Window to high energy physics with superconducting cosmic strings

• Ivan Rybak

Room: Seminario de Física Atómica, Nuclear y Molecular

Searching for dark matter with COSINE-100

• Sophia Hollick

Room: Seminario de Física Atómica, Nuclear y Molecular

Low-mass WIMP detection with TREX-DM

• Álvaro Ezquerro Sastre

Room: Seminario de Física Atómica, Nuclear y Molecular

The Schrödinger equation is incomplete: Hamiltonian pictures of QFT in curved spacetimes

• David Martinez

Room: Seminario de Física Atómica, Nuclear y Molecular

Hunting Axions with the International Axion Observatory (IAXO)

• Julia Vogel

Room: Seminario de Física Atómica, Nuclear y Molecular

Detecting axions from monster stars

• Maurizio Giannotti

Room: Seminario de Física Atómica, Nuclear y Molecular

ANAIS-112: updated results on annual modulation with three-year exposure and future prospects

• Tamara Pardo

Room: Seminario de Física Atómica, Nuclear y Molecular

Light new physics coupling to tau leptons

• Jorge Alda

Room: Seminario de Física Atómica, Nuclear y Molecular

Time-domain astrophysics at the Observatorio Astrofísico de Javalambre

• Alessandro Ederoclite

Room: Seminario de Física Atómica, Nuclear y Molecular

Vacuum energy in a spherical \delta-\delta' geometry

• Inés Cavero

Room: Seminario de Física Atómica, Nuclear y Molecular

Detecting (high frequency) gravitational waves in a box

• Diego Blas

Room: Seminario de Física Atómica, Nuclear y Molecular 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.

Relative locality in curved spacetimes

• Javier Relancio

Room: Seminario de Física Atómica, Nuclear y Molecular