Site selection constraints and options for LILA-Pioneer and LILA-Horizon

TL;DR

The paper explores potential lunar sites for deploying LILA gravitational wave detectors, considering environmental, logistical, and scientific constraints to optimize lunar GW detection in the deciHz regime.

Contribution

It identifies multiple feasible lunar locations for LILA detectors, balancing scientific goals with practical deployment constraints.

Findings

Many candidate sites are suitable for LILA-Pioneer and LILA-Horizon.

Site selection depends on noise isolation, environmental protection, and accessibility.

LUNA's unique lunar environment enables low-frequency GW detection.

Abstract

The Earth's Moon presents a uniquely advantageous environment for detecting astrophysical gravitational waves (GWs), particularly in the scientifically interesting deciHz regime. The Laser Interferometer Lunar Antennae (LILA) project plans to perform GW measurements on the lunar surface, using the Moon's unique seismic quietness to access the deciHz regime. Two mission concepts are considered: the initial LILA-Pioneer L-shaped strainmeter and the more advanced LILA-Horizon triangular interferometer. Because the detection frequency is so low, LILA requires only the Moon's precession around the Earth and Sun to triangulate (unlike Earth-based detectors). Thus, the science return of LILA is site-agnostic; however, significant constraints are imposed by practical considerations. These include the need for isolation from anthropogenic noise, protection from the lunar environment, accessibility for lunar terrain vehicles, and line-of-sight. Candidate sites are shown for both LILA-Pioneer and LILA-Horizon, demonstrating that many options exist for deployment of both tools.