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	1. Characteristics of nonautonomous W-shaped soliton and Peregrine comb in a variable-coefficient higher-order nonlinear Schrödinger equation
	Xing Zhang,Yin-Chuan Zhao,Feng-Hua Qi,Liu-Ying Cai
	Physics 17 October 2016
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	Abstract:In this paper, we study the nonautonomous characteristics of the W-shaped solitons on constant backgrounds for a variable-coefficient higher-order nonlinear Schrödinger (vc-HNLS) equation. Several types of solitons are obtained in exponentially, linearly and periodically fluctuating decreasing dispersion profiles, respectively. We also show the compression effect of the third-order dispersion (TOD) coefficient on the W-shaped soliton. We further analyze the formation and spatiotemporal characteristics of the Peregrine combs (PCs) when TOD coefficient is of the periodic form. Moreover, the PC can be converted into the Peregrine wall if the modulation amplitude is equal to 1.
	TO cite this article:Xing Zhang,Yin-Chuan Zhao,Feng-Hua Qi, et al. Characteristics of nonautonomous W-shaped soliton and Peregrine comb in a variable-coefficient higher-order nonlinear Schrödinger equation[OL].[17 October 2016] http://en.paper.edu.cn/en_releasepaper/content/4707262


	2. Position diversity in dependence network increases individual economic production
	XIE Wen-Jie,Yang Yan-Hong,JIANG Zhi-Qiang,Zhou Wei-Xing
	Physics 24 May 2016
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	Abstract:The availability of big data recorded from massively multiplayer online role-playing game (MMORPG) allow us to gain a deeper understanding the potential connection between avatar's network positidon and their economic production. We use a statistical filtering method to construct dependence networks from weighted friendship networks of avatars. We identify 30 distinct motif positions in the 13 directed triadic motifs which represent microscopic dependence among avatars. Based on structural similarity of motif positions, we further classify avatars into different groups. The node position diversity of avatars is found to be positively correlated with their economic production. We also find that the economic production of leaf nodes are significantly lower than that of the other nodes in the same motif. Our findings shed light on understanding the influence of network structure on economic activities and production in social system.
	TO cite this article:XIE Wen-Jie,Yang Yan-Hong,JIANG Zhi-Qiang, et al. Position diversity in dependence network increases individual economic production[OL].[24 May 2016] http://en.paper.edu.cn/en_releasepaper/content/4692010

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	3. The stochastic dynamical theory for the complex systems with power-law distributions
	Du Jiulin
	Physics 20 November 2015
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	Abstract:The stochastic dynamical theory for the systems with power-law distributions has been discussed by means of using the Langevin equations with inhomogeneous friction and noise and the corresponding Fokker-Planck equations. The power-law distributions and the generalized fluctuation-dissipation relation under which these distributions can be generated in a complex system away from equilibrium have been found. And simultaneously, the Klein-Kramers equation and the Smoluchowski equation have been generalized to the dynamical systems with the solutions of power-law distributions. The numerical analyses have shown the power-law distributions all excellently fitting with the solutions of the dynamics of the Langevin equations.
	TO cite this article:Du Jiulin. The stochastic dynamical theory for the complex systems with power-law distributions[OL].[20 November 2015] http://en.paper.edu.cn/en_releasepaper/content/4661711


	4. Thermodynamics of noncommutative geometry inspired black holes
	WU Yumei,LIU Chang,MIAO Yangang
	Physics 04 November 2015
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	Abstract:With the rational fraction form or the exponential form as a replacement of $delta$-function form as the density distribution of black holes, the mass-smeared regularized AdS black holes are investigated from their configurations and thermodynamics, including variation of the mass with respect to the horizon radius and the Hawking temperature, entropy, Gibbs free energy, and heat capacity at a constant pressure as well. It turns out that the mass-smeared black hole possesses anextremal configuration in which the temperature is zero. Based on the first law of thermodynamics, there is a modification to the area law which depends on the form of smearing. The Gibbs free energy corresponding to phase structure may behave differently at different vacuum pressures, specifically, the phase structure is more complex in a low pressure. We reveal similarities for the black holes of the two forms both in configurations and thermodynamics.
	TO cite this article:WU Yumei,LIU Chang,MIAO Yangang. Thermodynamics of noncommutative geometry inspired black holes[OL].[ 4 November 2015] http://en.paper.edu.cn/en_releasepaper/content/4659732


