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    <title>DSpace Collection:</title>
    <link>http://theses.ncl.ac.uk/jspui/handle/10443/5374</link>
    <description />
    <pubDate>Sat, 08 Aug 2026 06:24:11 GMT</pubDate>
    <dc:date>2026-08-08T06:24:11Z</dc:date>
    <item>
      <title>Self Interacting Fuzzy Dark Matter and its Observational Implications</title>
      <link>http://theses.ncl.ac.uk/jspui/handle/10443/6792</link>
      <description>Title: Self Interacting Fuzzy Dark Matter and its Observational Implications
Authors: Indjin, Milos
Abstract: We investigate aspects of Fuzzy Dark Matter (FDM) in both the non-interacting and repul&#xD;
sively self-interacting regimes, critically discussing the role of interactions on virialised profiles,&#xD;
using our findings to fit to galactic rotation curves of a range of dark matter dominated galax&#xD;
ies, thus proposing a way to numerically reconstruct a galaxy from analysing observational&#xD;
curves. Specifically, we firstly analyse the ground state solution of the Gross-Pitaevskii-Poisson&#xD;
equations- the soliton core. A generalised ansatz is formed along with a soliton-specific di&#xD;
mensionless interaction strength. The virial theorem is utilised to explain core dependencies&#xD;
on boson (m) and total mass, and self-interaction (g), and a degeneracy in the pairing of m&#xD;
and g is also uncovered. Moreover, we introduce a Super-Gaussian profile from empirically&#xD;
fitting to numerically generated self-interacting soliton ground states. This profile, joined with&#xD;
a Navarro-Frenk-White (NFW) halo profile, is used to fit self-interacting FDM to observational&#xD;
data of dark matter dominated galaxies, finding the crucial result that a single m and g pair&#xD;
fits all selected galaxies. Thirdly, we present three dimensional (3D) simulation results of self&#xD;
interacting FDM, and we demonstrate a scheme which allows us to reconstruct density profiles&#xD;
whose inferred rotation curves replicate observational data. In particular, we present a sim&#xD;
ulated self-interacting FDM halo corresponding to a galaxy for which we have observational&#xD;
data, specifically galaxy UGCA444. We find an elegant form of the core-halo mass relation,&#xD;
depending on the total energy of the system and qualitatively comment on the variation in&#xD;
granule number and size depending on total energy. Next, we analyse the dynamical aspects of&#xD;
the halo. In particular we (i) investigate the effects of m and g on the oscillation frequency of&#xD;
soliton cores; (ii) reveal evidence for a cooling (condensation) process, where the core density&#xD;
grows on time scales longer than the age of the universe; (iii) finally, we undertake a preliminary&#xD;
investigation of the orbital dynamics of test particles in our recreated galaxy, commenting on&#xD;
the velocity dispersion and the implications for the age gradient of stars in disc galaxies.
Description: Ph. D. Thesis.</description>
      <pubDate>Wed, 01 Jan 2025 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://theses.ncl.ac.uk/jspui/handle/10443/6792</guid>
      <dc:date>2025-01-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>A study of imbalanced quantum droplets</title>
      <link>http://theses.ncl.ac.uk/jspui/handle/10443/6783</link>
      <description>Title: A study of imbalanced quantum droplets
Authors: Flynn, Thomas A
Abstract: Gases of ultracold atoms have proved to be a highly versatile platform for studying&#xD;
quantum physics due in part to their high controllability. One example of this control is&#xD;
the manipulation of interactions. A single-component Bose gas in free space is unstable to&#xD;
collapse under attractive contact interactions, whereas, in an attractive two-component&#xD;
Bose gas the collapse is arrested by the repulsion from quantum fluctuations, forming&#xD;
self-bound liquid droplets: quantum droplets. Quantum droplets are therefore a quantum&#xD;
fluid in which quantum fluctuations are not only present but integral. During formation&#xD;
quantum droplets preserve a constant density ratio such that the droplet can be approxi&#xD;
mately described by its total density rather than in terms of two independent component&#xD;
densities. This approximation, known as density locking, is powerful but limiting. Droplet&#xD;
experiments typically begin with a population imbalance during formation, meaning that&#xD;
imbalanced droplets may be the most prevalent. Motivated by a link with an experi&#xD;
mental 174YbCs mixture, which deviates from many of the assumptions built into the&#xD;
density-locked model, the primary focus of this thesis is: how are droplets modified by&#xD;
imbalances that break the assumptions of density locking?&#xD;
This thesis begins by showing that, up to a saturation limit, free-space droplets can&#xD;
lower their energy through population imbalancing but correspondingly become less stably&#xD;
bound. By perturbing these imbalanced droplets, breathing modes are observed to have a&#xD;
complex parameter space of multiple, superimposed, decaying modes with time-dependent&#xD;
frequencies and decay rates.&#xD;
All droplets are experimentally formed in harmonic traps, and so the free-space imbal&#xD;
anced results are extended to study how harmonic traps affect the structure and breathing&#xD;
modes of imbalanced droplets. Beyond the droplet formation, there is a crucial question&#xD;
around the stability of the imbalance during a release into free space. A key result of this&#xD;
thesis is that imbalances can be retained during either an instantaneous or linearly-ramped&#xD;
trap release.&#xD;
Finally, the imbalanced droplet results above are applied to explore the 174YbCs pa&#xD;
rameter space, by measuring droplet size, peak densities and lifetimes. A variety of&#xD;
dynamics are studied from droplet formation and excitations, to proposing potential ex&#xD;
periments serving as a platform to study the non-equilibrium dynamics of droplets.
