Talks (non-conference)

When the temperature of the universe was about 100 GeV, the electroweak phase transition took place. In this process, the electroweak symmetry broke, and the particles of the Standard Model became massive. [...]

Introduction to information retrieval for summer students including a list of selected services of the DESY library

Sound waves sourced by bubble collisions during a cosmological first order phase transition can constitute an observable gravitational wave signal. In the standard picture, the gravitational wave spectrum is described in terms of four parameters: the wall velocity and the strength, duration and temperature of the phase transition. [...]

In many extensions of the Standard Model, the electroweak phase transition is first order. Such a phase transition proceeds via the formation and collision of bubbles. [...]

In many extensions of the Standard Model, the electroweak phase transition is first order. Such a phase transition proceeds via the formation and collision of bubbles. [...]

Sound waves sourced by bubble collisions during a cosmological first order phase transition can constitute an observable gravitational wave signal. In the standard picture, the gravitational wave spectrum is described in terms of four parameters: the wall velocity and the strength, duration and temperature of the phase transition. [...]

Sound waves sourced by bubble collisions during a cosmological first order phase transition can constitute an observable gravitational wave signal. In the standard picture, the gravitational wave spectrum is described in terms of four parameters: the wall velocity and the strength, duration and temperature of the phase transition. [...]