Two positions for a Researcher (with Ph.D.) are open within the project Towards Precision Tests of Ultralight Dark Matter with Gravitational Imaging Waves. Application deadline: March 13, 2025. More info in Euraxess.
Next generation of gravitational wave detectors will have the sensibility to detect potential deviations in gravitational waveforms with respect to general relativity. However, current agnostic tests are plagued by a lack of realistic deviations, making it difficult to interpret such detections with respect to specific theories.
Probing Ultralight Bosons with Binary Black Holes
Daniel Baumann, Horng Sheng Chia, Rafael A. Porto
A plausible model of inflation driven by strong gravitational wave turbulence
Sebastien Galtier (LPP), Jason Laurie, Sergey V. Nazarenko (INPHYNI)
Extreme mass-ratio inspirals into black holes surrounded by scalar clouds
Richard Brito and Shreya Shah
One of the most efficient energy sources in the universe is the matter accretion onto compact objects, such as black holes (BHs) and neutron stars (NSs). Since magnetic fields are ubiquitous everywhere, the accretion flow is expected to be magnetized in nature, where the large-scale magnetic fields inside the disks are commonly rooted either from the companion star or the interstellar medium.
A meeting of the NewFunFiCO network will take place in Valencia, from 20-22 May 2025. More information can be found here.
In the last week of January 2025 we received the visits of Profs. Luis Carlos Crispino and Kunihito Uzawa. Great to have you here!
On January 29th the group got together to celebrate the new position, as assistant professor of António Morais, at the U. Minho, and the Ph.D. thesis of Nuno M. Santos. Congratulations to both!
The CIDMA meetin 2025 took place on January 20th 2025. Our group contributed with two presentations by C. Herdeiro and R. Luna. The meeting webpage can be found here.