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Determination of the Hubble Constant from Quadruply Imaged Gravitational Lens Systems

机译:从四极成像重力透镜系统确定霍布布尔常数

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Determining H0 from the time delays in quadruply imaged leng systems needs the knowledge of the deflecting potential ψ(r,θ). We present two different methods to solve this problem. On the one hand, we assume that the potential belongs to a broad class of non-elliptical models and we write down a system of equations which can be numerically solved to get all the parameters of the model using only the image positions and some physical constraints. On the other hand, we show how it is possible to estimate H0 from the time delays without completely reconstructing the potential, provided that ψ(r,θ)=raF(θ), whatever the shape function F(θ) is. After some tests on simulated cases, we apply both methods to the real quadruple lenges PG1115+080 and B1422+231 finally obtaining H0 = 58+17-15 km s-1 Mpc-1.
机译:从四向成像的LENG系统中的时间延迟确定H0需要了解偏转电位ψ(R,θ)。我们提出了两种不同的方法来解决这个问题。一方面,我们假设潜力属于广泛的非椭圆模型,我们写下了一个等式系统,可以数量解决,以仅使用图像位置和一些物理约束来获取模型的所有参数。另一方面,我们示出了如何从时延迟估计H0而不完全重建电位,只要ψ(r,θ)= raf(θ),无论形状函数f(θ)是什么。在对模拟案例进行一些测试后,我们将两种方法应用于真正的四端速PG1115 + 080和B1422 + 231最终获得H0 = 58 + 17-15公里的S-1 MPC-1。

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