نتایج جستجو برای: probability density

تعداد نتایج: 608426  

2005
Peter Hall Hong Ooi

We discuss properties of two methods for ascribing probabilities to the shape of a probability distribution. One is based on the idea of counting the number of modes of a bootstrap version of a standard kernel density estimator. We argue that the simplest form of that method suffers from the same difficulties that inhibit level accuracy of Silverman’s bandwidth-based test for modality: the cond...

پایان نامه :وزارت علوم، تحقیقات و فناوری - دانشگاه رازی - دانشکده علوم 1387

boron nitride semiconducting zigzag swcnt, $b_{cb}$$n_{cn}$$c_{1-cb-cn}$, as a potential candidate for making nanoelectronic devices was examined. in contrast to the previous dft calculations, wherein just one boron and nitrogen doping configuration have been considered, here for the average over all possible configurations, density of states (dos) was calculated in terms of boron and nitrogen ...

Journal: :desert 2015
zhaofei liu zongxue xu

two statistical downscaling models, the non-homogeneous hidden markov model (nhmm) and the statistical down–scaling model (sdsm) were used to generate future scenarios of both mean and extremes in the tarim river basin,which were based on nine combined scenarios including three general circulation models (gcms) (csiro30, echam5,and gfdl21) predictor sets and three special report on emission sce...

Journal: :Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics 1995
Chekhlov Yakhot

High-resolution numerical experiments, described in this work, show that velocity fluctuations governed by the one-dimensional Burgers equation driven by a white-intime random noise with the spectrum |f(k)| ∝ k exhibit a biscaling behavior: All moments of velocity differences Sn≤3(r) = |u(x+ r)− u(x)| n ≡ |∆u| ∝ rn/3, while Sn>3(r) ∝ r ξn with ξn ≈ 1 for real n > 0 (Chekhlov and Yakhot, Phys. R...

Journal: :Physical review. E, Statistical, nonlinear, and soft matter physics 2010
Kwok Sau Fa K G Wang

In this paper, we present an integrodifferential diffusion equation for continuous-time random walk that is valid for a generic waiting time probability density function. Using this equation, we also study diffusion behaviors for a couple of specific waiting time probability density functions such as exponential and a combination of power law and generalized Mittag-Leffler function. We show tha...

Journal: :Physical review letters 1996
Yakhot Chekhlov

The dynamics of velocity fluctuations governed by the Burgers equation, driven by the white-in-time random forcing function with f fsx 1 r , td 2 fsx, t0dg2 ~ rdst 2 t0d is considered on the interval 0 , x , L. The properties of the probability density function of velocity differences PsDu, rd are investigated for the three cases j ­ h0; 1y2; 2j. It is shown that the tail of the probability den...

Journal: :Journal of theoretical biology 1998
K C Chen R M Ford P T Cummings

The angular turning probability density distribution for motile bacteria is usually measured in local coordinates and is therefore inconvenient for global analyses of the chemotactic bacterial migration. In this paper we present analytical derivations that convert the local angular turning probability density distribution into a global one. The explicit expression of a reduced global turning pr...

Journal: :Physical review. E, Statistical, nonlinear, and soft matter physics 2002
Wenhua Hai Chaohong Lee Guishu Chong Lei Shi

Using the idea of the macroscopic quantum wave function and the definition of the classical chaos, we analytically reveal that the probability density of two periodically driven and weakly coupled Bose-Einstein condensates is deterministic but not predictable. Numerical calculation for the time evolutions of the chaotic probability density demonstrates the analytical result and exhibits the non...

2008
Mark Daniel Ward

cannot be a probability density function. To see this, note 2x− x = −x(x− √ 2)(x+ √ 2). If C = 0, then f(x) = 0 for all x, so ∫∞ −∞ f(x) = 0, but every probability density function has ∫∞ −∞ f(x) = 1. If C > 0, then f(x) < 0 on the range x ∈ (0, √ 2), but every probability density function has f(x) ≥ 0 for all x. If C < 0, then f(x) < 0 on the range x ∈ ( √ 2, 5/2), but every probability densit...

Journal: :Monthly Notices of the Royal Astronomical Society 2015

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