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    Generic effective sources for first-order in mass-ratio gravitational self-force calculations in Schwarzschild spacetime

    Chao Zhang (张超)1,*, Rong-gen Cai (蔡荣根)1,†, Guoyang Fu (付国杨)2,‡, Yungui Gong (龚云贵)1,§, Xuchen Lu (路旭晨)1,∥, and Wenting Zhou (周文婷)1,¶

    • 1Institute of Fundamental Physics and Quantum Technology, Department of Physics, School of Physical Science and Technology, Ningbo University, Ningbo, Zhejiang 315211, China
    • 2School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China

    • *Contact author: zhangchao1@nbu.edu.cn
    • †Contact author: caironggen@nbu.edu.cn
    • ‡Contact author: fuguoyangedu@sjtu.edu.cn
    • §Contact author: gongyungui@nbu.edu.cn
    • ∥Contact author: luxuchen@nbu.edu.cn
    • Contact author: zhouwenting@nbu.edu.cn

    Phys. Rev. D 112, 104069 – Published 24 November, 2025

    DOI: https://doi.org/10.1103/z9jr-qxc7

    Abstract

    The numerical calculation of gravitational self-force in extreme mass ratio inspiral systems is fundamentally challenging due to the singular nature of point-particle sources. To overcome these difficulties, the effective source method offers an innovative alternative by replacing traditional regularization techniques with a reformulation of the problem. In this paper, we present the first fully analytic framework for constructing effective sources to compute the gravitational self-force for generic orbits in Schwarzschild spacetime. By reformulating the singular field through angular modulation in terms of a tetrad decomposition, the effective source can be constructed with the linear combination of scalar modes. The derived effective source is continuous across the particle’s worldline, enabling efficient numerical implementation in 1+1 dimensions.

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