Conveners
S8
- Kwang Sik Jeong (Pusan National University)
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Peizhi Du (University of Science and Technology of China)26/08/2026, 13:30
The standard cosmological model (ΛCDM model) assumes adiabatic initial conditions for primordial density perturbations. However, many new physics scenarios can deviate from this assumption and generate isocurvature perturbations across a wide range of scales. In this talk, I will discuss how isocurvature can induce gravitational waves at second order in perturbation theory. Moreover, Pulsar...
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Sudhakantha Girmohanta (Institute for Basic Science, CTPU-PTC, Korea)26/08/2026, 14:10
The discovery of a nano-Hz stochastic gravitational wave background by Pulsar Timing Array (PTA) collaborations can be interpreted as arising from a strongly supercooled phase transition in a nearly conformal dark sector. I will present a concrete model for this phase transition, and show that the strong supercooling it requires generically dilutes any pre-existing baryon asymmetry and dark...
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