Seismic full-waveform inversion is an ideal tool to recover the Earth's interior structure over various scales from the recorded data. At the heart of the inversion process is wavefield simulation, which is often rigid, costly, and not data driven. The commonly used time domain wave equation modeling is a relatively expensive and usually executed for one source at a time. In realistic inversion scenarios, the frequencies needed to illuminate the Earth are limited (Sirgue & Pratt, 2004). Frequency-domain seismic modeling, based on the Helmholtz wave equation, provides compact representations of subsurface wavefields (Marfurt, 1984). Those representations are highly desirable in applications like waveform inversion (Pratt et al., 1998). However, the computational cost of numerically solving the Helmholtz equation increases almost exponentially with frequency. The cost becomes more of a burden when we have to compute multi high frequency wavefields, as each frequency often requires its own matrix inversion. Besides, the complexity of the Helmholtz equation, when we consider more realistic physics like those for anisotropic media, limits our ability to solve it numerically (Wu & Alkhalifah, 2018).A recently developed physics-informed neural network (PINN) framework (Raissi et al., 2019) showed potential as an efficient surrogate modeling approach for frequency-domain wavefields (Alkhalifah, Song, bin