基于变压器的行星系统生成模型

IF 5.8 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Yann Alibert, Jeanne Davoult, Sara Marques
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引用次数: 0

摘要

上下文。行星系统形成的数值计算在计算能力方面要求很高。然而,这些合成的行星系统可以提供在给定的数值框架中预测的同一系统中行星属性之间的相关性。反过来,这种相关性可以用来指导和优先考虑旨在发现某些类型的行星(如类地行星)的观测活动。我们的目标是开发一个生成模型,能够捕捉同一系统中行星之间的相关性和统计关系。这样一个模型,在Bern模型的基础上训练,提供了以很少的计算成本生成大量合成行星系统的可能性。例如,这些综合系统可用于指导观测活动。我们使用了一个由大约25,000个行星系统组成的训练数据库,每个系统最多有20个行星,并假设有一颗类似太阳的恒星,这些系统是用伯尔尼模型生成的。我们的生成模型基于转换器体系结构,它以有效地捕获序列中的相关性而闻名,并形成了所有现代大型语言模型的基础。为了评估生成模型的有效性,我们进行了视觉和统计比较,以及机器学习驱动的测试。最后,作为一个用例,我们考虑了TOI-469系统,在这个系统中,我们的目标是根据系统中发现的第一颗行星b的特性来预测行星c和d的可能属性。使用不同的比较方法,我们证明了由我们的模型生成的系统的性质与由Bern模型直接计算的系统的性质非常相似。我们还证明,不同的分类器不能区分直接计算和生成的种群,增加了对同一系统中行星之间的统计相关性相似的信心。最后,我们展示了在TOI-469系统的情况下,使用生成模型允许我们基于已经观测到的行星的特性来预测尚未观测到的行星的特性。我们在网站上向社区提供的生成模型可用于研究各种问题,例如理解系统中行星某些属性之间的相关性,或在给定某些部分信息(例如,存在一些更容易观察的行星)的情况下预测行星系统的组成。然而,重要的是要注意,我们生成模型的性能依赖于底层数值模型的能力——这里是Bern模型——准确地表示行星系统的实际形成过程。另一方面,我们的生成模型可以很容易地使用社区提供的其他数值模型作为输入进行再训练。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A transformer-based generative model for planetary systems
Context. Numerical calculations of planetary system formation are very demanding in terms of computing power. These synthetic planetary systems can, however, provide access to correlations, as predicted in a given numerical framework, between the properties of planets in the same system. Such correlations can, in return, be used to guide and prioritise observational campaigns aimed at discovering certain types of planets, such as Earth-like planets.Aims. Our goal is to develop a generative model capable of capturing correlations and statistical relationships between planets in the same system. Such a model, trained on the Bern model, offers the possibility to generate a large number of synthetic planetary systems with little computational cost. These synthetic systems can be used, for example, to guide observational campaigns.Methods. We used a training database of approximately 25 000 planetary systems, each with up to 20 planets and assuming a solar-type star, generated using the Bern model. Our generative model is based on the transformer architecture, which is well-known for efficiently capturing correlations in sequences and forms the basis of all modern large language models. To assess the validity of the generative model, we performed visual and statistical comparisons, as well as machine learning-driven tests. Lastly, as a use case, we considered the TOI-469 system, in which we aimed to predict the possible properties of planets c and d based on the properties of planet b, the first planet detected in the system.Results. Using different comparison methods, we show that the properties of systems generated by our model are very similar to those of the systems computed directly by the Bern model. We also demonstrate that different classifiers cannot distinguish between the directly computed and generated populations, adding confidence that the statistical correlations between planets in the same system are similar. Lastly, we show in the case of the TOI-469 system that using the generative model allows us to predict the properties of planets not yet observed based on the properties of the already observed planet.Conclusions. Our generative model, which we provide to the community on our website, can be used to study a variety of problems, such as understanding correlations between certain properties of planets in systems or predicting the composition of a planetary system given some partial information (e.g. the presence of some easier-to-observe planets). Nevertheless, it is important to note that the performance of our generative model relies on the ability of the underlying numerical model – here, the Bern model – to accurately represent the actual formation process of planetary systems. Our generative model could, on the other hand, very easily be retrained using as input other numerical models provided by the community.
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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