Saturnalia 2023

Dec 18, 2023, 9:00 AM → Dec 21, 2023, 8:00 PM Europe/Madrid

Seminario de Física Atómica, Nuclear y Molecular (Facultad de Ciencias)

Jaime Ruz (CAPA), Javier Redondo (CAPA, DPTUZ), Mathieu Kaltschmidt (Universidad de Zaragoza), Maykoll Reyes (Universidad de Zaragoza), Siannah Penaranda-Rivas (University of Zaragoza, Spain)

Conference series dedicated to catch up with the recent Theoretical and Experimental developments in the broad range of fields covered by our center CAPA,  as well as with the adventures and misfortunes of our dear young expats.

saturnalia23_poster_final.pdf

Mon, December 18

12:30 PM → 1:00 PM Window to high energy physics with superconducting cosmic strings

Speaker: Ivan Rybak

Saturnalia_2023_Rybak.pdf

1:00 PM → 1:30 PM Searching for dark matter with COSINE-100

Speaker: Sophia Hollick

Hollick_Saturnalia2023.pdf

1:30 PM → 2:00 PM Low-mass WIMP detection with TREX-DM

Speaker: Álvaro Ezquerro Sastre

TREXDM_saturnalia_2023_AEzquerro.pdf

Tue, December 19

12:30 PM → 1:00 PM The Schrödinger equation is incomplete: Hamiltonian pictures of QFT in curved spacetimes

Speaker: David Martinez

PureStates_QFT.pdf

1:00 PM → 1:30 PM Hunting Axions with the International Axion Observatory (IAXO)

Speaker: Julia Vogel

1:30 PM → 2:00 PM Detecting axions from monster stars

Speaker: Maurizio Giannotti

Monster_Star_Axions.pdf

Wed, December 20

12:30 PM → 1:00 PM ANAIS-112: updated results on annual modulation with three-year exposure and future prospects

Speaker: Tamara Pardo

TPardo_Saturnalia23.pdf

1:00 PM → 1:30 PM Light new physics coupling to tau leptons

Speaker: Jorge Alda

slides.pdf

Thu, December 21

11:30 AM → 12:00 PM Time-domain astrophysics at the Observatorio Astrofísico de Javalambre

Speaker: Alessandro Ederoclite

12:00 PM → 12:30 PM Vacuum energy in a spherical \delta-\delta' geometry

Speaker: Inés Cavero

Saturnalia_20231221.pdf

12:30 PM → 1:00 PM Detecting (high frequency) gravitational waves in a box

In the presence of a background EM field, the passage of GWs generate different modes in EM cavities by either their effect on the background field or by interacting with the boundaries of the cavity. In this talk, I will describe this process in some detail and show that these set-ups provide some of the best bounds for GWs in the MHz-GHz band. I shall finish by briefly describing the way GWs interact with spin systems.

Speaker: Diego Blas

ZGZ_Blas2.pdf

ZGZ_Blas.pdf

1:00 PM → 1:30 PM Relative locality in curved spacetimes

Speaker: Javier Relancio

Saturnalia_23_Relancio.pdf