<?xml version="1.0" encoding="UTF-8"?>
<feed xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns="http://www.w3.org/2005/Atom">
<title>Physics</title>
<link href="http://hdl.handle.net/10468/224" rel="alternate"/>
<subtitle/>
<id>http://hdl.handle.net/10468/224</id>
<updated>2013-05-22T10:02:49Z</updated>
<dc:date>2013-05-22T10:02:49Z</dc:date>
<entry>
<title>Typical tropospheric aerosol backscatter profiles for Southern Ireland: The Cork Raman lidar</title>
<link href="http://hdl.handle.net/10468/887" rel="alternate"/>
<author>
<name>McAuliffe, Michael A. P.</name>
</author>
<author>
<name>Ruth, Albert A.</name>
</author>
<id>http://hdl.handle.net/10468/887</id>
<updated>2013-03-08T03:02:22Z</updated>
<published>2013-02-01T00:00:00Z</published>
<summary type="text">Typical tropospheric aerosol backscatter profiles for Southern Ireland: The Cork Raman lidar
McAuliffe, Michael A. P.; Ruth, Albert A.
A Raman lidar instrument (UCLID) was established at the University College Cork as part of the European lidar network EARLINET. Raman backscatter coefficients, extinction coefficients and lidar ratios were measured within the period 28/08/2010 and 24/04/2011. Typical atmospheric scenarios over Southern Ireland in terms of the aerosol load in the planetary boundary layer are outlined. The lidar ratios found are typical for marine atmospheric condition (lidar ratio ca. 20–25 sr). The height of the planetary boundary layer is below 1000 m and therefore low in comparison to heights found at other lidar sites in Europe. On the 21st of April a large aerosol load was detected, which was assigned to a Saharan dust event based on HYSPLIT trajectories and DREAM forecasts along with the lidar ratio (70 sr) for the period concerned. The dust was found at two heights, pure dust at 2.5 km and dust mixing with pollution from 0.7 to 1.8 km with a lidar ratio of 40–50 sr.
</summary>
<dc:date>2013-02-01T00:00:00Z</dc:date>
</entry>
<entry>
<title>Quantum behavior in mesoscopic systems</title>
<link href="http://hdl.handle.net/10468/964" rel="alternate"/>
<author>
<name>Lo Gullo, Nicolino</name>
</author>
<id>http://hdl.handle.net/10468/964</id>
<updated>2013-03-26T03:09:09Z</updated>
<published>2013-01-01T00:00:00Z</published>
<summary type="text">Quantum behavior in mesoscopic systems
Lo Gullo, Nicolino
In this thesis I present the work done during my PhD. The Thesis is divided into two parts; in the first one I present the study of mesoscopic quantum systems whereas in the second one I address the problem of the definition of Markov regime for quantum system dynamics. The first work presented is the study of vortex patterns in (quasi) two dimensional rotating Bose Einstein condensates (BECs). I consider the case of an anisotropy trapping potential and I shall show that the ground state of the system hosts vortex patterns that are unstable. In a second work I designed an experimental scheme to transfer entanglement from two entangled photons to two BECs. This work is meant to propose a feasible experimental set up to bring entanglement from microscopic to macroscopic systems for both the study of fundamental questions (quantum to classical transition) and technological applications. In the last work of the first part another experimental scheme is presented in order to detect coherences of a mechanical oscillator which is assumed to have been previously cooled down to the quantum regime. In this regime in fact the system can rapidly undergo decoherence so that new techniques have to be employed in order to detect and manipulate their states. In the scheme I propose a micro-mechanical oscillator is coupled to a BEC and the detection is performed by monitoring the BEC with a negligible back-action on the cantilever. In the second part of the thesis I give a definition of Markov regime for open quantum dynamics. The importance of such definition comes from both the mathematical description of the system dynamics and from the understanding of the role played by the environment in the evolution of an open system. In the Markov regime the mathematical description can be simplified and the role of the environment is a passive one.
</summary>
<dc:date>2013-01-01T00:00:00Z</dc:date>
</entry>
<entry>
<title>Intercomparison of NO3 radical detection instruments in the atmosphere simulation chamber SAPHIR</title>
<link href="http://hdl.handle.net/10468/958" rel="alternate"/>
<author>
<name>Dorn, H.-P.</name>
</author>
<author>
<name>Apodaca, R. L.</name>
</author>
<author>
<name>Ball, S. M.</name>
</author>
<author>
<name>Brauers, T.</name>
</author>
<author>
<name>Brown, S. S.</name>
</author>
<author>
<name>Crowley, J. N.</name>
</author>
<author>
<name>Dubé, W. P.</name>
</author>
<author>
<name>Fuchs, H.</name>
</author>
<author>
<name>Häseler, R.</name>
</author>
<author>
<name>Heitmann, U.</name>
</author>
<author>
<name>Jones, R. L.</name>
</author>
<author>
<name>Kiendler-Scharr, A.</name>
</author>
<author>
<name>Labazan, I.</name>
</author>
<author>
<name>Langridge, J. M.</name>
</author>
<author>
<name>Meinen, J.</name>
</author>
<author>
<name>Mentel, T. F.</name>
</author>
<author>
<name>Platt, U.</name>
</author>
<author>
<name>Pöhler, D.</name>
</author>
<author>
<name>Rohrer, F.</name>
</author>
<author>
<name>Ruth, Albert A.</name>
</author>
<author>
<name>Schlosser, E.</name>
</author>
<author>
<name>Schuster, G</name>
</author>
<author>
<name>Shillings, A. J. L.</name>
</author>
<author>
<name>Simpson, W. R.</name>
</author>
<author>
<name>Thieser, J.</name>
</author>
<author>
<name>Tillmann, R.</name>
</author>
<author>
<name>Varma, R.</name>
</author>
<author>
<name>Venables, Dean S.</name>
</author>
<author>
<name>Wahner, A.</name>
</author>
<id>http://hdl.handle.net/10468/958</id>
<updated>2013-05-07T16:20:06Z</updated>
<published>2013-01-01T00:00:00Z</published>
<summary type="text">Intercomparison of NO3 radical detection instruments in the atmosphere simulation chamber SAPHIR
Dorn, H.-P.; Apodaca, R. L.; Ball, S. M.; Brauers, T.; Brown, S. S.; Crowley, J. N.; Dubé, W. P.; Fuchs, H.; Häseler, R.; Heitmann, U.; Jones, R. L.; Kiendler-Scharr, A.; Labazan, I.; Langridge, J. M.; Meinen, J.; Mentel, T. F.; Platt, U.; Pöhler, D.; Rohrer, F.; Ruth, Albert A.; Schlosser, E.; Schuster, G; Shillings, A. J. L.; Simpson, W. R.; Thieser, J.; Tillmann, R.; Varma, R.; Venables, Dean S.; Wahner, A.
