Seminars 2019/2020
CANCELED
Seminar Speaker:  Prof. Mauro Paternostro 
Venue:  Room B10A, Kane Building, UCC 
Date and Time:  2nd March 2020, 4pm 
Seminar Title:  
Abstract: Pending

24th February 2020
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Seminar Speaker:  Prof. Verònica Ahufinger 
Venue:  Room B10A, Kane Building, UCC 
Date and Time:  24th February 2020, 4pm 
Seminar Title:  Ultracold atoms carrying orbital angular momentum in lattices of rings: topology and quantum magnetism 
Abstract: In this talk, we will discuss the physics of ultracold atoms carrying Orbital Angular Momentum (OAM) in lattices of ring potentials in the singleparticle and in the Mott insulator limits. In the former limit, we find topologically protected edge states. In the latter limit, we show that the system can realize a variety of spin1/2 models, including the XYZ Heisenberg model with or without external field. In the context of topology, we study the singleparticle properties of a system formed by ultracold atoms loaded into the manifold of l=1 OAM states of an optical lattice with a diamond chain geometry [1,2]. Through a series of successive basis rotations, we show that the OAM degree of freedom induces phases in some tunneling amplitudes of the tightbinding model that are equivalent to a net flux through the plaquettes and give rise to a topologically nontrivial band structure and protected edge states. In addition, we demonstrate that the system also exhibits AharanovBohm caging. In two dimensional (2D) lattices, we also propose a realization of a 2D high order topological insulator [3]. We describe the system in terms of two decoupled lattice models, each of them displaying onedimensional edge states and zerodimensional corner states that are correlated with the topological properties of the bulk. We show that this topologically nontrivial regime can be explored in a wide range of experimentally feasible values of the parameters of the physical system. Furthermore, we propose an alternative way to characterize the secondorder topological corner states based on the computation of the Zak's phases of the bands of firstorder edge states. In the Mott insulator limit, we focus on unit filling, where each trap is occupied by a single atom and a direct mapping between the OAM and spin1/2 states can be performed [4]. We consider explicitly the dependence of the effective couplings on the geometry of the system and demonstrate that several models of interest related to a general XYZ Heisenberg model with external field can be obtained. Furthermore, we discuss how the relative strength of the effective couplings can be tuned and which phases can be explored by doing so in realistic setups. [1] G. Pelegrí, A. M. Marques, R. G. Dias, A. J. Daley, V. Ahufinger and J. Mompart, Topological edge states with ultracold atoms carrying orbital angular momentum in a diamond chain. Phys. Rev. A 99, 023612 (2019). [2] G. Pelegrí, A. M. Marques, R. G. Dias, A. J. Daley, J. Mompart and V. Ahufinger, Topological edge states and AharanovBohm caging with ultracold atoms carrying orbital angular momentum. Phys. Rev. A 99, 023613 (2019). [3] G. Pelegrí, A. M. Marques, V. Ahufinger, J. Mompart, and R. G. Dias, Secondorder topological corner states with ultracold atoms carrying orbital angular momentum in optical lattices, Phys. Rev. B. 100, 205109 (2019). [4] G. Pelegrí, J. Mompart, V. Ahufinger, A. J. Daley, Quantum magnetism with ultracold bosons carrying orbital angular momentum, Phys. Rev. A 100, 023615 (2019).

10th February 2020
Seminar Speaker:  Prof. Paul Callanan and Prof. Niall Ó' Murchadha 
Venue:  Room B10A, Kane Building, UCC 
Date and Time:  10th February 2020, 4pm 
Seminar Title:  The 2019 Nobel Prize in Physics – a review 
Abstract: The Nobel Prize in Physics 2019 was awarded "for contributions to our understanding of the evolution of the universe and Earth's place in the cosmos" with one half to James Peebles "for theoretical discoveries in physical cosmology", the other half jointly to Michel Mayor and Didier Queloz "for the discovery of an exoplanet orbiting a solartype star." 
