The elements of the CKM matrix are fundamental parameters of the Standard Model. Substantial experimental and theory efforts are under way aimed at determining them ever more precisely and accurately.
Strong gravitational lensing is a powerful observational tool in astrophysics and cosmology which has been used to study the mass and light properties of galaxies and quasars the scales and distributions of dark matter subhaloes and the expansion history of the Universe.
In recent times quantum computational complexity has been a major interest to both QI and HEP communities. Complexity in the Krylov basis is one such candidate which has proved its worth in several setups by providing us with meaningful insights.
Black holes serve as natural laboratories for probing gravity under extreme conditions. New Insights in Black Hole Physics from Holography, hosted at the Instituto de Física Teórica UAM/CSIC in Madrid, will bring together leading researchers to discuss recent advances in black hole physics through the framework of holography. The workshop will cover a range of […]
I will give a brief overview of the so called flavor anomalies, describing the main strategies followed to disclose physics beyond the Standard Model. I will focus on selected modes and observables that can help identifying the nature of new physics.
Cluster cosmology is potentially one of the most powerful observational probes of structure formation. However, enabling unbiased cosmological constraints requires careful modeling of the cluster selection function. In the case of optical cluster cosmology, this requires accurate modeling of projection effects. We will introduce a new simulation-based inference framework with which we reanalyze DES Y1 […]