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Open Physics

formerly Central European Journal of Physics

Editor-in-Chief: Seidel, Sally

Managing Editor: Lesna-Szreter, Paulina


IMPACT FACTOR 2017: 0.755
5-year IMPACT FACTOR: 0.820

CiteScore 2018: 1.01

SCImago Journal Rank (SJR) 2018: 0.237
Source Normalized Impact per Paper (SNIP) 2018: 0.541

ICV 2017: 162.45

Open Access
Online
ISSN
2391-5471
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Volume 6, Issue 1

Issues

Volume 13 (2015)

On the truncated Pareto distribution with applications

Lorenzo Zaninetti / Mario Ferraro
Published Online: 2008-03-26 | DOI: https://doi.org/10.2478/s11534-008-0008-2

Abstract

The Pareto probability distribution is widely applied in different fields such us finance, physics, hydrology, geology and astronomy. This note deals with an application of the Pareto distribution to astrophysics and more precisely to the statistical analysis of masses of stars and of diameters of asteroids. In particular a comparison between the usual Pareto distribution and its truncated version is presented. Finally, a possible physical mechanism that produces Pareto tails for the distribution of the masses of stars is presented.

PACS: 95.75.-z; 96.30.Ys; 97.10.Xq

Keywords: statistical distributions; asteroids-meteoroids; stars: luminosity and mass functions

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About the article

Published Online: 2008-03-26

Published in Print: 2008-03-01


Citation Information: Open Physics, Volume 6, Issue 1, Pages 1–6, ISSN (Online) 2391-5471, DOI: https://doi.org/10.2478/s11534-008-0008-2.

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© 2008 Versita Warsaw. This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 3.0 License. BY-NC-ND 3.0

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