With the development of next-generation gravitational waves detectors, we aim to measure and infer data on a broader range of the energy and redshift spectrum. However, in this range, deviations...Show moreWith the development of next-generation gravitational waves detectors, we aim to measure and infer data on a broader range of the energy and redshift spectrum. However, in this range, deviations from theories that predict a non-standard propagation speed for GWs are expected to become non negligible anymore. Moreover, it has been shown that the presence of inhomogeneities and structures in our universe does affect the GWs observables: with the forecasted level of precision of future detectors, such corrections can not be ignored. In this work we set in the frame of quartic scalar-tensor theories of gravity to study such relativistic effects with the presence of an extra scalar degree of freedom. Due to the complexity of the full theory, we opted for a phenomenological approach to describe the dispersion relation and amplitude evolution of the metric perturbation. Using this technique, we evaluated the relativistic corrections to frequency and direction of propagation of the GWs wave-vector. On the other hand, it was not possible to analytically calculate the relativistic corrections to the tensor amplitude even using the parametric approach, as a consequence of the elevated number of terms in the amplitude evolution equation. Nevertheless, after selecting from such equation the transverse-traceless modes, we were able to find, using the N-P formalism, which types of term can actually contribute to the evolution of the physical modes.Show less
The imaging of biological tissue is an important aspect to understand the human body and the processes taking place at small scales. Existing optical and electron microscopy techniques face trade...Show moreThe imaging of biological tissue is an important aspect to understand the human body and the processes taking place at small scales. Existing optical and electron microscopy techniques face trade-offs between resolution and beam damage. Optical near-field electron microscopy (ONEM) is a newly developed technique combining optical microscopy with electron microscopy. A sample is illuminated from the back with light in the visible spectrum, a near-field shadow is cast on a low workfunction photocathode. Photons are converted into electrons by the photoelectric effect and finally, the electrons exit the photocathode towards the detection optics. As a result, ONEM allows the imaging of (biological) samples without exposure to the damaging electron beam without being diffraction limited. We explore the preparation of samples suitable for ONEM experiments consisting of a fused silica substrate with an indium tin oxide (ITO) coating and a slice of biological tissue from a mouse tail. We create a cap over the biotissue from either single-layer graphene or amorphous carbon and finally, we grow a thin caesium photocathode in situ to lower the workfunction. Using a blue laser with a wavelength of 450 nm, we show for the first time that optical near-field electron microscopy can be used to image biological tissue. We can distinguish features in ONEM matching features in PEEM when overlapping the images. The resolution of these features is in the order of 100 nm when using a 5.7 μm field of view. Furthermore, we show that a carbon or graphene layer is required for ONEM imaging, yet this layer decreases the resolution of the PEEM image.Show less
Supernovae are powerful cosmic explosions that usually occur within their host galaxies. However, recent observations have discovered a small but growing number of supernovae located outside of...Show moreSupernovae are powerful cosmic explosions that usually occur within their host galaxies. However, recent observations have discovered a small but growing number of supernovae located outside of their host galaxies, known as orphan supernovae. This thesis project aims to investigate these peculiar events and their host environments to gain insights into the mechanisms that drive them. The objectives include analyzing a large sample of supernovae and determining if we actually observe a population of orphan supernovae. The methodology involves data analysis and theoretical modeling, utilizing public catalogs, archival data, and wide-field surveys.Show less
The galactic Interstellar Medıum or ısm is one of the most studied components of the galaxy. In spite of this, no widely accepted complete dynamical model of the ısm exists. Two of the most...Show moreThe galactic Interstellar Medıum or ısm is one of the most studied components of the galaxy. In spite of this, no widely accepted complete dynamical model of the ısm exists. Two of the most influential models proposed by Cox and Smith, (1974) & McKee and Ostriker, (1977), differ substantially in their descriptions of the geometry of supernova remnant cavities in the ısm. No direct analysis of the geometry of cavities in the ısm has been done due to concerns over observations of neutral hydrogen (Hı) being dominated by velocity caustics. Clark et al. (2019), showed that the linear structure