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The Universe is thrumming with gravitational waves. June 2023 brought the first evidence for an all-sky background of nanohertz-frequency gravitational waves, discovered by collaborations including the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) and groups in Europe, Australia, India, and China. This was an endeavor decades in the making, requiring painstakingly precise timing observations of scores of millisecond pulsars across the Milky Way using flagship radio telescopes. While the results from separate groups are consistent with one another—and the leading interpretation of a population of supermassive black-hole binaries as the source—the observations provoke many new questions.
- Do the results imply a population of binaries more massive than expected?
- What are the observational milestones as the first resolvable binary signals come into focus?
- Can we link these signals to their host galaxies through ranking protocols and by leveraging electromagnetic counterparts?
- And will our understanding of the gravitational-wave background hit a cosmic-variance barrier?
In this talk, I will chart the path to discovery, reflect on what we have learned during our year+ since our announcement, and explore the exciting opportunities and synergies ahead—including the role of next-generation instruments radio instruments— as we move ever closer to the LISA era.
Margrethe Bohr Auditorium, Niels Bohr Building.
Coffee and cake from 14.45.
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Event Venue & Nearby Stays
Niels Bohr Bygningen, Jagtvej 128,Copenhagen, Copenhagen , Denmark
