LISA and the electroweak phase transition

Description of the granted funding

The two greatest discoveries of physics so far this century were quite possibly finding the Higgs boson, and directly observing gravitational waves for the first time. The attention of particle physicists is now turning to what lies beyond the Higgs, while cosmologists and astrophysicists wonder what other sources of gravitational waves are out there. My project connects these two questions by investigating cosmological sources of gravitational waves, which have longer wavelengths than we can detect on Earth. In 2034 a space-based gravitational wave detector called LISA will be launched, which might be able to see gravitational waves produced around the time the Higgs boson itself 'turned on' – depending on exactly how that happened. I will use computer simulations both to predict which models of physics allow the 'turning on' of the Higgs boson to produce gravitational waves that LISA can see, and also to understand the characteristics of the resulting gravitational waves.
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Starting year

2019

End year

2024

Granted funding

David Weir Orcid -palvelun logo
438 874 €

David J Weir Orcid -palvelun logo
438 874 €

Related funding decisions

353131
Research costs of Academy Research Fellows(2022)
159 714 €
328958
Research costs of Academy Research Fellows(2019)
208 873 €

Funder

Research Council of Finland

Funding instrument

Academy research fellows

Other information

Funding decision number

324882

Fields of science

Physical sciences

Research fields

Hiukkas- ja ydinfysiikka

Identified topics

space, physics