3rd February 2020
Seminar Speaker:  Dr Emanuele Pelucchi 
Venue:  Room B10A, Kane Building, UCC 
Date and Time:  3rd February 2020, 4pm 
Seminar Title:  Quantum Dots for Quantum Informaiton Processing 
Abstract: Quantum technologies are now at the centre of an intense research effort aiming at harnessing the potential of quantum states for unconventional computing. Recent hype around quantum supremacy risks to shadow the number of important alternative technologies being researched and developed, and the broad challenges which still need addressing. In this talk we present an overlook of the recent activities of the EPN group in the field of QD sources of nonclassical light, and discuss key challenges/ direction/ perspectives [13] 
18th November 2019
Seminar Speaker:  Dr H.V.J. Linnartz 
Venue:  Room B10A, Kane Building, UCC 
Date and Time:  18^{th} November 2019, 4pm 
Seminar Title:  Interstellar ice  a solid approach to molecular complexity in space 
Abstract: Chemical processes in space are completely different than those on Earth. Given the low number densities one would not expect much chemical diversity in space. Today some 225 different molecules have been identified in the interstellar medium, the highly dilute space in between stars, and it is found that icy dust grains play an important role in the formation of both rather simple and much more complex species, such as small sugars. In laboratory studies the underlying processes can be investigated. In this talk I will show how to make water under dark interstellar cloud conditions and how to link recent observations of so called COMs (complex organic molecules) on comets to solid state formation schemes triggered by atom addition reactions and upon UV excitation. 
11th November 2019
Seminar Speaker:  Steve Campbell 
Venue:  Room B10A, Kane Building, UCC 
Date and Time:  11^{th} November 2019, 4pm 
Seminar Title:  Quantum speed limits: Practical tool. Fundamental insights. 
Abstract: Uncertainty lies at the very heart of quantum mechanics. This notion is mathematically captured by the famous indeterminacy principles laid out by Heisenberg in 1927. One does not need to be a physics student to have come across the positionmomentum uncertainty principle, while less well known is the energytime (ET) formulation. A remarkable outcome from the ET uncertainty relation is the quantum speed limit, which uses the basic tenets of quantum mechanics to bound the minimal time a quantum system needs to evolve between two distinct states. In the last decades the study of the quantum speed limit has enjoyed a renewed interest partially driven by the rapid development of quantum technologies and quantum thermodynamic devices, where a minimal time sets the ultimate bounds on efficiency. Clearly then the QSL provides a practical tool for the design of optimal quantum devices. However, considering its origins, it is not surprising that recently there has been a growing interest in exploring how the quantum speed limit can provide some fundamental insights into the dynamics of quantum systems. The goal of this seminar is to introduce the basic aspects of quantum speeds limits and provide some examples of their broad utility. 
4th November 2019
Seminar Speaker:  Daniel Kennefick 
Venue:  Room B10A, Kane Building, UCC 
Date and Time:  4^{th} November 2019, 4pm 
Seminar Title:  No Shadow of Doubt: The Eclipse Expeditions of 1919 and the Irish dimension 
Abstract: This is the centenary year of the celebrated eclipse expeditions of 1919 which confirmed Einstein's theory of General Relativity. In recent decades the story of these expeditions has focused on Arthur Stanley Eddington and the question of his alleged bias in favor of Einstein’s theory. It has been alleged that Eddington threw out data which did not favor Einstein’s theory. Meticulous examination of the expeditions’ papers reveals that this view is mistaken. The relevant data was taken by the expedition organized by the Greenwich observatory and it was the director of that observatory, the Astronomer Royal, Frank Watson Dyson, who was responsible for the decisions in question. Studies of the data analysis sheets and comparison with modern reanalysis of the original plates vindicate his decision. The story of the two expeditions,is a remarkable one and this talk will examine the people, the instruments and the science of the teams and how their work changed science forever. It turns out that the key data upon which Dyson relied was taken by an Irishman, using an Irish made and owned telescope, so the Irish contribution to this famous experiment was considerable. 
