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2025 | OriginalPaper | Chapter

Development of Mass and Energy Rate (Density) of Dissipative Systems Over Their Lifetimes: A Comparison of a Low-Mass Star, like Our Sun, a Human, and the Roman Empire

Author : Martin van Duin

Published in: Navigating Complexity in Big History

Publisher: Springer Nature Switzerland

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Abstract

This chapter delves into the intricate dynamics of dissipative systems, focusing on the evolution of mass and energy rate density over their lifetimes. By comparing a low-mass star like our Sun, a human, and the Roman Empire, the text provides a comprehensive analysis of how these systems develop, stabilize, and ultimately decline. The study highlights the unique characteristics and complexities of each system, offering insights into their energy processing mechanisms and the factors that drive their evolution. The chapter explores the concept of energy rate density as a metric for complexity, discussing its applicability and limitations in different contexts. It also examines the role of information processing in the development of complex systems, suggesting that traditional metrics may not fully capture the intricacies of biological and social systems. The detailed examination of mass and energy flows, along with the use of proxies for system complexity, makes this chapter a valuable resource for understanding the dynamics of dissipative systems across various realms. The text also discusses the historical and cultural significance of these systems, providing a broader perspective on their development and impact. Overall, this chapter offers a deep dive into the complexities of dissipative systems, shedding light on their energy dynamics and the factors that shape their evolution.

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Metadata
Title
Development of Mass and Energy Rate (Density) of Dissipative Systems Over Their Lifetimes: A Comparison of a Low-Mass Star, like Our Sun, a Human, and the Roman Empire
Author
Martin van Duin
Copyright Year
2025
DOI
https://doi.org/10.1007/978-3-031-85410-1_11

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