Description: PhD Thesis</description>
      <pubDate>Wed, 01 Jan 2025 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://theses.ncl.ac.uk/jspui/handle/10443/6783</guid>
      <dc:date>2025-01-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Charge control of defect colour centres in hexagonal boron nitride</title>
      <link>http://theses.ncl.ac.uk/jspui/handle/10443/6773</link>
      <description>Title: Charge control of defect colour centres in hexagonal boron nitride
Authors: Prasad, Madhava Krishna
Abstract: Colour centres in hexagonal boron nitride (hBN) have gained significant interest as they&#xD;
are active at room temperature and embedded in a two-dimensional material. The latter&#xD;
leads to minimal total internal reflection and coupling to photonic devices with nanometre&#xD;
proximity. Colour centres in hBN are particularly interesting as they have applications in&#xD;
quantum information, communications, metrology and LED technology. Current research&#xD;
has largely focused on photoluminescence from these defects. However, the integration of&#xD;
solid-state emitters into electronics necessitates the defects to be electrically driven. It is&#xD;
therefore essential to understand charge control of these defects.&#xD;
Recently, it was discovered that the charge state of defects in hBN can be controlled&#xD;
by interfacing it with graphene. It was observed that charge transfer between optically&#xD;
active defects in hBN and graphene led to the quenching of photoluminescence from these&#xD;
emitters. Therefore, interfacing hBN with graphene offers a pathway to inject carriers&#xD;
into hBN for the electrical control of defects. This is especially useful as graphene, also&#xD;
being a two-dimensional material, is a suitable gate to apply vertical electric fields across&#xD;
emitters in hBN.&#xD;
In this thesis, the study of charge transfer between hBN and graphene has been ex&#xD;
plored both from a theoretical and experimental standpoint. The theoretical approach&#xD;
involves using density functional theory to perform electronic structure calculations of de&#xD;
fects in hBN and subsequently deriving defect properties, such as band structure, defect&#xD;
geometry, and formation energies. The results of these calculations allowed the determina&#xD;
tion of the degree of charge transfer between defects in hBN and graphene. Furthermore,&#xD;
periodic boundary conditions and the choice of methodology for the assignment of charge&#xD;
to different layers had a significant impact on the derived value of charge transfer. A&#xD;
methodology to determine charge transfer that was robust against these effects was de&#xD;
veloped.&#xD;
The impact of the thickness of encapsulating hBN and graphene layers on charge&#xD;
transfer and the thermodynamics of the defect was also explored. The energy path for the&#xD;
Charge control of defect colour centres in hexagonal boron nitride&#xD;
reorientation of the defect between two equilibrium structures was studied to determine&#xD;
metastable intermediate states. It was found that the energy ordering of different phases&#xD;
of a defect was sensitive to the encapsulation of the host layer by graphene and hBN. As&#xD;
such, encapsulating layers can impact the spectroscopic properties of the defect.&#xD;
Experimentally, site control of emitters in hBN was studied. This involved the growth&#xD;
of an aluminium oxide (Al2O3) spacer between graphene and hBN to mitigate the quench&#xD;
ing of emitters. The Al2O3 was then patterned using electron beam lithography and etched&#xD;
to create an array of pillars. hBN was then deposited on top hosting emitters, with the&#xD;
aim of emitters being quenched in regions where there was direct contact with graphene&#xD;
and active in regions where an intermediate Al2O3 layer was present. Emitters were found&#xD;
predominantly on the edges of the pillars and quenching occurred in the regions where&#xD;
the pillars were absent. Hence spatial contol over colour centres in hBN was achieved.