The detection of atmospheric NO3 radicals is still challenging owing to its low mixing ratios (≈ 1 to 300 pptv) in the troposphere. While long-path differential optical absorption spectroscopy (DOAS) is a well established NO3 detection approach for over 25 yr, newly sensitive techniques have been developed in the past decade. This publication outlines the results of the first comprehensive intercomparison of seven instruments developed for the spectroscopic detection of tropospheric NO3. Four instruments were based on cavity ring-down spectroscopy (CRDS), two utilised open-path cavity enhanced absorption spectroscopy (CEAS), and one applied "classical" long-path DOAS. The intercomparison campaign "NO3Comp" was held at the atmosphere simulation chamber SAPHIR in Jülich (Germany) in June 2007. Twelve experiments were performed in the well mixed chamber for variable concentrations of NO3, N2O5, NO2, hydrocarbons, and water vapour, in the absence and in the presence of inorganic or organic aerosol. The overall precision of the cavity instruments varied between 0.5 and 5 pptv for integration times of 1 s to 5 min; that of the DOAS instrument was 9 pptv for an acquisition time of 1 min. The NO3 data of all instruments correlated excellently with the NOAA-CRDS instrument, which was selected as the common reference because of its superb sensitivity, high time resolution, and most comprehensive data coverage. The median of the coefficient of determination (r2) over all experiments of the campaign (60 correlations) is r2 = 0.981 (25th/75th percentiles: 0.949/0.994; min/max: 0.540/0.999). The linear regression analysis of the campaign data set yielded very small intercepts (1.2 ± 5.3 pptv) and the average slope of the regression lines was close to unity (1.02, min: 0.72, max: 1.36). The deviation of individual regression slopes from unity was always within the combined accuracies of each instrument pair. The very good correspondence between the NO3 measurements by all instruments for aerosol-free experiments indicates that the losses of NO3 in the inlet of the instruments were determined reliably by the participants for the corresponding conditions. In the presence of inorganic or organic aerosol, however, differences in the measured NO3 mixing ratios were detectable among the instruments. In individual experiments the discrepancies increased with time, pointing to additional NO3 radical losses by aerosol deposited onto the inlet walls of the instruments. Instruments using DOAS analyses showed no significant effect of aerosol on the detection of NO3. No hint of a cross interference of NO2 was found. The effect of non-Lambert–Beer behaviour of water vapour absorption lines on the accuracy of the NO3 detection by broadband techniques was small and well controlled. The NO3Comp campaign demonstrated the high quality, reliability and robustness of performance of current state-of-the-art instrumentation for NO3 detection.
</summary>
<dc:date>2013-01-01T00:00:00Z</dc:date>
</entry>
<entry>
<title>Spatial and energetic mode dynamics of cold atomic systems</title>
<link href="http://hdl.handle.net/10468/963" rel="alternate"/>
<author>
<name>O'Sullivan, Brian</name>
</author>
<id>http://hdl.handle.net/10468/963</id>
<updated>2013-03-26T03:09:07Z</updated>
<published>2012-12-01T00:00:00Z</published>
<summary type="text">Spatial and energetic mode dynamics of cold atomic systems
O'Sullivan, Brian
In this thesis we relate the formal description of various cold atomic systems in the&#13;
energy eigenbasis, to the observable spatial mode dynamics. Herein the `spatial mode&#13;
dynamics' refers to the direction of photon emission following the spontaneous emission&#13;
of an excited fermion in the presence of a same species and spin ideal anisotropic Fermi&#13;
sea in its internal ground state. Due to the Pauli principle, the presence of the ground&#13;
state Fermi sea renders the phase space, anisotropic and only partially accessible, thereby&#13;
a ecting the direction of photon emission following spontaneous emission.&#13;
The spatial and energetic mode dynamics also refers to the quantum `tunneling' interaction&#13;
between localised spatial modes, synonymous with double well type potentials.&#13;
Here we relate the dynamics of the wavefunction in both the energetic and spatial representations.&#13;
Using this approach we approximate the relationship between the spatial&#13;
and energetic representations of a wavefunction spanning three spatial and energetic&#13;
modes. This is extended to a process known as Spatial Adiabatic Passage, which is a&#13;
technique to transport matter waves between localised spatial modes. This approach&#13;
allows us to interpret the transport of matter waves as a signature of a geometric phase&#13;
acquired by the one of the internal energy eigenstates of the system during the cyclical&#13;
evolution. We further show that this geometric phase may be used to create spatial&#13;
mode qubit and qutrit states.
</summary>
<dc:date>2012-12-01T00:00:00Z</dc:date>
</entry>
</feed>
