Théorie

Stochastic formalism of cosmic inflation, with applications to the physics of primordial black holes. La soutenance HDR Vincent Vennin

Dear friends and colleagues,

It is my pleasure to invite you to my habilitation defense, which will take place on the 30th of June at 3pm. 

I will present my work on the stochastic formalism of cosmic inflation, with applications to the physics of primordial black holes (a short description follows below).

Due to the current covid-19 restrictions, unfortunately, only members of the jury will be allowed to be physically present. The defense will however be broadcasted online, via the BlackBoard Collaborate platform:

Vainshtein screening for slowly rotating stars 

We study the Vainshtein mechanism in the context of slowly rotating stars in scalar-tensor theories.
While the Vainshtein screening is well established for spherically symmetric spacetimes, we introduce a slow rotation of the source and examine its validity in the axi-symmetric case.
We solve for the frame-dragging function accounting for the slow rotation and show that the deviations from the general relativity (GR) solution are screened in the weak-field approximation, meaning the solution for the frame-dragging function is the same as GR to leading order.

Formation and abundance of primordial black holes

Primordial black holes can form in the early Universe from the collapse of cosmological perturbations after the cosmological horizon crossing. They are possible candidates for the dark matter as well as for the seeds of supermassive black holes observed today in the centre of galaxies. In calculations of spherically symmetric collapse, a Lagrangian relativistic hydrodynamical code is used to follow the non linear evolution. If the perturbation is larger than a threshold depending on the equation of state and on the specific shape of the perturbation, a black hole is formed.

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