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Can AI Understand Our Universe? Test of Fine-Tuning GPT by Astrophysical Data

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arxiv 2404.10019 v1 pith:WTMAQEV2 submitted 2024-04-14 astro-ph.IM astro-ph.GAastro-ph.HEcs.AIcs.LGphysics.data-an

classification astro-ph.IMastro-ph.GAastro-ph.HEcs.AIcs.LGphysics.data-an
keywords datauniversearticleastrophysicalfundamentalgrbsmodelquasars
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ChatGPT has been the most talked-about concept in recent months, captivating both professionals and the general public alike, and has sparked discussions about the changes that artificial intelligence (AI) will bring to the world. As physicists and astrophysicists, we are curious about if scientific data can be correctly analyzed by large language models (LLMs) and yield accurate physics. In this article, we fine-tune the generative pre-trained transformer (GPT) model by the astronomical data from the observations of galaxies, quasars, stars, gamma-ray bursts (GRBs), and the simulations of black holes (BHs), the fine-tuned model demonstrates its capability to classify astrophysical phenomena, distinguish between two types of GRBs, deduce the redshift of quasars, and estimate BH parameters. We regard this as a successful test, marking the LLM's proven efficacy in scientific research. With the ever-growing volume of multidisciplinary data and the advancement of AI technology, we look forward to the emergence of a more fundamental and comprehensive understanding of our universe. This article also shares some interesting thoughts on data collection and AI design. Using the approach of understanding the universe - looking outward at data and inward for fundamental building blocks - as a guideline, we propose a method of series expansion for AI, suggesting ways to train and control AI that is smarter than humans.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 3 citations worldwide. Full citation record

  1. Machine Learning-Based Analytical Expressions for Gray-Body Factors and Application to Primordial Black Holes

    astro-ph.CO 2025-04 conditional novelty 6.0 of 10

    Symbolic regression is used to derive compact error-function approximations for Schwarzschild gray-body factors, and the approximations reproduce the Hawking spectra and primordial black hole constraints from full num...

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