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Xiao-Bo Gong

Publications and source records attributed to Xiao-Bo Gong.

4 recordsLinked to original sources

Mean-squared displacement and variance for confined Brownian motion

For one-dimension Brownian motion in the confined system with the size $L$, the mean-squared displacement(MSD) defined by $\left \langle (x-x_0)^2 \right\rangle$ should be proportional to $t^{α(t)}$. The power $α(t)$ should range from $1$ to $0$ over time, and the MSD turns from $2Dt$ to $c L^2$, here the coefficient $c$ independent of $t$, $D$ being the diffusion coefficient. The paper aims to quantitatively solve the MSD in the intermediate confinement regime. The key to this problem is how to deal with the propagator and the normalization factor of the Fokker-Planck equation(FPE) with the Dirichlet Boundaries. Applying the Euler-Maclaurin approximation(EMA) and integration by parts for the small $t$, we obtain the MSD being $2Dt(1-\frac{2\sqrtξ }{3π\sqrtπ})$, with $t_{ch}=\frac{L^2}{4π^2D},ξ\equiv \frac{t}{t_{ch}}$, and the power $α(t)$ being $\frac{1-0.18\sqrtξ}{1-0.12\sqrtξ}$. Further, we analysis the MSD and the power for the $d$-dimension system with $γ$-dimension confinement. In the case of $γ< d$, there exists the sub-diffusive behavior in the intermediate time. The universal description is consistent with the recent experiments and simulations in the micro-nano systems. Finally, we calculate the position variance(PV) meaning $\left\langle (x-\left\langle x \right\rangle)^2 \right\rangle$. Under the initial condition referring to the different probability density function(PDF) being $p_{0}(x)$, MSD and PV should exhibit different dependencies on time, which reflect corresponding diffusion behaviors.As examples, the paper discusses the representative initial PDFs reading $p_{0}(x)=δ(x-x_0)$, with the midpoint $x_0=\frac{L}{2}$ and the endpoint $x_0=ε$(or $0^+$).The MSD(equal to PV) reads $2Dt(1-\frac{5π^3 Dt}{L^2})$,and $\frac{4}π(2Dt)[1+\frac{2\sqrt{πDt}}{L}]$for the small $t$,respectively.

cond-mat.stat-mech

A new derivation of the relationship between diffusion coefficient and entropy in classical Brownian motion by the ensemble method

The diffusion coefficient--a measure of dissipation, and the entropy--a measure of fluctuation are found to be intimately correlated in many physical systems. Unlike the fluctuation dissipation theorem in linear response theory, the correlation is often strongly non-linear. To understand this complex dependence, we consider the classical Brownian diffusion in this work. Under certain rational assumption, i.e. in the bi-component fluid mixture, the mass of the Brownian particle $M$ is far greater than that of the bath molecule $m$, we can adopt the weakly couple limit. Only considering the first-order approximation of the mass ratio $m/M$, we obtain a linear motion equation in the reference frame of the observer as a Brownian particle. Based on this equivalent equation, we get the Hamiltonian at equilibrium. Finally, using canonical ensemble method, we define a new entropy that is similar to the Kolmogorov-Sinai entropy. Further, we present an analytic expression of the relationship between the diffusion coefficient $D$ and the entropy $S$ in the thermal equilibrium, that is to say, $D =\frac{\hbar}{eM} \exp{[S/(k_Bd)]}$, where $d$ is the dimension of the space, $k_B$ the Boltzmann constant, $\hbar $ the reduced Planck constant and $e$ the Euler number. This kind of scaling relation has been well-known and well-tested since the similar one for single component is firstly derived by Rosenfeld with the expansion of volume ratio.

cond-mat.stat-mech

Geometric phase and topological phase diagram of the one-dimensional $XXZ$ Heisenberg spin chain in a longitudinal field

In this paper, we determine the geometric phase for the one-dimensional $XXZ$ Heisenberg chain with spin-$1/2$, the exchange couple $J$ and the spin anisotropy parameter $Δ$ in a longitudinal field(LF) with the reduced field strength $h$. Using the Jordan-Wigner transformation and the mean-field theory based on the Wick's theorem, a semi-analytical theory has been developed in terms of order parameters which satisfy the self-consistent equations. The values of the order parameters are numerically computed using the matrix-product-state(MPS) method. The validity of the mean-filed theory could be checked through the comparison between the self-consistent solutions and the numerical results. Finally, we draw the the topological phase diagrams in the case $J<0$ and the case $J>0$.

cond-mat.stat-mech

Phase-Transition Theory of Kerr Black Holes in Electromagnetic Field

For a Kerr black hole (KBH) with spin $J$ and mass $M$ in a steady electromagnetic field, a special Wald vacuum solution (WVS) has been found in the case of no-source uniform field. For WVS, the Meissner effect (ME) occurs only in the the extreme KBH where $M^2/J=1$, in this case, the magnetic field is totally excluded from the event horizon (EH) of KBH. However, WVS does not consider the Hawking radiation (HR) but treats KBH as an absolutely black body. If HR is added , researchers believe that the condition is not so restricted and it is possible for ME to occur in less extreme case. How less is the "less extreme case"? This paper tries to answer this question. Since the Hawking temperature $T_H$ of KBH defined by HR is proportional to the surface gravity $κ$ at the EH, this question is actually about the so-called existence/non-existence of ME (ME/NME) or superconducting phase transition. In this paper, we study the connection between the superconductivity of KBH-EH and the existence of Weyl Fermion (WF). Using thermodynamic formulas and the KBH state equation, we prove that the inherent-parameter condition for ME to occur is $M^2/J\leq ε_c=1.5$ in force-free fields whether it be in the simple axisymmetric vacuum zero source case or in the non-zero source case which can be described by the nonlinear Grad-Shafranov (G-S) equation. We suggest that this is a second-order phase transition and we calculate the critical exponents $δ=1$ and $η=1/2$ for the specific heat diverging at constant $J$, and the critical point $(M_c, Ω_c)$, which equals $(1.22\sqrt{ J}, 0.16/\sqrt{ J})$ where $Ω$ is the angular velocity of KBH. Furthermore we draw the phase diagrams in both $(M, J)$ and $(M,Ω)$ coordinates.

gr-qc