Come join us at @GRAPPAinstitute!
Keep an eye on https://t.co/pp6Ol2hgDV for open PhD, Postdoc and Tenure-Track positions at @GRAPPAinstitute (as well as related positions at @uva_api).
On the 19th of May 2025, I successfully defended my thesis and was awarded my doctorate.
It's an honour to be surrounded by leaders across domains in physics.
Thank you to my advisors @samayanissanke@PhilippMoesta@C_Weniger for everything ❤️.
#academia#AcademicTwitter#PhD
Applying it to the case of dark matter (DM) spikes around massive black holes (BHs), they show that a fully relativistic treatment is needed to accurately model the environmental dephasing of gravitational wave (GW) signals from EMRIs
New GRAPPA paper! https://t.co/bMoFZMvRw0 The authors (Rodrigo Vicente, Theophanes Karydas, @gfbertone) introduce a relativistic framework to model environmental effects on extreme mass-ratio inspirals (EMRIs) in collisionless media
Today we had a fantastic Colloquium by Dr. Malcolm Fairbairn (@KingsCollegeLon) to tell us about "Galaxies, Axions, Gravitational Waves, Black Holes and More Galaxies"
It's a real pleasure to have Dr. Jonathan Gair (@mpi_grav) giving the GRAPPA Colloquium today, to tell us about "Opportunities and challenges in SBI for future gravitational wave detectors"
We had a busy & wonderful day @GRAPPAinstitute yesterday with 2 PhD defences! Huge congratulations to Dr Montel @AnauNoemi & Dr Tomaselli on their brilliant theses & defences. Such an honour to be on your defence committees. We are so proud of you & wish you the..
It was fantastic having you the last 4 years at the Institute, you have been a key part of GRAPPA and we will certainly miss you! We wish you all the best for the future 🎉
Huge congratulations to Dr Tomaselli for a brilliant PhD defence and beautiful thesis, with cum laude & many congratulations to the proud supervisors Gianfranco Bertone @DD_Baumann@GRAPPAinstitute
The method relies on the assumption that the multi-million dimensional posterior of cosmic ICs can be described by a simple Gaussian, where the mean and covariance have been trained on the Quijote N-body simulations suite
Owing to its simplicity, the method is significantly faster than other proposed algorithms (training only takes ~1h on a GPU, and sampling just ~3s for 1000 samples), while still being highly precise and interpretable
Paper alert!
The authors introduce a fast and accurate method to reconstruct the cosmological initial conditions from present-day dark matter density fields, including uncertainty quantification!
https://t.co/QBSjpJaMbT
Led by GRAPPA PhD Oleg Savchenko
PBS Space Time has picked up a PRX paper by current and former GRAPPA members. Huge congrats to Dion Noordhuis, Anirudh Prabhu, Sam Witte and @C_Weniger for the fantastic piece of work!
https://t.co/mZBuAstF94
All active #NeutronStars should be surrounded by dense #AxionClouds if the axion has a mass in a specific range. This occurs because the polar caps of neutron stars produce axion clouds that are bound to the star and struggle to dissipate energy.
🔗 https://t.co/rg07BTA8xB