Abstract
Particle Physics and Gravitational Waves as complementary windows on the Universe
Particle physics and gravitational waves provide complementary probes of the deep structure of the Universe. Gravitational waves from the mergers of neutron stars and black holes are sensitive to the structure of dense quark matter (GSI/FAIR related physics) and to different dark matter scenarios. Measurements of stochastic gravitational waves backgrounds can teach us about possible first order phase transitions in the early Universe, including providing sensitivity to the TeV scale which is of key interest to future particle collider experiments. Gravitational waves measurements will also give new probes of the evolution and expansion of the Universe, complementary to measurements with electromagnetic radiation. This seminar explores the physics synergies between the science opportunities provided by next generation gravitational waves measurements and particle physics experiments in the next decade and beyond when GSI/FAIR, HL-LHC, LISA and the Einstein telescope will be running timewise in parallel.
For extra details, see the Perspectives article by Steven D. Bass, Laura Baudis, Gianfranco Bertone, Oliver Buchmueller, Babette Döbrich, Reinhard Genzel, Anne M. Green, Klaus Helbing, Michèle Heurs, Karl Jakobs, Markus Klute, Samaya Nissanke, Hiranya Peiris, Albino Perego, Stefan Pokorski, Matthias Schott, Stefano Vitale, Georg Weiglein, Jochen Weller



















