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Leiming Du

Publications and source records attributed to Leiming Du.

3 recordsLinked to original sources

A State-Variable Theory of Evolving Material Symmetry

Material architecture can evolve during loading, yet its mechanically expressed symmetry depends on both the structural state and the constitutive coupling. We connect these quantities through one parent-invariant free energy with a symmetric traceless internal tensor $\mathbf Q$. Its stabilizer distinguishes isotropic, uniaxial, and biaxial states, and projected gradient kinetics satisfies the structural dissipation inequality. Parent invariance generally guarantees only symmetry inheritance. For an explicit two-coupling elastic potential, we derive a stiffness-contraction reconstruction of $\mathbf Q$ and prove equality of the structural and tangent rotational symmetries for every nonzero coupling pair. The associated acoustic tensor links residual symmetry to protected transverse degeneracies. For a small uniaxial state, the leading squared-speed gap is $|γ_2s|\sin^2\vartheta/(2ρ_0)$; coupling selectivity and residual protection can suppress this term. We also derive a directional acoustic-trace reconstruction and state calibrated and nuisance-aware inverse conditions. Dimensionless structural-field, acoustic, transient finite-element, and synthetic inverse examples illustrate the predictions. The framework connects state evolution, mechanically expressed symmetry, and conditional observability without assigning independent dynamics to a group label.

physics.app-ph↗

The correlations of multi-wave band luminosity and BLR luminosity in Fermi 2LAC blazars

We collect a sample of 78 Fermi detected blazars with broad line region (BLR) data and the quasi-simultaneous multi-wave band data. By analyzing the sample, we find: (1) For whole blazar sample, there exist significant correlations between radio, $γ$-ray luminosity and BLR luminosity. The slope of the best-fit linear regression equation is close to the theoretical value 1. Our results provided another support of jet-disk symbiosis. (2) For FSRQ sample, we find a significant correlation between radio luminosity and optical luminosity, and weaker correlations between X-ray luminosity and radio, optical luminosity. It indicates that the X-ray band radiation mechanism is slightly different from radio and optical bands. The X-ray emission is diluted by inverse Compton scattering (IC). There is a significant correlation between BLR luminosity and $γ$-ray luminosity, but no correlations between X-ray luminosity and BLR, $γ$-ray luminosity, which suggests that the seed soft photons are different for IC process. From these results we suggest that the X-ray band emission is diluted by synchrotron self-Compton (SSC) process, $γ$-ray band emission is produced by external Compton (EC) process.

astro-ph.HE↗

On estimators of the jet bolometric luminosity of Fermi 2LAC blazars

Bolometric luminosity is a basic physical parameter that is widely used in the study of blazars. Due to the lack of simultaneous full wavelength data, several estimators of the bolometric luminosity are being used in practice. In this paper, we study and evaluate the reliability and significance of six estimators, the $5GHz$ luminosity, the 1keV luminosity, the $γ$-ray luminosity, the $5GHz$ luminosity+the 1keV luminosity, the $5GHz$ luminosity+the $γ$-ray luminosity and the 1keV luminosity+the $γ$-ray luminosity, by analyzing the linear correlations between the integrated bolometric luminosity and them. Our main results are as follows. (i) All the six estimators are reliable in the sense that they are all significant correlated with the bolometric luminosity. (ii) Ranking from the higher significance of the reliability to lower one the six estimators are the the $5GHz$ luminosity+the $γ$-ray luminosity, the 1keV luminosity+the $γ$-ray luminosity, $γ$-ray luminosity, the $5GHz$ luminosity+the 1keV luminosity, the $5GHz$ luminosity and the 1keV luminosity. (iii) We suggest that the bolometric luminosity can be well estimated by the $γ$-ray luminosity using the best linear equation that given in this paper for Fermi FSRQs. (iv) According to the linear regressions obtained in the analysis, we provide calibration for each estimator.

astro-ph.HE↗