of Hı is most likely not caused by velocity caustics. In this thesis, we propose to extend upon her findings and present a comparison of general cavity features in the ısm to both Cox’s and McKee’s models. This was achieved by comparing the cavities found by applying a void-finding watershed-like algorithm to the velocity-channel Hı images of the Canadıan Galactıc Plane Survey data and comparing the results with models of the ısm based on the Cox & McKee descriptions. We found evidence supporting Clark et al.’s position that narrow velocity channel images are not dominated by velocity caustics, but could not definitively support either Cox’s or McKee’s description of the ısm, even though the watershed algorithm was capable of obtaining the distribution of cavities in the model cavities.Show less
In recent years, deep neural networks have attracted the attention of both the academic community and the general public. An effort to theoretically understand the intricacies of these systems is...Show moreIn recent years, deep neural networks have attracted the attention of both the academic community and the general public. An effort to theoretically understand the intricacies of these systems is ongoing and physics-inspired approaches may have a part to play. In this thesis, we will discuss recent results in the theoretical study of deep linear neural networks. This class of neural networks has very limited real-world applications, but it could provide a good training ground for developing theoretical techniques that could prove useful beyond the simple linear case. We will also argue that Fisher information, and in particular “sloppy model” logic, can be a useful tool for future research on deep neural networks, in particular for network architecture optimization.Show less
Circuit partitioning is a powerful technique in the Noisy Intermediate Scale Quantum era. This method allows the evaluation of many-qubit algorithms with fewer qubits by writing the expectation...Show moreCircuit partitioning is a powerful technique in the Noisy Intermediate Scale Quantum era. This method allows the evaluation of many-qubit algorithms with fewer qubits by writing the expectation value of an observable as a weighted sum of products of inner products which are obtained by evaluating smaller circuits. However the number of terms in this sum generally scales exponentially with the depth of the circuit. The recently introduced Subset Partition Model only evaluates a subset of these terms. Here we explore the application of the Subset Partition Model for Variational Quantum Eigensolvers. Based on our investigation, we conjecture that this model may not be generally applicable to this Variational Quantum Algorithm due to the breaking of the Variational Principle. In addition, optimizing Partitioned Quantum Circuits is challenging due to the Barren Plateau problem that arises for even small circuit sizes. To address this problem, this thesis proposes a novel optimization algorithm that takes advantage of the additional structure on the cost function induced by circuit partitioning. By utilizing this new algorithm, we demonstrate that we can alleviate the barren plateau problem in the optimization of Partitioned Quantum Circuits.Show less
In our research project, we conducted an analysis of the impact of dark matter haloes on the motion of the Milky Way. Our study focused on dark matter haloes located within a radius of 200 Mega...Show moreIn our research project, we conducted an analysis of the impact of dark matter haloes on the motion of the Milky Way. Our study focused on dark matter haloes located within a radius of 200 Mega Parsecs (Mpc) from the Milky Way. The cosmological framework we implemented was the Lambda Cold Dark Matter model. Our primary objective was to deter- mine the peculiar acceleration of the Milky Way and derive insights about its motion. To achieve this, we compared the peculiar acceleration to the Hubble rate, a significant parameter in cosmology, as a reference point. By means of our study, we aimed to determine whether the Milky Way would eventually reach the Great Attractor or undergo a change in its direction of motion. Additionally, we generated an all-sky structure map for the haloes to explore the density distribution within each region. This anal- ysis allowed us to examine the concentration of dark matter throughout the universe inside the 200 Mpc from the Milky Way. In our research, we utilized data obtained from the SIBELIUS-DARK project, which provided a robust scientific basis for our study.Show less
