Date:

Saturday, May 6, 2017 - 10:30

Venue:

Martin Wood Lecture Theatre, Clarendon Laboratory

## Tabs

From action at a distance to gravitational waves

In Newtonian gravity, as in electrostatics, the force on one body depends on the current position of another. This fiction is satisfactory so long as the bodies move much more slowly than the speed of light. The force between fast-moving bodies cannot depend on the current positions because information about locations cannot travel faster than the speed of light. In fact when we suddenly move a body, there must be an expending spherical shell around the body in which the gravitational field associated with its old location morphs into the field associated with its new location. When this idea is worked up mathematically we conclude that a body communicates directly with the vacuum just around it, which communicates with the vacuum a bit further away, and so on, until eventually the second body is reached and it experiences the updates force. Action-at-a-distance has given way to coupling to a dynamical vacuum, and gravitational fields are reconfigured by waves that carry energy and momentum. Gravitational waves are a bit more complicated than electromagnetic waves (tensor rather than vector modes), and they are harder to generate because it's hard to get massive bodies moving relativistically. Not too hard for Mother Nature, however!

The birth of gravitational wave astronomy

I will review the detection of the expected ‘chirrup’ signal from a pair of merging massive black holes by the Laser Interferometer Gravitational-Wave Observatory (LIGO) on 14th September 2015, as well as subsequent experimental developments. This was both a tour-de-force of precision measurement pushing the limits of current technology and signal processing, and a pleasing confirmation of the computationally challenging solution of the nonlinear Einstein field equations governing this system.

Exploring the very early universe with gravitational waves

String theory is the leading candidate for a fundamental quantum theory of all interactions including gravity, at energies approaching the Planck scale. While laboratory experiments cannot directly test the theory, such energies were achieved in the very early universe. Thus there may well be gravitational wave signals of stringy physics – a ‘soundscape’ connected to the landscape of string vacua. The forthcoming LISA satellite & other experiments have the sensitivity to detect such signals.