6 papers
Frequency & Radiative Analysis of Random Yagi-UHF/VHF Phased Array
Luis M. Bres, Luis A. Hernandez, Teviet D. Creighton
This paper investigates a phased array ground station capable of tracking multiple sources, multi-beamforming, electronic steering, easy scaling, and low cost. The project will dev…
Site selection constraints and options for LILA-Pioneer and LILA-Horizon
James Trippe, Ronald Polidan, Teviet Creighton +6
The Earth's Moon presents a uniquely advantageous environment for detecting astrophysical gravitational waves (GWs), particularly in the scientifically interesting deciHz regime. T…
Potential for Lunar Interior Science by the Gravitational-Wave Detector LILA
Mark P. Panning, Philippe Lognonné, Teviet Creighton +4
The Laser Interferometer Lunar Antenna (LILA), a concept for measuring sub-Hz gravitational waves on the Moon, would use laser strainmeters to obtain extremely sensitive strain mea…
Fundamental Noise and Gravitational-Wave Sensitivity of the Laser Interferometer Lunar Antenna (LILA)
Teviet Creighton, Philippe Lognonné, Mark P. Panning +3
The Earth's Moon presents a uniquely advantageous environment for detecting astrophysical gravitational waves (GWs) in the frequency range of millihertz to decihertz. Unlike Terres…
Laser Interferometer Lunar Antenna (LILA): Advancing the U.S. Priorities in Gravitational-wave and Lunar Science
Karan Jani, Matthew Abernathy, Emanuele Berti +30
The Laser Interferometer Lunar Antenna (LILA) is a next-generation gravitational-wave (GW) facility on the Moon. By harnessing the Moon's unique environment, LILA fills a critical…
Atmospheric Newtonian Noise May Constrain Third-Generation Gravitational-Wave Detectors
Wenhui Wang, Teviet Creighton
Advanced gravitational-wave detector designs are pushing towards lower frequencies, where certain types of noise, previously considered negligible, may come to dominate the detecto…