Abstract
This article continues to study the linearized Chandrasekhar equation. We use the Hilbert-type inequalities to accurately calculate the norm of the Fredholm integral operator and obtain the exact range for the parameters of the linearized Chandrasekhar equation to ensure that there is a unique solution to the equation in \(L^p\) space. A series of examples that can accurately calculate the norm of Fredholm integral operator shows that the Chandrasekhar kernel functions do not need to meet harsh conditions. As the symbolic part of the Chandrasekhar kernel function and the non-homogeneous terms satisfy the exponential decay condition, we yield a normed convergence rate of the approximation solution in \(L^p\) sense, which adds new results to the theory of radiation transfer in astrophysics.
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Acknowledgements
The authors would like to thank the anonymous referee for a careful reading of the manuscript and several helpful comments which contributed to improve the presentation of the paper. Sheng-Ya Feng is partially supported by the National Natural Science Foundation of China (Grant Nos. 11501203 and 11426109), the China Postdoctoral Science Foundation (Grant No. 2016M600278), and the National Foundation of China Scholarship Council (Grant No. 201806745028). Der-Chen Chang is partially supported by an NSF Grant DMS-1408839 and a McDevitt Endowment Fund at Georgetown University.
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Feng, SY., Chang, DC. Existence, uniqueness, and approximation solutions to linearized Chandrasekhar equation with sharp bounds. Anal.Math.Phys. 10, 17 (2020). https://doi.org/10.1007/s13324-020-00359-2
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DOI: https://doi.org/10.1007/s13324-020-00359-2
Keywords
- Chandrasekhar kernel
- Hilbert–Hardy inequality
- Fixed point theorem
- \(L^p\) solution
- Approximation solution