RAS Discussion Meeting

Gravitational wave spectrum

The gravitational wave spectrum [Credit: Christopher Moore, Robert Cole and Christopher Berry

The next few years promise to be exciting ones for the field of gravitational wave astronomy: ground-based gravitational wave detectors will begin taking data at unprecedented sensitivities; pulsar timing arrays are continuing to improve their timing accuracy; and several experiments are studying the cosmic microwave background polarisation in great detail. Together, these methods are probing a huge range of the gravitational wave spectrum, and detections will offer a wealth of new information on compact binaries, supermassive black holes, and general relativity in extreme environments from the early universe to black hole mergers.

Exploiting the datasets provided by these cutting edge observations has spurred the development of novel data analysis methods to understand gravitational wave sources.

This Royal Astronomical Society discussion meeting will bring together researchers from these diverse areas to encourage the sharing of techniques and foster further collaboration within the data analysis community.

Registration:
Registration and poster abstract submission can be done on the registration page. Attendance is free for RAS members, or £15 for non-members (£5 for students; note that students can join the RAS for only £1!) to be payable on the day.

When & Where:
Friday, 12th December 2014, 10:30-15:30, followed by the Monthly A&G Meeting. Geological Society Lecture Theatre, RAS, Burlington House, London, UK.

Organisers: Matthew Pitkin (University of Glasgow), John Veitch (University of Birmingham) and Ik Siong Heng (University of Glasgow).