Simulating time-domain observations of gravitational wave (GW) detector environments will allow for a better understanding of GW sources, augment datasets for GW signal detection and help in characterizing the noise of the detectors, leading to better physics. This paper presents a novel approach to simulating fixed-length time-domain signals using a three-player Wasserstein Generative Adversarial Network (WGAN), called DVGAN, that includes an auxiliary discriminator that discriminates on the derivatives of input signals. An ablation study is used to compare the effects of including adversarial feedback from an auxiliary derivative discriminator with a vanilla two-player WGAN. We show that discriminating on derivatives can stabilize the learning of GAN components on 1D continuous signals during their training phase. This results in smoother generated signals that are less distinguishable from real samples and better capture the distributions of the training data. DVGAN is also used to simulate real transient noise events captured in the advanced LIGO GW detector.
翻译:模拟重力波探测器环境的时空观测将使人们更好地了解GW源,增加GW信号探测的数据集,并有助于描述探测器的噪音,从而导致更好的物理学。本文介绍了一种新型的方法,利用一个叫作DVGAN的三位玩家瓦塞尔斯坦·格恩蒂恩·德韦斯特·德瓦萨里尔网络(WGAN)模拟固定长时空域信号,其中包括一个对输入信号衍生物有区别的辅助歧视器。还进行了一项反向研究,将辅助衍生物分析器的对抗性反馈与香草双球探测器WGAN进行对比。我们表明,对衍生物的区别对待可以稳定其在培训阶段对1D连续信号的学习。其结果是,光滑生成的信号不易与真实样本区分,更能捕捉到培训数据的分布。DVGAN还用于模拟高级LIGGG GW探测器所捕捉到的真正瞬动噪音事件。