring the effects of the RS KK graviton on the W+Wβˆ’Ξ³(Z)W^+W^-\gamma(Z) production processes.Comment: 22 pages, 18 figure

    Anomaly analysis of Hawking radiation from 2+1 dimensional spinning black hole

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    Considering gravitational and gauge anomalies at the horizon, a new successful method that to derive Hawking radiations from black holes has been developed recently by Wilczek et al.. By using the dimensional reduction technique, we apply this method to a non-vacuum solution, the 2+1 dimensional spinning black hole. The Hawking temperature and angular velocity on the horizon are obtained. The results may partially imply that this method is independent of the gravity theory, the dimension of spacetime and the topological structure of the event horizon.Comment: v2: 5 pages, typos corrected, references adde

    Tests for CPT sum rule and U-spin violation in Time-dependent CP violation of Bs0β†’K+Kβˆ’B^0_s \to K^+ K^- and Bd0β†’Ο€+Ο€βˆ’B^0_d \to \pi^+ \pi^-

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    Recent LHCb data for time-dependent CP violation in Bd0β†’Ο€+Ο€βˆ’B_d^0 \to \pi^+\pi^- and Bs0β†’K+Kβˆ’B^0_s\to K^+K^- show deviations from theoretical predictions. Besides their central values for CK+Kβˆ’\mathcal C_{K^+K^-}, SK+Kβˆ’\mathcal S_{K^+K^-} and AK+Kβˆ’Ξ”Ξ“\mathcal A^{\Delta \Gamma}_{K^+K^-} violate quantum mechanic CPT invariant sum rule (CPT sum rule) prediction of ∣CK+Kβˆ’βˆ£2+∣SK+Kβˆ’βˆ£2+∣AK+Kβˆ’Ξ”Ξ“βˆ£2=1|\mathcal C_{K^+K^-}|^2 + |\mathcal S_{K^+K^-}| ^2 + |\mathcal A^{\Delta \Gamma}_{K^+K^-}|^2 = 1 (LHCb data imply the sum to be 0.67Β±0.200.67\pm 0.20.), their values for CK+Kβˆ’=0.24Β±0.06Β±0.02\mathcal C_{K^+ K^-}= 0.24\pm 0.06\pm {0.02} and CΟ€+Ο€βˆ’=βˆ’0.24Β±0.07Β±0.01\mathcal C_{\pi^+ \pi^-} = - 0.24\pm 0.07\pm 0.01 also show large violation of SU(3) or its U-spin sub-group symmetry (SU(3)/U) relation CK+Kβˆ’/CΟ€βˆ’Ο€+=βˆ’B(Bd0β†’Ο€βˆ’Ο€+)Ο„Bs0/B(Bs0β†’K+Kβˆ’)Ο„Bd0\mathcal C_{K^+ K^-} /\mathcal C_{\pi^- \pi^+} = - \mathcal B(B_d^0 \to \pi^- \pi^+)\tau_{B^0_s}/\mathcal B(B^0_s \to K^+ K^-)\tau_{B_d^0} (LHCb data imply the ratio of left-side to right-side to be 4.67Β±1.884.67\pm 1.88.) . The LHCb results need to be further confirmed to be taken seriously. We suggest to use time-dependent CP violation in Bsβ†’K0KΛ‰0,Ο€+Ο€βˆ’,Ο€0Ο€0B_s\to K^0\bar K^0, \pi^+\pi^-, \pi^0\pi^0 to further test the CPT sum rule. Assuming that the sum rule holds, we propose that violation of the SU(3)/U relation may indicate a large FSI phase difference in the Ο€+Ο€βˆ’\pi^+\pi^- and K+Kβˆ’K^+K^- re-scattering. We suggest several other U-spin pairs of Bβ†’PPB\to PP decays to further test SU(3)/U relations.Comment: 12 pages, 1 figure; ACP of Bd0β†’Ο€+Ο€βˆ’B^0_d \to \pi^+ \pi^- updated to the latest HFAG average, figures slightly changed, a few comments and refs adde

