NewFunFiCO mid term meeting
The NewFunFiCO mid term meeting took place online on March 20 bringing together many consortium members, to share their experiences with the REA.
The NewFunFiCO mid term meeting took place online on March 20 bringing together many consortium members, to share their experiences with the REA.
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.
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.
Nuno M. Santos successfullly defended his Ph.D. thesis on January 10 2025. The defense was online and the degree awarded with distinction from IST-Lisbon. Well done Nuno and all the best for what comes next!
The XVII black holes workshop took place at the University of Aveiro, from 19-20 December 2024. Over 70 participants got involved into two intense days of seminars and discussions on this growing and fascinating research topic. See you all in Lisbon in 2025! UA coverage here.
Gr@v co-authored the article in the journal Computers in Biology and Medicine, with title “Next-generation chemotherapy treatments based on black hole algorithms: From cancer remission to chronic disease management”. This is an interdisciplinary research applying ideas from black hole physics to create a new methodology in chemotherapy treatments. See here the UA coverage.
In this talk, I will discuss the freeze-in dark matter production mechanism at low reheating temperatures. The process is Boltzmann-suppressed if the dark matter mass is above the reheating temperature, and, in this case, the coupling to the thermal bath has to be significant to account for the observed dark matter relic density.