Abstract
We propose a new optical configuration for an interferometric gravitational wave detector based on the speedmeter concept using a sloshing cavity. Speedmeters provide an inherently better quantum-noise limited sensitivity at low frequencies than the currently used Michelson interferometers. We show that a practical sloshing cavity can be added relatively simply to an existing dual-recycled Michelson interferometer such as Advanced LIGO.
Original language | English |
---|---|
Article number | 025007 |
Pages (from-to) | 1-10 |
Number of pages | 10 |
Journal | Classical and Quantum Gravity |
Volume | 37 |
Issue number | 2 |
DOIs | |
Publication status | Published - 19 Dec 2019 |
Bibliographical note
6 pages, 6 figuresKeywords
- gravitational wave
- interferometry
- quantum noise