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Forecasting the progression of human civilization on the Kardashev Scale through 2060 with a machine learning approach
Energy has been propelling the development of human civilization for millennia. Humanity presently stands at Type 0.7276 on the Kardashev Scale, which was proposed to quantify the relationship between energy consumption and the development of civilizations. However, current predictions of human civi...
Autores principales: | , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2023
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10338519/ https://www.ncbi.nlm.nih.gov/pubmed/37438428 http://dx.doi.org/10.1038/s41598-023-38351-y |
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author | Zhang, Antong Yang, Jiani Luo, Yangcheng Fan, Siteng |
author_facet | Zhang, Antong Yang, Jiani Luo, Yangcheng Fan, Siteng |
author_sort | Zhang, Antong |
collection | PubMed |
description | Energy has been propelling the development of human civilization for millennia. Humanity presently stands at Type 0.7276 on the Kardashev Scale, which was proposed to quantify the relationship between energy consumption and the development of civilizations. However, current predictions of human civilization remain underdeveloped and energy consumption models are oversimplified. In order to improve the precision of the prediction, we use machine learning models random forest and autoregressive integrated moving average to simulate and predict energy consumption on a global scale and the position of humanity on the Kardashev Scale through 2060. The result suggests that global energy consumption is expected to reach ~ 887 EJ in 2060, and humanity will become a Type 0.7449 civilization. Additionally, the potential energy segmentation changes before 2060 and the influence of the advent of nuclear fusion are discussed. We conclude that if energy strategies and technologies remain in the present course, it may take human civilization millennia to become a Type 1 civilization. The machine learning tool we develop significantly improves the previous projection of the Kardashev Scale, which is critical in the context of civilization development. |
format | Online Article Text |
id | pubmed-10338519 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2023 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-103385192023-07-14 Forecasting the progression of human civilization on the Kardashev Scale through 2060 with a machine learning approach Zhang, Antong Yang, Jiani Luo, Yangcheng Fan, Siteng Sci Rep Article Energy has been propelling the development of human civilization for millennia. Humanity presently stands at Type 0.7276 on the Kardashev Scale, which was proposed to quantify the relationship between energy consumption and the development of civilizations. However, current predictions of human civilization remain underdeveloped and energy consumption models are oversimplified. In order to improve the precision of the prediction, we use machine learning models random forest and autoregressive integrated moving average to simulate and predict energy consumption on a global scale and the position of humanity on the Kardashev Scale through 2060. The result suggests that global energy consumption is expected to reach ~ 887 EJ in 2060, and humanity will become a Type 0.7449 civilization. Additionally, the potential energy segmentation changes before 2060 and the influence of the advent of nuclear fusion are discussed. We conclude that if energy strategies and technologies remain in the present course, it may take human civilization millennia to become a Type 1 civilization. The machine learning tool we develop significantly improves the previous projection of the Kardashev Scale, which is critical in the context of civilization development. Nature Publishing Group UK 2023-07-12 /pmc/articles/PMC10338519/ /pubmed/37438428 http://dx.doi.org/10.1038/s41598-023-38351-y Text en © The Author(s) 2023 https://creativecommons.org/licenses/by/4.0/Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) . |
spellingShingle | Article Zhang, Antong Yang, Jiani Luo, Yangcheng Fan, Siteng Forecasting the progression of human civilization on the Kardashev Scale through 2060 with a machine learning approach |
title | Forecasting the progression of human civilization on the Kardashev Scale through 2060 with a machine learning approach |
title_full | Forecasting the progression of human civilization on the Kardashev Scale through 2060 with a machine learning approach |
title_fullStr | Forecasting the progression of human civilization on the Kardashev Scale through 2060 with a machine learning approach |
title_full_unstemmed | Forecasting the progression of human civilization on the Kardashev Scale through 2060 with a machine learning approach |
title_short | Forecasting the progression of human civilization on the Kardashev Scale through 2060 with a machine learning approach |
title_sort | forecasting the progression of human civilization on the kardashev scale through 2060 with a machine learning approach |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10338519/ https://www.ncbi.nlm.nih.gov/pubmed/37438428 http://dx.doi.org/10.1038/s41598-023-38351-y |
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