21st October 2019
Seminar Speaker:  Mark Reynolds 
Venue:  Room B10A, Kane Building, UCC 
Date and Time:  21st October 2019, 4pm 
Seminar Title:  Probing the Spin Evolution of SuperMassive Black Holes at Cosmological Distances 
Abstract: Astronomical observations have demonstrated that massive black holes exist at the center of every large galaxy *and* that the mass of this black hole is correlated with a number of properties of the host galaxy, such as stellar mass. In general relativity, black holes may be described by 2 numbers: mass & spin (angular momentum). The coevolution of a supermassive black hole with its host galaxy through cosmic time will be encoded in the spin of the massive black hole. An established method of measuring the spin of black holes in the local Universe is through the study of relativistic reflection features from the inner accretion disk. At the current time, more distant sources are nominally impossible to study in such detail. However, gravitational lensing provide a means to boost our current capabilities. I will discuss work wherein we have, for the first time, directly measured the spin of cosmologically distant supermassive black holes, by taking advantage of the boost in signal provided by gravitational lensing of distant Quasars. I will show how we can use this method to begin to assemble a sample of such systems to place direct constraints on the cosmological spin evolution of supermassive black holes. 
14th October 2019
Seminar Speaker:  Mark Mitchison 
Venue:  Room B10A, Kane Building, UCC 
Date and Time:  14th October 2019, 4pm 
Seminar Title:  A spin heat engine coupled to a harmonicoscillator flywheel 
Abstract: I will present a recent realisation of a heat engine comprising a single trapped ion [1], focussing on the theoretical underpinnings of this experiment. The ion’s spin constitutes the working medium, while its quantised vibrations act as the load, or “flywheel”, which captures the output work. Characterising the flywheel’s Husimi Q function allows us to measure the mechanical work output of a heat engine with singlequantum resolution for the first time. The measurements reveal the random character of the energy transferred to the flywheel, due to unavoidable thermal fluctuations. I will explain how the ergotropy — a key quantity in quantum thermodynamics — allows us to distinguish between useful work and useless thermal energy by examining the flywheel’s quantum state. The results elucidate how fluctuations fundamentally limit engine performance at the nanoscale. [1] D. von Lindenfels et al., Phys. Rev. Lett. 123, 080602 (2019) 
7th October 2019
Seminar Speaker:  Benjamin Lingnau 
Venue:  Room B10A, Kane Building, UCC 
Date and Time:  7th October 2019, 4pm 
Seminar Title:  Nonlinear Laser Dynamics  an Introduction 
Abstract: Laser dynamics describes the state of operation where a laser's output intensity is varying in time. Initially thought of as a nuisance, laser dynamics nowadays attracts a lot of attention as an enabling technology for future applications. Whether it's ultrahighbandwidth telecommunications, highly sensitive measurement setups, or selfdriving cars, laser dynamics has found its way into modern technology. 
16th September 2019
Seminar Speaker:  Prof. Jerome V Moloney 
Venue:  Room B10A, Kane Building, UCC 
Date and Time:  16tg September 2019, 4pm 
Seminar Title:  Ultrafast Carrier Interactions in Semiconductors and Gases: From Modelocking in Semiconductor Disk Lasers to Kerr nonlinearity suppression in the Atmosphere 
Abstract: Semiconductor disk lasers are ideal testbeds for studying strong departures of carriers (electrons and holes) from quasiFermi distributions. Carriers, opticallypumped into high momentum states, scatter into lower momentum ones and are extracted as photons near the lasing wavelength. High peak intensity femtosecond duration pulses burn deep kinetic holes in the carrier distributions – the latter are replenished through kinetic hole filling and subsequently cool (via phonons) to the lattice temperature. In the extreme NLO limit, where the field coupling dominates the Coulomb potential, ultrashort pulses highly detuned from the semiconductor bandgap can expose dominant intraband interactions that can accelerate carriers across the full Brillouin zone (Bloch oscillations) and enhance harmonic generation relative to purely interband processes. Recent experiments with strong THz driving fields dramatically support this observation. Finally, in the intermediate limit of highly detuned USP interactions in gases, the effective Coulomb interaction being an order of magnitude stronger than in a semiconductor, can enhance manybody interactions between electrons transiently driven from individual nuclei. The latter disrupts the phase coherence of the induced polarization leading to a residual population of electrons in continuum states at intensities well below the tunnel ionization limit. A key consequence, is the prediction that multiJoule 10µm ps pulses can be confined over multiple kilometer ranges in the atmosphere. In my talk, I will attempt to pull these apparently diverse phenomena together and illustrate with recent experiments that support them. 