Description: Ph. D. Thesis.</description>
      <pubDate>Wed, 01 Jan 2025 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://theses.ncl.ac.uk/jspui/handle/10443/6773</guid>
      <dc:date>2025-01-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Phase transition and conductivity modification of porous silicon via CO2 laser processing</title>
      <link>http://theses.ncl.ac.uk/jspui/handle/10443/6765</link>
      <description>Title: Phase transition and conductivity modification of porous silicon via CO2 laser processing
Authors: Qadi, Haifa Ali Ibrahim
Abstract: This study investigates how laser irradiation modifies the optical, structural and electrical properties of porous silicon (PS). PS samples were fabricated by electrochemically etching p-type&#xD;
crystalline silicon wafers at a current density of 63 mA/cm2&#xD;
for 20 minutes. A continuous wave&#xD;
CO2 laser (10.6 µm, 5–40 W) was then applied. A comprehensive suite of characterisation techniques, including scanning electron microscopy (SEM), atomic force microscopy (AFM), X-ray&#xD;
diffraction (XRD), X-ray photoelectron spectroscopy (XPS), secondary ion mass spectrometry&#xD;
(SIMS), Kelvin probe force microscopy (KPFM), Raman spectroscopy and current-voltage (I-V)&#xD;
measurements was used to analyse the samples before and after laser irradiation.&#xD;
The unique interaction between the 10.6 µm CO2 laser and PS is attributed to the significant&#xD;
IR absorption of PS at this wavelength, unlike bulk silicon. Upon laser irradiation, vibrational&#xD;
excitation triggers localised heating and the formation of heat zones, which induce two distinct&#xD;
stages. During the pre-melting consolidation stage, localised heating leads to partial melting of&#xD;
pore walls, causing adjacent pores to merge. As pores coalesce, the number of individual pores&#xD;
decreases, and the material between them consolidates, resulting in thicker pore walls, wider&#xD;
remaining pores, and an overall reduction in porosity. SEM and AFM analyses reveal a decrease&#xD;
in PS layer thickness and a smoother surface, with a roughness decreasing from 1.48 to 0.82 nm,&#xD;
approaching that of the underlying crystalline silicon substrate.&#xD;
In the melting stage, where the temperature exceeds the melting point of the silicon, the AFM&#xD;
images show a complete pore collapse, indicating that the silicon has fully melted. Raman spectroscopy transitions from a broadened, redshifted spectrum with an additional lower-frequency&#xD;
peak to a sharp crystalline peak at 520 cm-1 (with a 2.8 cm-1 full width at half maximum) in&#xD;
the laser-modified regions. Increasing laser intensity and exposure further broadens the peak&#xD;
and induces a redshift, accompanied by the emergence of a secondary peak, suggesting stress&#xD;
effects. XRD confirms the reformation of a single-crystalline structure, while XPS analysis&#xD;
reveals significant oxidation and the formation of a silicon oxide layer in the laser-irradiated&#xD;
areas, a layer that when removed by HF etching restores the Raman spectral profile.&#xD;
Electrical characterisation shows that the laser-processed areas exhibit metallic-like behaviour,&#xD;
as evidenced by I-V measurements and KPFM data indicating a high-work function network.&#xD;
This behaviour is attributed to the uneven distribution of boron during electrochemical etching,&#xD;
leading to the formation of heavily doped silicon nanowires. Upon laser irradiation, these regions&#xD;
melt and recrystallise, resulting in localised metallic-like conduction because of the high density&#xD;
of charge carriers and a reduced bandgap. Overall, the controlled laser irradiation process&#xD;
offers a precise means of tailoring PS properties, with significant implications for advanced&#xD;
applications in optical waveguides, biosensors, photovoltaics, microelectronics, energy storage,&#xD;
and plasmonic devices
Description: PhD Thesis</description>
      <pubDate>Wed, 01 Jan 2025 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://theses.ncl.ac.uk/jspui/handle/10443/6765</guid>
      <dc:date>2025-01-01T00:00:00Z</dc:date>
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