Séminaire du GDR QCD – 12/12/2024

 

 

 

A new type of gravitational-wave detection of low-frequency based on pulsars has revealed as signal that is so far not well described by standard astrophysical explanations as super-massive black holes. If the signal is interpreted as a signal of a first order transition from the early universe, it points to the temperature range of the QGP-hadron transition.

 

References: https://arxiv.org/abs/2306.16219 & https://arxiv.org/pdf/2306.16214

 

Indico: https://indico.in2p3.fr/event/34818/