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Hauptverfasser: Lindblom, Lee, Zhou, Tianji
Format: Preprint
Veröffentlicht: 2025
Schlagworte:
Online-Zugang:https://arxiv.org/abs/2502.10528
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author Lindblom, Lee
Zhou, Tianji
author_facet Lindblom, Lee
Zhou, Tianji
contents The relativistic inverse stellar structure problem determines the equation of state of the stellar matter given a knowledge of suitable macroscopic observable properties (e.g. their masses and radii) of the stars composed of that material. This study determines how accurately this equation of state can be determined using noisy mass and radius observations. The relationship between the size of the observational errors and the accuracy of the inferred equation of state is evaluated, and the optimal number of adjustable equation of state parameters needed to achieve the highest accuracy is determined.
format Preprint
id arxiv_https___arxiv_org_abs_2502_10528
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Uncertainty Quantification for the Relativistic Inverse Stellar Structure Problem
Lindblom, Lee
Zhou, Tianji
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
The relativistic inverse stellar structure problem determines the equation of state of the stellar matter given a knowledge of suitable macroscopic observable properties (e.g. their masses and radii) of the stars composed of that material. This study determines how accurately this equation of state can be determined using noisy mass and radius observations. The relationship between the size of the observational errors and the accuracy of the inferred equation of state is evaluated, and the optimal number of adjustable equation of state parameters needed to achieve the highest accuracy is determined.
title Uncertainty Quantification for the Relativistic Inverse Stellar Structure Problem
topic High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2502.10528