awhere kB is the Boltzmann constant, T is the temperature, and η 那里千字节是伯磁曼常数, T是温度和η[translate] athe diffusion velocity of the considered particle is the same to 正在翻译,请等待...[translate] athe equation for decay time into the above equation, and by[translate]...
However, as I indicated in a comment, I am doubtful this equation is modelling what you think it is. By your description, the repository starts out with an amount of300300. The first year, an additional300300are added to it, for a total of600600, not including decay. T...
General equation for Zeno-like effects in spontaneous exponential decaymeasurement theoryZeno effectdynamical descriptionspontaneous decayDifferent perturbation mechanisms of the spontaneous decay constant are shown: the inelastic interaction of emitted particles with particle detector, decay onto an unstable ...
By using frequency-support considerations for AM− and AN+, we can obtain better decay in M and N, and thus this term is less serious than our argument suggests. While HM+ is not necessarily AM+, the same argument applies. References Aizenman, M., Duminil-Copin, H.: Marginal trivial...
The four free parameters of the model are fixed by the chiral condensate, and by the pseudoscalar meson properties (pion mass, kaon mass, pion decay constant). We discuss the T=0 equation of state (EoS) which describes quark confinement (zero quark matter pressure) below the critical ...
Exponential decay is the mathematical term used to illustrate the concept of a exponentially decreasing quantity. If a given total decreases by a certain percentage every year, for example, the formula for exponential decay can be used to model the decay. Answer and Explanation: The formul...
This is related to the nature of the observability inequalities for the adjoint heat equation that are unable to provide estimates on the solutions at t = T because of the very strong smoothing effect. In fact, as indicated in the context of the constant-coefficient heat equation, even when ...
We present and test two new methods for the numerical solution of the relativistic wave equation [(-+m)+(-+m)+V(r)-M]ψ( r--> )=0, which appears in the theory of relativistic quark-antiquark bound states. Our methods work directly in position space, and hence have the desirable fe...
In contrast to (6.5) below, (6.2) is satisfied for all times , and we use the word “ancient” to emphasize this fact. That is, the solution is a stationary process, its distribution is constant in time. The law of the sequence of mean-zero, Gaussian random variables is uniquely deter...
It is found that a large localized pulse can suffer modulational instability and then collapse into the shortest-wavelength modes, as for the classical nonlinear Schrödinger equation. However, the total energy of the nonconservative GNSE can also become constant during the collapse via local ...