The Beam Dump eXperiment is a state of the art, modern beam dump experiment approved by JLab PAC with maximum scientific rate. BDX aims to detect light dark matter particles in the interaction of the intense 11 GeV CEBAF electron beam with the dump of experimental Hall-A. In this contribution I will show the genesis of the experiment and its evolution  toward a pilot run we just concluded at Jlab (BDX-MINI). The physics case, as well as the experimental technique (simulation framework, detector design and prototyping), will be review and discussed.
 

Many astrophysical observations as well as anomalies in processes involving electromagnetic currents (e.g. the muon anomalous magnetic moment) could be reconciled assuming the existence of a new kind of matter, not directly interacting with light, called Dark Matter (DM). While gravitational effects of DM are quite well established, despite the tremendous efforts being devoted to reveal the nature of DM in terms of new elementary particles, no clear results have been obtained so far. Many experimental efforts are dedicated to direct detection of galactic DM, as well as to study the indirect effects of its presence. Due to the lack of results by ‘traditional’ DM searches, in the last few years the experimental activity extended to search for hints of DM produced at accelerators. Technological advances allow nowadays running high intensity  beams of moderate energy well suited for these studies. According to some theories beyond the Standard Model (SM) Light Dark Matter (LDM ) (1-1000 MeV) can interact with SM matter via a new force, mediated by a heavy vector boson called A’ or ‘heavy photon’. Depending on the relative masses of the A’ and the DM particles, the A’ can decay to SM particles (‘visible’ decay) and/or to light DM states (‘invisible’ decay). In this talk, I will give an overview of the LDM physics, focusing on the current experimental effort in the field.
 

We will discuss some newly found solutions to the full massless semiclassical Einstein equation (SCE) in a cosmological setting (Λ=0).

After a short introduction to the relevant notions we present the SCE in a particular shape which allows for the construction of a Minkowski-vacuum-like states. In this setting, solving the SCE breaks down into solving a certain ODE which can be approached numerically and, at least generically, we obtain solutions that well fit physical expectations. Moreover, these solutions indicate dark energy as a quantum effect on cosmological metrics and, since in our model m=Λ=0, this may not be traced back to the usual, obvious dark-energy/cosmological constant effect of a quantum field. Also we will shortly discuss some more physical problems that can be solved by our model. To close the talk, we will briefly speak about de Sitter solutions of the model and thereby foreshadow another talk taking place at the University of Genova later in the week.

In this talk I will give a description of the boundary structure of 3 + 1-dimensional gravity (in the Palatini–Cartan formalism) coupled to to gauge (Yang–Mills) and matter (scalar and spinorial) fields through the use of the Kijowski–Tulczijew construction. In particular, the reduced phase space is obtained as the reduction of a symplectic space by some first class constraints. Furthermore, if time permits I will give a cohomological description (BFV) of it. This is a joint work with A. S. Cattaneo and F. Fila-Robattino.

In this set of lectures we consider the different types of interpretations that have been considered for physical theories in general, and sketch out a variety of interpretations of quantum mechanics and their problems, including “textbook” quantum mechanics, issues of local causality and signal locality, Copenhagen quantum mechanics, operationalist quantum mechanics, some issues with hidden variable theories in general, Bohm-deBroglie quantum mechanics, consistent histories quantum mechanics, many worlds quantum mechanics, Qbism, and perhaps a few more (or a few less!) as time permits. 

Material science and quantum chemistry, among other fields, have shown the hard way that our capacity to solve quantum mechanical problems is severely limited. Exact solutions with 10²³ particles are out of the question, approximate analytical solutions are hard to find and control and numerical approaches suffer from the inherent limitation of representing a quantum problem on a classical computer. In the last two decades or so, the idea of doing quantum simulations, namely finding quantum systems that can solve specific problems has gained considerable traction due to progress in cold atomic gases and in material science. In this talk, the challenges in this field will be reviewed, starting from the reasons why we need such quantum simulators, and then giving several examples in cold atomic gases and condensed matter of realised quantum simulators and the problems that they allowed to tackle.

Photovoltaic solar energy is one of the most important technologies to decarbonize the energy sector. In many regions of the planet, solar energy is the cheapest way to generate electricity.
In this talk, I will first introduce perovskite/silicon tandem solar cells, which allow to overcome the efficiency limit of market -dominant silicon cells with a theoretical limit of 29.4% power conversion efficiency (PCE). Then, I will discuss how photonic concepts were implement ed to reach 29.8% PCE at Helmholtz-Zentrum Berlin. In the second part of my talk, I will discuss why energy yield calculations are important and how modelling can be used for accurate energy-yield modelling.

Over the past 60 years, the formidable task of measuring the complex structure of coherent light has remained elusive. Fortunately, the last decade has seen the rise of a completely novel class of techniques based on computational imaging. These methods represent a paradigm shift away from experimental hardware toward sophisticated computer algorithms. In doing so, computational optics is paving theway to a new generation of high dimensional metrologies, finally providing a route to measure the most extreme events humans can create. This talk will detail the development of single-pulse, broadband computational metrologies specifically designed to measure ultrafast pulses of light across the electromagnetic spectrum.

The spontaneous production of particles due to a gravitational field is one of the cornerstones of the theory of quantum fields in curved spacetime. This effect has an important role in our current understanding of the early phases of the Universe. I will introduce this phenomenon and point out the difficulties that arise when computing physical magnitudes, e.g. the stress-energy tensor.  I will show how we can overcome these issues and how to generalize this description to interacting fields, e.g., to understand the generation of matter during the reheating phase in the inflationary scenario.

The idea of the multifractals is basically contained in the large deviation theory; however, the introduction of the multifractal description in 1980s had an important role in statistical physics, chaos and disordered systems. In particular, to clarify in a rather neat way that the usual idea, coming from critical phenomena, that just few scaling exponents are relevant, is not completely correct, and an infinite set of exponents is necessary for a complete characterization of the scaling features.

In this seminar, the multifractal approach to fully developed turbulence will be discussed, in particular some nontrivial predictions for the statistical properties of the velocity gradients, the existence of an intermediate dissipative range andLagrangian statistics.