Sep 14 2017 - De 12:00 hasta 14:00 Aitor Landete D-branes, axion monodromy and large-field inflation
This thesis explores different realizations of large-field inflation in type II string theory compactifications, in presence of the open-string sector, within the context of axion monodromy.
Sep 13 2017 - De 12:00 hasta 13:00 Sara Saa The Higgs as a pseudo-Goldstone boson

This thesis explores the possibility that the Higgs particle may have a pseudo-Goldstone boson origin.

Sep 8 2017 - De 12:00 hasta 13:00 Ana Isabel Salvador Counts-in-Cells with the Dark Energy Survey

We use the Counts-in-Cells (CiC) method to obtain the galaxy bias. CiC is a method based on dividing the sphere in cells of the same volume and counting the number of galaxies in each cell.

Jul 28 2017 - De 10:00 hasta 11:00 Sandra Robles The naturalness criterion for supersymmetric scenarios

Supersymmetry (SUSY) has been considered since long ago the leading paradigm of beyond the Standard

Abr 19 2017 - De 12:00 hasta 14:00 Emilia da Silva Holographic Revivals
Dic 16 2016 - De 12:30 hasta 14:30 Víctor Martín Lozano Collider Phenomenology of Dark Matter Models
Sep 15 2016 - De 12:00 hasta 14:00 Miguel Montero Muñoz Gauge symmetries in Quantum Gravity and String Theory

This thesis explores the spectrum of states charged under global and gauge symmetries in String Theory, and the constraints that they pose on specific phenomenological models.

Jun 24 2016 - De 12:00 hasta 14:00 Ilaria Brivio Hunting a dynamical Higgs

Particle physics is at the dawn of a new era: the discovery of the Higgs boson
in 2012 marked a turning point, confirming, on one hand, the particle content of

Jun 14 2016 - De 12:00 hasta 14:00 Santiago Ávila Large Scale Structure of the Universe: from Simulations to Observations
Jun 14 2016 - De 10:00 hasta 14:00 Ander Retolaza Applications of toric Calabi-Yau singularities to Cosmological model building in String Theory

String Theory is nowadays the best candidate to describe gravity at the quantum level together with the other interactions and matter fields.