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Fast Prediction and Evaluation of Gravitational Waveforms Using Surrogate Models

机译:使用代理模型的重力波形快速预测和评估

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We propose a solution to the problem of quickly and accurately predicting gravitational waveforms within any given physical model. The method is relevant for both real-time applications and more traditional scenarios where the generation of waveforms using standard methods can be prohibitively expensive. Our approach is based on three offline steps resulting in an accurate reduced order model in both parameter and physical dimensions that can be used as a surrogate for the true or fiducial waveform family. First, a set of m parameter values is determined using a greedy algorithm from which a reduced basis representation is constructed. Second, these m parameters induce the selection of m time values for interpolating a waveform time series using an empirical interpolant that is built for the fiducial waveform family. Third, a fit in the parameter dimension is performed for the waveform’s value at each of these m times. The cost of predicting L waveform time samples for a generic parameter choice is of order O(mL+mcfit) online operations, where cfit denotes the fitting function operation count and, typically, m?L. The result is a compact, computationally efficient, and accurate surrogate model that retains the original physics of the fiducial waveform family while also being fast to evaluate. We generate accurate surrogate models for effective-one-body waveforms of nonspinning binary black hole coalescences with durations as long as 105M, mass ratios from 1 to 10, and for multiple spherical harmonic modes. We find that these surrogates are more than 3 orders of magnitude faster to evaluate as compared to the cost of generating effective-one-body waveforms in standard ways. Surrogate model building for other waveform families and models follows the same steps and has the same low computational online scaling cost. For expensive numerical simulations of binary black hole coalescences, we thus anticipate extremely large speedups in generating new waveforms with a surrogate. As waveform generation is one of the dominant costs in parameter estimation algorithms and parameter space exploration, surrogate models offer a new and practical way to dramatically accelerate such studies without impacting accuracy. Surrogates built in this paper, as well as others, are available from GWSurrogate, a publicly available python package.
机译:我们提出了解决问题的解决方案,以便在任何给定的物理模型中快速准确地预测引力波形。该方法与实时应用以及使用标准方法的波形产生的更传统的情景相关,可能是非常昂贵的。我们的方法基于三个离线步骤,从而在参数和物理尺寸中获得准确的减少的订单模型,可以用作真实或基准波形系列的代理。首先,使用从中构建减少的基础表示的贪婪算法来确定一组M个参数值。其次,这些M个参数诱导使用构成为基准波形系列的经验内插内插入波形时间序列的M时间值的选择。第三,在这些M次中的每一个的波形的值下执行参数尺寸的拟合。预测通用参数选择的L波形时间样本的成本是OR顺序O(ML + MCFIT)在线操作,其中CFIT表示拟合函数操作计数,通常,m?l。结果是一种紧凑,计算的高效和准确的代理模型,其保留了基准波形系列的原始物理,同时也快速评估。我们为不超过105米,1至10的质量比和多个球形谐波模式产生准确的代理模型。我们发现,与标准方式生成有效一体波形的成本相比,这些替代品越来越快3个数量级。其他波形系列和模型的代理模型建筑跟随相同的步骤,并且具有相同的低计算在线缩放成本。对于二元黑洞聚合的昂贵数值模拟,因此我们预计使用代理生成新的波形时非常大的加速。由于波形生成是参数估计算法和参数空间探索中的主要成本之一,代理模型提供了一种新的和实用的方法,可以在不影响准确率的情况下大大加速这些研究。本文建造的代理以及其他人可以从GWSurrogate,一个公开的Python包提供。

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