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Baryon Physics and Tight Coupling Approximation in Boltzmann Codes

机译:Boldonmann Codes中的Baryon物理和紧密耦合近似

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We provide two derivations of the baryonic equations that can be straightforwardly implemented in existing Einstein–Boltzmann solvers. One of the derivations begins with an action principle, while the other exploits the conservation of the stress-energy tensor. While our result is manifestly covariant and satisfies the Bianchi identities, we point out that this is not the case for the implementation of the seminal work by Ma and Bertschinger and in the existing Boltzmann codes. We also study the tight coupling approximation up to the second order without choosing any gauge using the covariant full baryon equations. We implement the improved baryon equations in a Boltzmann code and investigate the change in the estimate of cosmological parameters by performing an MCMC analysis. With the covariantly correct baryon equations of motion, we find 1 % deviation for the best fit values of the cosmological parameters that should be taken into account. While in this paper, we study the Λ CDM model only, our baryon equations can be easily implemented in other models and various modified gravity theories.
机译:我们提供了两个可以在现有的Einstein-Boltzmann溶剂中直接实现的缩官方程的两个推导。其中一个推导始于动作原理,而另一个衍生物始于保护压力 - 能量张量的保护。虽然我们的结果表明,但满足了Bianchi身份,但我们指出了MA和Bertschinger和现有的Boltzmann Codes中的开创性工作并非如此。我们还在不使用协变为全缩放方程式的情况下研究紧密的耦合近似,而不选择任何规格。我们通过执行MCMC分析来实现Boldzmann码中的改进的Baryon方程,并通过执行MCMC分析来研究宇宙学参数估计的变化。利用相辅相机的矫正矫正运动的运动方程,我们发现应该考虑宇宙学参数的最佳拟合值的1%偏差。在本文中,我们仅研究λCDM型号,我们的Baryon方程可以在其他模型和各种改进的重力理论中容易地实现。

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