دورية أكاديمية

Random walks with non-Gaussian step-size distributions and the folding of random polymer chains.

التفاصيل البيبلوغرافية
العنوان: Random walks with non-Gaussian step-size distributions and the folding of random polymer chains.
المؤلفون: Shaw RH; Department of Physics, University of Alberta, Edmonton, Alberta, Canada T6G 2J1. dshaw@phys.ualberta.ca, Tuszyński JA
المصدر: Physical review. E, Statistical, nonlinear, and soft matter physics [Phys Rev E Stat Nonlin Soft Matter Phys] 2003 Mar; Vol. 67 (3 Pt 1), pp. 031102. Date of Electronic Publication: 2003 Mar 13.
نوع المنشور: Journal Article
اللغة: English
بيانات الدورية: Publisher: American Physical Society Country of Publication: United States NLM ID: 101136452 Publication Model: Print-Electronic Cited Medium: Print ISSN: 1539-3755 (Print) Linking ISSN: 15393755 NLM ISO Abbreviation: Phys Rev E Stat Nonlin Soft Matter Phys Subsets: PubMed not MEDLINE
أسماء مطبوعة: Publication: : Ridge, NY : American Physical Society
Original Publication: Melville, NY : Published by the American Physical Society through the American Institute of Physics, c2001-
مستخلص: In this paper, we study a random walker whose step-size distribution is of non-Gaussian bimodal form due to the addition of a quartic term in the exponential. By the central limit theorem, we know that in the limit of a large number of steps, the probability distribution representing the distance the walker has traveled becomes Gaussian. We investigate the nature of this convergence both numerically and analytically. We obtain a scaling relation describing the number of steps required for convergence in terms of the width and separation of the peaks of the step-size distribution. We assume in the concluding section that our model is well suited for the application of the folding of a random polymer chain.
تواريخ الأحداث: Date Created: 20030412 Date Completed: 20030926 Latest Revision: 20030411
رمز التحديث: 20221213
DOI: 10.1103/PhysRevE.67.031102
PMID: 12689050
قاعدة البيانات: MEDLINE
الوصف
تدمد:1539-3755
DOI:10.1103/PhysRevE.67.031102