High Precision Measurements Using an Optical Cavity
Faculty Mentor Name
Michele Zanolin, Malik Rakhmanov
Format Preference
Poster
Abstract
After the Gravitational Wave detections from both Binary Black Hole (BBH) mergers and from a Binary Neutron Star (BNS) merger, the next and most pressing Gravitational Wave signal will come from Core-Collapse Supernovae (CCSNe). In order to detect such signals, development on the laser interferometers is necessary. The aim of this research is to develop and optimize techniques specific for frequencies in the hundreds of hertz where Gravitational Waves from CCSNe contain a majority of their energy.
- POSTER PRESENTATION
- IGNITE GRANT
Location
ERAU - Prescott, AZ; AC1-Atrium, 11 am - 3 pm | Eagle Gym, 7 - 9 pm
Start Date
3-29-2019 11:00 AM
End Date
3-29-2019 9:00 PM
High Precision Measurements Using an Optical Cavity
ERAU - Prescott, AZ; AC1-Atrium, 11 am - 3 pm | Eagle Gym, 7 - 9 pm
After the Gravitational Wave detections from both Binary Black Hole (BBH) mergers and from a Binary Neutron Star (BNS) merger, the next and most pressing Gravitational Wave signal will come from Core-Collapse Supernovae (CCSNe). In order to detect such signals, development on the laser interferometers is necessary. The aim of this research is to develop and optimize techniques specific for frequencies in the hundreds of hertz where Gravitational Waves from CCSNe contain a majority of their energy.
- POSTER PRESENTATION
- IGNITE GRANT