University of Birmingham > Talks@bham > Astrophysics Talks Series > Pushing the low and high-frequency detector sensitivity (below 10 and above 1kHz)

  Browse A-Z

Log in

System Admin (disabled)details Birmingham usersdetails No account?details

Information on

Subscribing to talksdetails Finding a talkdetails Adding a talkdetails Disseminating talksdetails Help and Documentationdetails

Pushing the low and high-frequency detector sensitivity (below 10 and above 1kHz)

Add to your list(s) Download to your calendar using vCal

If you have a question about this talk, please contact Nathan Steinle.

Gravitational-wave observations across multiple frequency bands will be the future of gravitational-wave astronomy, similar to the development of electromagnetic observations. In this talk, I will focus on ground-based detectors, and talk about the efforts in improving the detector sensitivity both at the low and high-frequency end of the spectrum. I will highlight two technologies: the 6D seismometer and the quantum filter. Apart from the application to gravitational-wave detections, these two also allow us to explore quantum behaviours of macroscopic objects and new principles of high-precision measurements.

This talk is part of the Astrophysics Talks Series series.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.

Other lists

Type the title of a new list here Cond. Mat. seminar Applied Mathematics Seminar Series

Other talks

TBC Quantum simulations using ultra cold ytterbium Geometry of alternating projections in metric spaces with bounded curvature Ultrafast, all-optical, and highly efficient imaging of molecular chirality Modelling uncertainty in image analysis. Extending the Lax type operator for finite W-algebras
 

Talks@bham, University of Birmingham. Contact Us | Help and Documentation | Privacy and Publicity.
talks@bham is based on talks.cam from the University of Cambridge.