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Airy beams for radiative near-field communications: Funda...
[Submitted on 19 Aug 2025 (v1), last revised 28 Aug 2026 (this v · 2025-08-19 · via eess.SP updates on arXiv.org

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Abstract:In next-generation wireless networks, the combination of electrically large radiating apertures and high-frequency transmission extends the radiating near-field region around the transmitter. In this region, unlike in the far field, the wavefront is nonplanar, which provides additional degrees of freedom to shape and steer the transmitted beam in a desired manner. In this paper, we focus on Airy beams, which may exhibit several highly desirable properties in the near-field region. Ideally, these beams follow self-accelerating (curved) trajectories, demonstrate resilience to perturbations through self-healing, and maintain a consistent intensity profile across all planes perpendicular to the propagation direction, making them effectively diffraction-free. Specifically, we first present the underlying principles of self-accelerating beams radiated by continuous aperture field distributions. We then address several challenges regarding the generation of Airy beams, including their exponential decay due to finite energy constraints and spatial truncation of the aperture. Moreover, we examine their free-space propagation characteristics. The second part of the paper focuses on the propagation behavior of Airy beams in non-line-of-sight (NLoS) scenarios. A comparison is also presented between Airy beams and Gaussian beams. Our theoretical and numerical results show that Airy beams may offer a performance advantage over Gaussian beams in certain NLoS channels, provided that their key properties are largely preserved, specifically, self-acceleration along a parabolic trajectory and diffraction-free propagation. In the presence of an obstacle, this requires that the portion of the transmit aperture with a clear line-of-sight to the receiver is sufficiently large.

Submission history

From: Donatella Darsena [view email]
[v1] Tue, 19 Aug 2025 10:20:31 UTC (2,756 KB)
[v2] Mon, 22 Jun 2026 09:18:52 UTC (3,715 KB)
[v3] Fri, 28 Aug 2026 20:27:37 UTC (6,013 KB)