Title seminar: Modified gravity, generalized SU(2) Proca theory, and inflation
Speaker: Yeinzon Rodríguez García
Title seminar: Modified gravity, generalized SU(2) Proca theory, and inflation
Speaker: Yeinzon Rodríguez García
Hoy, al entrar en el Edificio Trilingüe de la Facultad de Ciencias de la Universidad de Salamanca nos hemos encontrado con una sorpresa:
Esta semana tendremos un coloquio un tanto especial, que además será el último de este curso académico.Este viernes 14 de junio a las 12.30 horas se celebra un nuevo Seminario en el
Salón de Actos del IRNASA-CSIC (C/Cordel de Merinas s/n),
con acceso libre y gratuito hasta completar aforo,
a cargo del profesor de la Universidad de Santiago de Compostela Dr. Remigio Paradelo.
También será emitido en streaming a través del siguiente enlace: https://www.youtube.com/live/leQjumn73eo?si=sxRHuX6HoEDbgxFhA
This is the first announcement of the eight IUFFyM colloquium of the season next Thursday, June 13th
“Transporte dinámico en el efecto Hall cuántico”
C. Altimiras
SPEC, Université Paris-Saclay
Before the colloquium (12:30 – 13:00), some coffee and snacks will be offered as usual next to the pendulum to encourage the participation.
Speaker: Fernando Buitrago (Universidad de Valladolid)Title: Why do galaxy sizes matter?
Abstract: During the last decades, galaxy sizes have been a very active research topic in Astrophysics given the fact that they are one of the few direct observables from objects in the distant Universe. In this seminar, I will review the different approaches that were traditionally taken, showing what we have learned about how our Universe works over time. However, galaxies are fuzzy objects, and as such it is very hard to assign sizes to them. One would naively think that by observing for larger integration times and/or by using better telescopes these objects will grow bigger and bigger. I will prove you wrong by describing a novel physically-motivated size proxy (the galaxy edges or galaxy truncations) that my team GEELSBE (Galactic Edges and Euclid in the Low Surface Brightness Era) at the University of Valladolid is studying. We have utilized the deepest pointings of the Hubble Space Telescope (while now using the James Webb Space Telescope and Machine Learning algorithms) to obtain the evolution of this parameter last 8 Gyr promising to give us first hand information not only about the baryonic mass assembly but also the dark matter halo evolution.
Date and time: Wednesday, June 05, (13:00)
Room: Aula V, Edificio Trilingüe, Facultad de Ciencias, Universidad de Salamanca
El siguiente encuentro de “de rerum natura” será este jueves 30 de mayo.
Os recordamos que tendrá lugar en el bar La Vegatería (C. Gütenberg, 13) a las 20:00h.


