Gravitational Wave Detection with Atom Interferometry

Dimopoulos, Savas ; /Stanford U., Phys. Dept. ; Graham, Peter W. ; /SLAC /Stanford U., Phys. Dept. ; Hogan, Jason M. ; Kasevich, Mark A. ; /Stanford U., Phys. Dept. ; Rajendran, Surjeet ; /SLAC /Stanford U., Phys. Dept.

关键词: ATOMS;    DETECTION;    GRAVITATIONAL WAVE DETECTORS;    GRAVITATIONAL WAVES;    INTERFEROMETERS;    INTERFEROMETRY;    SENSITIVITY;    DESIGN;    PERFORMANCE Gravitation and Cosmology;    GRQC;   

DOI  :  10.2172/922600
RP-ID  :  SLAC-PUB-13076
PID  :  OSTI ID: 922600
Others  :  Other: arXiv:0712.1250
Others  :  TRN: US200806%%69

学科分类：物理（综合）

美国|英语

来源: SciTech Connect

【 摘 要 】

We propose two distinct atom interferometer gravitational wave detectors, one terrestrial and another satellite-based, utilizing the core technology of the Stanford 10m atom interferometer presently under construction. The terrestrial experiment can operate with strain sensitivity {approx} 10{sup -19}/{radical}Hz in the 1 Hz-10 Hz band, inaccessible to LIGO, and can detect gravitational waves from solar mass binaries out to megaparsec distances. The satellite experiment probes the same frequency spectrum as LISA with better strain sensitivity {approx} 10{sup -20}/{radical}Hz. Each configuration compares two widely separated atom interferometers run using common lasers. The effect of the gravitational waves on the propagating laser field produces the main effect in this configuration and enables a large enhancement in the gravitational wave signal while significantly suppressing many backgrounds. The use of ballistic atoms (instead of mirrors) as inertial test masses improves systematics coming from vibrations and acceleration noise, and reduces spacecraft control requirements.