	5. Weak Gravity Conjecture and Holographic/Agegraphic Dark Energy
	SUN Cheng-Yi
	Physics 05 December 2013
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	Abstract:A criterion that should be satisfied in the inflation andquintessence models has been motivated from the weak gravityconjecture (WGC) by Huang. However, it is found that the criterionis inconsistent with the holographic dark energy (HDE) and newagegraphic dark energy (NADE) models. In the note, we firstly showthat in the HDE and NADE models the criterion should be be replacedrespectively by two new criterions. Secondly, we apply the newcriterions indicated by WGC to survey the two models. We find thatthe contradiction between WGC and the NADE model is removed when thenew criterion is used. In the HDE model, we find the effects of thespatial curvature and the interaction should be considered in orderto match the new criterion.
	TO cite this article:SUN Cheng-Yi. Weak Gravity Conjecture and Holographic/Agegraphic Dark Energy[OL].[ 5 December 2013] http://en.paper.edu.cn/en_releasepaper/content/4573194


	6. Exact solutions for the Boussinesq-Burgerslong-wave equations in shallow water
	Wang Lei
	Physics 28 September 2013
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	Abstract:Boussinesq-Burgers (B-B) equations describe the long-wavepropagation in shallow water and are potentially applicable to theharbor and coastal designs. By virtue of the matrix extension in theWronskian technique, some exact solutions of the B-B equationsare obtained, such as the soliton, rational and periodic solutions.Solitonic interactions are discussed. Elastic-inelastic-interactioncoexistence is hereby observed, in addition to the previously-seenpure inelastic or elastic interactions.
	TO cite this article:Wang Lei. Exact solutions for the Boussinesq-Burgerslong-wave equations in shallow water[OL].[28 September 2013] http://en.paper.edu.cn/en_releasepaper/content/4562003


	7. Renormalizability and Nonrenormalizable Interactions
	Yao Haibo,Wu Shishu
	Physics 03 January 2011
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	Abstract:Arguments are provided which show that extension of renormalizability in quantum field theory is possible. By an appropriate choice of effective Lagrangian, a dressed Feynman propagator is obtained. In this scheme, higher order Feynman diagrams become self-convergent and nonrenormalizable interactions become renormalizable. As an example, the vacuum fluctuation effects on ho meson mass for the vector-tensor coupling model is discussed. It is found that the result can agree with the experimental value when coupling constant is adjusted.
	TO cite this article:Yao Haibo,Wu Shishu. Renormalizability and Nonrenormalizable Interactions[OL].[ 3 January 2011] http://en.paper.edu.cn/en_releasepaper/content/4403642


	8. Area spectrum of large AdS black hole from quasinormal modes
	WEI Shaowen,LIU Yuxiao
	Physics 12 November 2010
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	Abstract:Using the new physical interpretation of quasinormal modes proposed by Maggiore, we calculate the area and entropy spectra for the 3-dimensional and 5-dimensional large Ads black hole. The spectra are obtained by imposing the Bohr-Sommerfeld quantization condition and the adiabatic invariant quantity. With this semiclassical method, we find that the spacings of the area and entropy spectra aare equidistant and independent of the Ads radius of the black hole for both the casess. However, the spacings of the spectra are not the same for different dimension of space-time. The equidistant area spectra will be broken when the black hole has other paprameters (i.e., charge and angular momentum) of in a non-Einstein's gravity theory.
	TO cite this article:WEI Shaowen,LIU Yuxiao. Area spectrum of large AdS black hole from quasinormal modes[OL].[12 November 2010] http://en.paper.edu.cn/en_releasepaper/content/4391389


	9. Evolution of squeezed chaotic state in an amplitude dissipative channel
	Gang Ren,Hong-yi Fan,Li-yun Hu
	Physics 19 March 2010
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	Abstract:We investigate how the density operator of a squeezed chaotic field (a mixed state) evolves in the amplitude dissipative channel. We demonstrate that the evolved density operator ρ(t) is in a Gaussian quadratic form, and the Q-function of ρ(t) is derived, which manifestly exhibits the dissipation.
	TO cite this article:Gang Ren,Hong-yi Fan,Li-yun Hu. Evolution of squeezed chaotic state in an amplitude dissipative channel[OL].[19 March 2010] http://en.paper.edu.cn/en_releasepaper/content/40863


	10. Stable matter-wave packets in a traveling lattice potential
	Hai Wenhua,Li Zejun,Rong Shiguang
	Physics 04 March 2010
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	Abstract:We consider a Bose-Einstein condensate (BEC) driven by a traveling lattice potential and derive an exact traveling-wave solution of the one-dimensional (1D) Gross-Pitaevskii equation (GPE), which satisfies a balance condition between the optical potential and interatomic interaction. The balance condition means the conservation of the total potential, and the exact solution contains some Bloch-like states and shows that the matter-wave has spatial profile in the form of sinusoid wave and propagates like a quasi-free particle with the lattice velocity.
	TO cite this article:Hai Wenhua,Li Zejun,Rong Shiguang. Stable matter-wave packets in a traveling lattice potential[OL].[ 4 March 2010] http://en.paper.edu.cn/en_releasepaper/content/40419

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