Cosmic ray propagators in the fractional differential model of bounded anomalous diffusion
Vladimir V. Uchaikin, Renat T. Sibatov

TL;DR
This paper introduces a new bounded anomalous diffusion model using fractional derivatives to better represent cosmic ray propagation, accounting for finite particle speeds and providing a novel approach in cosmic ray physics.
Contribution
The paper proposes a new fractional differential model for cosmic ray propagation that incorporates finite particle speeds through the bounded anomalous diffusion framework.
Findings
Introduces a bounded anomalous diffusion model with fractional derivatives.
Analyzes and critiques existing models in cosmic ray physics.
Provides a new equation accounting for finite particle speeds.
Abstract
Fractional differential approach to cosmic ray physics problems is discussed. A short review in this field is given, some results are represented, analyzed and criticized. A new model called the bounded anomalous diffusion model is offered. Its equation includes the fractional material derivative which allows to take into account the finite speed of cosmic rays particles.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsFractional Differential Equations Solutions · Cosmology and Gravitation Theories · Astrophysics and Cosmic Phenomena