In the quest for finding a room temperature stable single photon source (SPS), defects in hexgonal boron nitride (hBN) have gained more and more attention in the previous years. This thesis studies...Show moreIn the quest for finding a room temperature stable single photon source (SPS), defects in hexgonal boron nitride (hBN) have gained more and more attention in the previous years. This thesis studies the single photon emit- ting properties of defects in a multi-layer hBN flake with a home-build confocal microscopy setup. As a reference system, nitrogen vacancy (NV) centers in nanodiamonds (NDs) are measured first, as there luminescent properties are well documented in literature. In order to improve on pre- vious work in this group, polarization selective elements are included in the optical setup. This inclusion allowed measurements of the absorption and emission dipoles of the SPSs and improved our results by (1) reduc- ing the background and (2) allowing more efficient excitation. We found that defects in hBN showed promising results in terms of single photon purity (g2(0) =0.09 ± 0.06) and brightness (35 KHz), outperforming the best single NV center (g2(0) =0.29 ± 0.07, brightness: 4 KHz). We also found that the hBN defects showed long term (up to 3000 ns) bunching behaviour, possibly related to the excitation power during measurements. This, together with the measurement of different hBN flakes, constitute interesting topics for future investigation.Show less
Microcavities play a significant role in the study of cavity quantum electrodynamics (CQED), as they induce efficient coupling of light and matter. Confining matter within a cavity, increases the...Show moreMicrocavities play a significant role in the study of cavity quantum electrodynamics (CQED), as they induce efficient coupling of light and matter. Confining matter within a cavity, increases the probability of deterministic interactions between e.g. a (quantum) particle and the light cast into the cavity by a laserbeam. Cavity parameters such as cavity length and radius of curvature of the micromirror define the cavity regime and consequently the physical phenomena that can be observed, from the bad-cavity (Purcell) regime to the strong coupling regime. We are looking for a highly controllable and repeatable way of producing microcavities with a small mode volume and a high finesse. This translates into the creation of micromirrors with radii of curvature between 10 μm and 50 μm and a depth of up to 1 μm. We offer an overview of micromirror production methods; CO2 laser ablation, focused ion beam milling (FIB), direct laser writing and current controlled curvature. For CO2 laser ablation the key parameters to control the dimensions of the ablated structure, are the power of the laser and the beamwaist. We perform simulations of the ablation process and show that micromirrors with the desired dimensions can be obtained by using a CO2 laser in a range between 420-440 mW and a beamwaist of 40 μm. We find that for these parameters clipping loss is negligible. Therefore, CO2 laser ablation meets the criteria and proves to be a reliable way of producing micromirrors.Show less
Our research is related to testing dark energy/modified gravity theories. We determine the positivity bounds on effective field theories with spontaneously broken Lorentz invariance. We consider...Show moreOur research is related to testing dark energy/modified gravity theories. We determine the positivity bounds on effective field theories with spontaneously broken Lorentz invariance. We consider all the operators in a low-energy — effective field theory (EFT) approach and gain the conditions for EFT coefficients so that a theory is healthy (without instabilities). These conditions are called the positivity bounds, for which a theory works. These positivity bounds can give us constraints about the cosmological model. We mainly follow the paper Positivity bounds on effective field theories with spontaneously broken Lorentz invariance by Paolo Creminelli, Oliver Janssen, and Leonardo Senatore, where the positivity bounds are calculated from the two-point correlation functions of conserved quantities like the Noether current and stress-energy tensor. Then we show how this new mechanism of finding positivity bounds can be used for real cosmological models.Show less
Due to it’s chirality, the electron transport or electronic transmission through a molecule can have a spin preference. This is called the Chiral-Induced Spin Selectivity (CISS) effect....Show moreDue to it’s chirality, the electron transport or electronic transmission through a molecule can have a spin preference. This is called the Chiral-Induced Spin Selectivity (CISS) effect. Understanding CISS may contribute to the understanding of life but can also be useful for spintronic applications. Within this research, a setup for measuring the CISS-effect locally, using a Photo-Emission Electron Microscope (PEEM), is investigated. It is found that using a linear polarizer in combination with a lambda half plate can be related to the parallel and perpendicular polarization direction with respect to the sample. This is useful for tuning circular and elliptical polarization to the samples surface. Besides, it turned out that difference in illumination response for metallic structures for different handedness of the elliptically polarized light, is mostly related to the size (∼ 1µm) of the structures, but not significantly to its geometry. The setup is tested for a Self-Assembled Monolayer consisting of alkanethiol molecules, for which it shows equal response for left- and right-handed circularly polarized light. A Low-Energy Electron Microscopy (LEEM) measurement shows that the self-assembly process has led to an ordered layer on the gold on Mica substrate. In extension to this research, for future research on the CISS-effect, it would be interesting to fabricate a Self-Assembled Monolayer of chiral molecules with different handedness in order to measure whether or not opposite response to different elliptical light polarizations.Show less
