Superluminal laser gravitational wave detector

Minchuan Zhou, Zifan Zhou, Selim M. Shahriar*

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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 languageEnglish (US)
Title of host publicationCLEO
Subtitle of host publicationApplications and Technology, CLEO_AT 2019
PublisherOptica Publishing Group (formerly OSA)
ISBN (Print)9781943580576
DOIs
StatePublished - 2019
EventCLEO: Applications and Technology, CLEO_AT 2019 - San Jose, United States
Duration: May 5 2019May 10 2019

Publication series

NameOptics InfoBase Conference Papers
VolumePart F127-CLEO_AT 2019
ISSN (Electronic)2162-2701

Conference

ConferenceCLEO: Applications and Technology, CLEO_AT 2019
Country/TerritoryUnited States
CitySan Jose
Period5/5/195/10/19

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

Fingerprint

Dive into the research topics of 'Superluminal laser gravitational wave detector'. Together they form a unique fingerprint.

Cite this