2,825 results for equation · 0.219s

arxiv.org/abs/cond-mat/0302046v4

Kinetics and Boltzmann kinetic equation for fluctuation Cooper pairs

The Boltzmann equation for excess Cooper pairs above T_c is derived in the framework of the time-dependent Ginzburg-Landau (TDGL) theory using Langevin's approach of the stochastic differential equation. The Newton dynamic equation for the momentum...

arxiv.org/abs/math/0410517v1

Stability of Solutions of Fuzzy Differential Equations

In this paper, We study the stability of solutions of fuzzy differential equations by Lyapunov's second method. By using scale equations and comparison principle for Lyapunov - like functions, we give some sufficient criterias for the stability and...

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arxiv.org/abs/1709.01785v1

Non-hyperbolic solutions to tangle equations involving composite links

Solving tangle equations is deeply connected with studying enzyme action on DNA. The main goal of this paper is to solve the system of tangle equations $N(O+X_1)=b_1$ and $N(O+X_2)=b_2 \# b_3$, where $X_1$ and $X_2$ are rational tangles, and $b_i$ is...

en.wikipedia.org/wiki/Equation_solving

Equation solving - Wikipedia

may be solved either numerically or symbolically. Solving an equation numerically means that only numbers are admitted as solutions. Solving an equation

arxiv.org/abs/1406.3524v4

A Fick-Jacobs equation for channels over 3D curves

The purpose of this paper is to provide new formulas for the effective diffusion coefficient of a generalized Fick-Jacobs equation for narrow 3-dimensional channels. The generalized Fick-Jacobs equation is obtained by projecting the 3-dimensional dif...

arxiv.org/abs/2405.05780v1

Neural Network Learning of Black-Scholes Equation for Option Pricing

One of the most discussed problems in the financial world is stock option pricing. The Black-Scholes Equation is a Parabolic Partial Differential Equation which provides an option pricing model. The present work proposes an approach based on Neural N...

arxiv.org/abs/1803.09137v3

A stochastic telegraph equation from the six-vertex model

A stochastic telegraph equation is defined by adding a random inhomogeneity to the classical (second order linear hyperbolic) telegraph differential equation. The inhomogeneities we consider are proportional to the two-dimensional white noise, and so...

math.stackexchange.com/questions/4428167/why-is-it-that-when-there-are-fewer-equations-than-unknowns-we-have-infinite-sol

Why is it that when there are fewer equations than unknowns we have ...

Apr 15, 2022 · Why is it that when there are fewer equations than unknowns we have infinite solutions in a system of linear equations? [closed] Ask Question Asked 3 years, 10 months ago Modified 3 years, …

arxiv.org/abs/2106.10061v1

Arterial Tube Laws and Wave Speeds

The 1-D theory of flow in the arteries yields an equation for the wave speed in terms of the density of blood and the distensibility of the vessel. By means of this equation there is a duality between the equation for the wave speed and the tube law...

arxiv.org/abs/1408.2726v2

Bloch-Redfield equations for modeling light-harvesting complexes

We challenge the misconception that Bloch-Redfield equations are a less powerful tool than phenomenological Lindblad equations for modeling exciton transport in photosynthetic complexes. This view predominantly originates from an indiscriminate use o...

arxiv.org/abs/math/0612758v1

Global time estimates for solutions to equations of dissipative type

Global time estimates of Lp-Lq norms of solutions to general strictly hyperbolic partial differential equations are considered. The case of special interest in this paper are equations exhibiting the dissipative behaviour. Results are applied to di...

arxiv.org/abs/2006.02540v1

On the Determinant Problem for the Relativistic Boltzmann Equation

This article considers a long-outstanding open question regarding the Jacobian determinant for the relativistic Boltzmann equation in the center-of-momentum coordinates. For the Newtonian Boltzmann equation, the center-of-momentum coordinates have pl...

arxiv.org/abs/1803.03557v1

Modified Fractional Logistic Equation

In the article [B.J.West, Exact solution to fractional logistic equation, Physica A: Statistical Mechanics and its Applications 429 (2015) 103-108], the author has obtained a function as the solution to fractional logistic equation (FLE). As demonstr...

arxiv.org/abs/1208.1165v5

A Generalized Mean-Reverting Equation and Applications

Consider a mean-reverting equation, generalized in the sense it is driven by a 1-dimensional centered Gaussian process with Hölder continuous paths on $[0,T]$ ($T > 0$). Taking that equation in rough paths sense only gives local existence of the sol...

arxiv.org/abs/2512.21070v1

Sparse identification of delay equations with distributed memory

We present a novel extension of the SINDy framework to delay differential equations with {\it distributed delays} and {\it renewal equations}, where typically the dependence from the past manifests via integrals in which the history is weighted throu...

arxiv.org/abs/1312.6759v3

ODE/IM correspondence and modified affine Toda field equations

We study the two-dimensional affine Toda field equations for affine Lie algebra $\hat{\mathfrak{g}}$ modified by a conformal transformation and the associated linear equations. In the conformal limit, the associated linear problem reduces to a (pseud...

math.stackexchange.com/questions/4428167/why-is-it-that-when-there-are-fewer-equations-than-unknowns-we-have-infinite-sol

Why is it that when there are fewer equations than unknowns we have ...

Apr 15, 2022 · Why is it that when there are fewer equations than unknowns we have infinite solutions in a system of linear equations? [closed] Ask Question Asked 3 years, 10 months ago Modified 3 years, …

arxiv.org/abs/0908.2269v2

A Symplectic Integrator for Hill's Equations

Hill's equations are an approximation that is useful in a number of areas of astrophysics including planetary rings and planetesimal disks. We derive a symplectic method for integrating Hill's equations based on a generalized leapfrog. This method...

arxiv.org/abs/gr-qc/0207113v1

New Path Equations in Absolute Parallelism Geometry

The Bazanski approach, for deriving the geodesic equations in Riemannian geometry, is generalized in the absolute parallelism geometry. As a consequence of this generalization three path equations are obtained. A striking feature in the derived equ...

arxiv.org/abs/1003.1338v1

Smooth and Peaked Solitons of the CH equation

The relations between smooth and peaked soliton solutions are reviewed for the Camassa-Holm (CH) shallow water wave equation in one spatial dimension. The canonical Hamiltonian formulation of the CH equation in action-angle variables is expressed fo...

arxiv.org/abs/1909.08472v1

A note on Kazdan-Warner equation on networks

We investigate the Kazdan-Warner equation on a network. In this case, the differential equation is defined on each edge, while appropriate transition conditions of Kirchhoff type are prescribed at the vertices. We show that the Kazdan-Warner theory e...

arxiv.org/abs/1801.06869v1

Counter-propagating waves in a system of transport-reaction equations

Hyperbolic transport-reaction equations are abundant in the description of movement of motile organisms. Here, we focus on system of four coupled transport-reaction equations that arises from an age-structuring of a species of turning individuals. Th...

arxiv.org/abs/2412.11933v2

Generalised Fermat equation: a survey of solved cases

Generalised Fermat equation (GFE) is the equation of the form $ax^p+by^q=cz^r$, where $a,b,c,p,q,r$ are positive integers. If $1/p+1/q+1/r<1$, GFE is known to have at most finitely many primitive integer solutions $(x,y,z)$. A large body of the liter...

arxiv.org/abs/2212.13269v5

Bethe-Salpeter equation for classical gravitational bound states

The Bethe-Salpeter equation is a non-perturbative, relativistic and covariant description of two-body bound states. We derive the classical Bethe-Salpeter equation for two massive point particles (with or without spin) in a bound gravitational system...