In the process of metastasis, cancer cells may transmigrate through the endothelium barrier of the vascular walls and into the circulatory blood system. During this process, the cancer cells...Show moreIn the process of metastasis, cancer cells may transmigrate through the endothelium barrier of the vascular walls and into the circulatory blood system. During this process, the cancer cells interact with the endothelial cells, resulting in the alternation of their mechanical properties. Although this interaction has been broadly studied from the perspective of cancer cells, no thorough investigation of the endothelial mechanical properties has been performed. In this thesis, by using a micro-rheology AFM-based approach, we show that the properties of endothelial cells change when cultured in cancer cell conditioned medium, as well as when in contact with cancer cells. We found that the stiffness of endothelial cells increased when cultured in a low-dilution cancer cell medium, while it decreased in high-dilution medium. This change was also evident on the viscoelasticity of the cells, with the endothelial cells cultured in high dilution medium showing lower viscoelastic properties. Furthermore, endothelial cells in direct contact with a cancer cell showed an increased height, as a result of the cancer cell's transmigration through the monolayer. Our findings demonstrate that the properties of endothelial cells change indirectly due to cancer cell secreted substances, and directly during the cancer cells' physical transmigration. This indicates that the endothelium is actively responding to the presence of cancer cells, rather than being a passive barrier as once believed.Show less
Cyclically driving subharmonic units can result in emergent memory effects, and such systems have the potential to store information and perform computations. For this reason, we numerically...Show moreCyclically driving subharmonic units can result in emergent memory effects, and such systems have the potential to store information and perform computations. For this reason, we numerically investigated the response to cyclic driving of two linearly coupled toggling bits, which are an inherently subharmonic unit. We found that there are 380 topologically distinct two-t-bit systems. Cyclic driving sometimes resulted in subharmonic responses with emergent periods of T=3 and T=4, as well as nonzero transients (tau>0). A variety of different orbits is possible, but the behavior (tau, T)=(0, 2) inherent to the single toggling bit, remains common in systems of two t-bits. A period of T=4 already occurred for weakly coupled systems that can be manufactured in experiments. We also found the restriction that tau + T < 4. Lastly, we conclude that coupling strength strongly affects the likelihood of avalanches occurring. The findings demonstrate both the capabilities and limitations of coupled toggling bits, which will valuable for future research.Show less
This work explores axion-photon conversion in the TeV halo of the Geminga pulsar and in neutron star magnetospheres. Based on the observed synchrotron and inverse Compton scattering radiation, the...Show moreThis work explores axion-photon conversion in the TeV halo of the Geminga pulsar and in neutron star magnetospheres. Based on the observed synchrotron and inverse Compton scattering radiation, the magnetic field inside the Geminga pulsar TeV halo is constrained to be < 2 μG, similar to literature constraints. The photon-axion conversion probability is ≲ 10−8, requiring an extreme signal-to-noise ratio for detection. In contrast, significant flux transfer can take place in the strongly magnetised anisotropic plasmas of neutron star magnetospheres. Following up on recent literature, this work provides a three-dimensional calculation of axion-photon conversion in anistropic plasmas, including the Euler-Heisenberg photon-photon scattering contribution in the limit BNS ≪ Bc = 4.4 · 1013 G. This allows for resonant double lens conversion, through which axion-like particles of arbitrarily small mass can resonantly induce photons. For relativistic axions the resonance length scale can exceed other typical scales of change in the plasma, in which case the conversion region and probability is truncated. For very light, relativistic axions, non-resonant contributions are important. In the Goldreich-Julian model with relativistic plasma, double lens resonance can occur at observable radio frequencies in the 100 GHz−1 THz regime. NB: Erratum. The derivation in chapter 3 sets magnetic permeability mu=1. For double lens resonant conversion this is inconsistent. Upon including the correct expression for mu, the EH contribution to the resonance condition (Eq. 3.28) is slightly changed:14*eta*B^2 -> 22*eta*B^2. The error should, of course, also be incorporated in the whole derivation.Show less