Abstract
We propose a gravitational wave detector that uses two superluminal lasers. Compared to the Advanced LIGO detector, the range for detecting binary neutron star inspirals is enhanced by a factor of 19 using this scheme.
| Original language | English (US) |
|---|---|
| Title of host publication | CLEO |
| Subtitle of host publication | Applications and Technology, CLEO_AT 2019 |
| Publisher | Optica Publishing Group (formerly OSA) |
| ISBN (Print) | 9781943580576 |
| DOIs | |
| State | Published - 2019 |
| Event | CLEO: Applications and Technology, CLEO_AT 2019 - San Jose, United States Duration: May 5 2019 → May 10 2019 |
Publication series
| Name | Optics InfoBase Conference Papers |
|---|---|
| Volume | Part F127-CLEO_AT 2019 |
| ISSN (Electronic) | 2162-2701 |
Conference
| Conference | CLEO: Applications and Technology, CLEO_AT 2019 |
|---|---|
| Country/Territory | United States |
| City | San Jose |
| Period | 5/5/19 → 5/10/19 |
Funding
intracavity power of the superluminal laser is 10W. This work was supported by AFOSR under Grants No. FA9550-18-01-0401 and FA9550-18-P-0003.
ASJC Scopus subject areas
- Electronic, Optical and Magnetic Materials
- Mechanics of Materials