riassunto2

MG11 
Talk detail
 

 Participant 

Christensen, Nelson

Institution

Carleton College - LIGO Scientific Collaboration  - Physics and Astronomy, Carleton College, 1 North College St. - Northfield - Minnesota - USA

Session

Talk

Abstract

GW1

Results from LIGO Observations

The Laser Interferometer Gravitational-wave Observatory (LIGO) detectors have reached their design sensitivity, and searches for gravitational waves are ongoing. Presented is a summary of the efforts to detect two types of signals. A stochastic background of gravitational waves can provide a look at the very early universe. Continuous wave signals from neutron stars bring valuable information on these compact objects. We describe LIGO's current efforts to detect or set limits on the magnitude of these types of signals.

 

Back to previous page