Large-step neural network for learning the symplectic evolution from partitioned data

Author:

Li Xin1,Li Jian23ORCID,Xia Zhihong Jeff4,Georgakarakos Nikolaos56

Affiliation:

1. Department of Statistics and Data Science, Southern University of Science and Technology of China . No 1088, Xueyuan Rd., Xili, Nanshan District, Shenzhen, Guangdong 518055, PR China

2. School of Astronomy and Space Science, Nanjing University , 163 Xianlin Avenue, Nanjing 210023, PR China

3. Key Laboratory of Modern Astronomy and Astrophysics in Ministry of Education, Nanjing University , Nanjing 210023, PR China

4. Department of Mathematics, Northwestern University , 2033 Sheridan Road, Evanston, IL 60208, USA

5. New York University Abu Dhabi , PO Box 129188 Abu Dhabi, United Arab Emirates

6. Center for Astro, Particle and Planetary Physics (CAP3), New York University Abu Dhabi , PO Box 129188 Abu Dhabi, United Arab Emirates

Abstract

ABSTRACT In this study, we focus on learning Hamiltonian systems, which involves predicting the coordinate ($\boldsymbol q$) and momentum ($\boldsymbol p$) variables generated by a symplectic mapping. Based on Chen & Tao (2021), the symplectic mapping is represented by a generating function. To extend the prediction time period, we develop a new learning scheme by splitting the time series ($\boldsymbol q_i$, $\boldsymbol p_i$) into several partitions. We then train a large-step neural network (LSNN) to approximate the generating function between the first partition (i.e. the initial condition) and each one of the remaining partitions. This partition approach makes our LSNN effectively suppress the accumulative error when predicting the system evolution. Then we train the LSNN to learn the motions of the 2:3 resonant Kuiper belt objects for a long time period of 25 000 yr. The results show that there are two significant improvements over the neural network constructed in our previous work: (1) the conservation of the Jacobi integral and (2) the highly accurate predictions of the orbital evolution. Overall, we propose that the designed LSNN has the potential to considerably improve predictions of the long-term evolution of more general Hamiltonian systems.

Funder

National Natural Science Foundation of China

National Key R&D Program of China

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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