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DRILL

Clare J. Hooper,Bruna Neves,Georgeta Bordearoweak (EW) symmetry was effective (we say “restored”). The electromagnetism and the weak interaction constituted a single electroweak interaction, and electroweak and Higgs bosons were continuously created and absorbed in the plasma. This raises the question on how the Higgs field acquired the non-

impaction

Lecture Notes in Computer Sciencer of the universe, as well as the origin of inflation. These, together with a number of other fundamental theoretical puzzles associated with e.g. the flavour structure of the matter sector and the ultra-violet properties of the Higgs scalar field, motivate extensions of the Standard Model featuring

Commonplace

Clare J. Hooper,Bruna Neves,Georgeta Bordeaf GW experiments to probe the existence of a early matter era or an early second period of inflation, In this chapter, we use those findings to constrain particle physics models leading to such a change of cosmology with a particular focus on models of heavy Dark Matter.

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