    Physical States and BRST Operators for Higher-spin WW Strings

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    In this paper, we mainly investigate the W2,sMβŠ—W2,sLW_{2,s}^{M}\otimes W_{2,s}^{L} system, in which the matter and the Liouville subsystems generate W2,sMW_{2,s}^{M} and W2,sLW_{2,s}^L algebras respectively. We first give a brief discussion of the physical states for corresponding WW stings. The lower states are given by freezing the spin-2 and spin-ss currents. Then, introducing two pairs of ghost-like fields, we give the realizations of W1,2,sW_{1,2,s} algebras. Based on these linear realizations, BRST operators for W2,sW_{2,s} algebras are obtained. Finally, we construct new BRST charges of Liouville system for W2,sLW_{2,s}^{L} strings at the specific values of central charges cc: c=βˆ’22/5c=-{22/5} for W2,3LW_{2,3}^{L} algebra, c=βˆ’24c=-24 for W2,4LW_{2,4}^{L} algebra and c=βˆ’2,βˆ’286/3c=-2,-{286/3} for W2,6LW_{2,6}^{L} algebra, at which the corresponding W2,sLW_{2,s}^L algebras are singular.Comment: 18 pages, 2 tables, no figure

    All-optical diode based on plasmonic attenuation and nonlinear frequency conversion

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    We present design of an all-optical diode in a metal-dielectric structure where plasmonic attenuation and quasi-phase-matching (QPM) is harnessed to improve its performance greatly. Due to the anti-symmetric design of the nonlinear susceptibility, different incident direction will ignite different plasmonic nonlinear process, which either compensates plasmonic attenuation sufficiently or accelerates it seriously. As a result, unidirectional output of plasmonic signal is achieved. This designed all-optical diode shows advantages of low power consumption, short sample length, high isolation contrast, wide acceptance of structural and initial conditions, and tunable unidirectionality, and becomes of practical interest

    A Monte Carlo Study of the Spectra from Inhomogeneous Accretion Flow

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    The model of inhomogeneous accretion flow, in which cold clumps are surrounded by hot gas or corona, has been proposed to explain the spectral features of black hole X-ray binaries (BHXBs). In this work, we try to find possible observational features in the continuum that can indicate the existence of clumps. The spectra of inhomogeneous accretion flow are calculated via the Monte Carlo method. Since the corresponding accretion flow is unsteady and complex, the accretion flow is described by a set of free parameters, the ranges of which can include the real cases. The influences of the parameters are investigated. It is found that the thermal component of the spectra deviates from the multi-color black body spectra in the middle power-law part. On the one hand, a warp appears due to the gap region between the clumps and the outer cold disk, and on the other hand, the slope of the line connecting the thermal peaks deviates from 4/3. The warp feature, as well as the correlation between the thermal peak at higher frequency and the spectral index, are possible to indicate the existence of clumps, and are worthy of further investigation with more self-consistent models.Comment: 11 pages, 3 figures, to appear in Research in Astronomy and Astrophysics (RAA

    Precise predictions for AHqβˆ’A_H q_- associated production in the littlest Higgs model with TT parity at the LHC

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    In the framework of the littlest Higgs model with TT parity, we present complete calculations for the AHqβˆ’A_H q_- (qβˆ’=uβˆ’,uΛ‰βˆ’,dβˆ’,dΛ‰βˆ’,cβˆ’,cΛ‰βˆ’,sβˆ’,sΛ‰βˆ’)(q_-=u_-, \bar{u}_-,d_-, \bar{d}_-,c_-, \bar{c}_-,s_-, \bar{s}_-) associated production up to the QCD next-to-leading order (NLO) at the CERN Large Hadron Collider with subsequent pure weak decay of TT-odd mirror quark. We apply the PROSPINO scheme to avoid the double counting problem and to keep the convergence of the perturbative QCD description. The theoretical correlations between the integrated cross section and the factorization and renormalization scale, the global symmetry-breaking scale and the Yukawa coupling parameter are studied separately. We also provide the kinematic distributions of the final decay products. Our numerical results show that the NLO QCD correction reduces the scale uncertainty and enhances the leading-order integrated cross section remarkably, with the KK factor varying in the range of 1.41∼1.681.41 \sim 1.68 (1.58∼1.891.58 \sim 1.89) as the increment of the global symmetry-breaking scale ff from 500Β GeV500~{\rm GeV} to 1.5Β TeV1.5~{\rm TeV} (1.1Β TeV1.1~{\rm TeV}) at the s=14Β TeV\sqrt{s} = 14~{\rm TeV} (8Β TeV8~{\rm TeV}) LHC. We find that it is possible to select the signal events of the AHqβˆ’A_Hq_- production from its background by putting proper cuts on the final leading jet and missing energy.Comment: 28 pages, 14 figure
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