arXiv subjects

Ali Kurmus

Publications and source records attributed to Ali Kurmus.

5 recordsLinked to original sources

arXiv2026

Visualizing Mathieu-Type Dynamics in a Tabletop Magnetic Trap: A Coil-Driven Parametric Oscillator

We present a tabletop demonstration of dynamic stabilization and ponderomotive-like trapping using a pair of sinusoidally-driven anti-Helmholtz coils and a suspended permanent magnet. The oscillating field produces a rapid micromotion superimposed on a slower secular oscillation, with micromotion amplitude increasing with displacement and peaking near the turning points. This behavior reveals a ponderomotive-like mechanism: a spatial gradient of micromotion amplitude that drives slow secular motion. The time-averaged effect provides a time-averaged harmonic (ponderomotive) restoring force that confines the magnet between the coils. Driving at 12-18 Hz places the system in a small-q regime where the two time scales are clearly separated and directly visible to the eye. Video tracking (included with this article) quantifies the motion and reveals a stability edge as the drive frequency is lowered (near 6-7 Hz in our apparatus). From trajectories in the 12-18 Hz range, we extract an effective Mathieu parameter q ~ 0.16 from the measured timescale separation of the secular versus drive frequencies. The apparatus uses inexpensive, readily available parts, and we provide a concise materials list, analysis code, field-gradient calibration data, and demonstration videos.

physics.atom-ph↗

arXiv2025

Non-orbital particle trapping in binary black holes through dynamic stability

We present an interdisciplinary comparison between binary black hole systems and Radio Frequency (RF) Paul Traps, modeling the gravitational binary system as a rotating saddle near its center. This analogy connects these seemingly unrelated systems through the concept of dynamic stability. The rotating saddle potential is analytically tractable, allowing us to prove the existence of bounded charged particle trajectories under certain conditions. By focusing on stellar-mass black holes with a weak electric charge-a feature consistent with specific astrophysical conditions that leaves the spacetime metric largely unaffected but can influence nearby particle interactions-we can neglect complicating factors such as magnetic fields from large accretion disks of heavier black holes or stellar winds. Our simulation results demonstrate that charged particles can exhibit stable, non-orbital trajectories near the center of a binary system with charged stellar-mass black holes, providing unique three-dimensional trapping primarily through gravity. This system is distinctive in the literature for its non-orbital trapping mechanism. While theoretically intriguing, this trapping relies on specific conditions, including nearly identical black hole masses. These types of non-orbital trapping mechanisms could potentially allow for longer-lived plasma configurations, enhancing our ability to detect electromagnetic signatures from these systems. The significance of this work lies in the novel comparison between a laboratory-scale quantum system and a larger astrophysical one, opening new avenues for exploring parallels between microscopic and cosmic phenomena across fourteen orders of magnitude in distance.

astro-ph.HE↗

arXiv2025

The asymmetric rotating saddle potential as a mechanical analog to the RF Paul trap

Under specific conditions, a rotating saddle potential can confine the motion of a particle on its surface. This time-varying hyperbolic potential shares key characteristics with the RF electric quadrupole ion trap (RF Paul trap), making it a valuable mechanical analog. Previous work has primarily focused on symmetric saddles, characterized by equal curvatures along the trapping and anti-trapping directions. However, most applications of RF Paul traps-such as atomic clocks, quantum computing, and quantum simulations-require asymmetry in the quadrupole potential to break the degeneracy of motional modes, which is essential for processes like laser cooling and other quantum manipulations. In this paper, we investigate the motion of trapped particles in asymmetric rotating saddles. We demonstrate that even minor asymmetries, including those arising from manufacturing imperfections, can significantly affect particle trajectories and stability. Our analysis includes both theoretical modeling and experimental measurements. We derive the equations of motion for asymmetric saddles and solve them to explore stability and precession effects. Additionally, we present lifetime measurements of particles in saddles with varying degrees of asymmetry to map key features of the a-q stability diagram, including counterintuitive demonstrations of stability for saddles with negative asymmetry. This study underscores the importance of incorporating asymmetry into mechanical models of ion traps to better reflect real-world implementations. Although motivated primarily by RF Paul traps, these asymmetry-related results are also relevant to emerging gravitational analogs, such as rotating saddle potentials in certain binary black hole systems.

physics.atom-ph↗

arXiv2023

Directly Characterizing Dome Seeing: Differential Image Motion Sensor Using Multisources (DIMSUM)

Image degradation impedes our ability to extract information from astronomical observations. One factor contributing to this degradation is ``dome seeing", the reduction in image quality due to variations in the index of refraction within the observatory dome. Addressing this challenge, we introduce a novel setup-DIMSUM (Differential Image Motion Sensor Using Multisources)-which offers a simple installation and provides direct characterization of local index of refraction variations. This is achieved by measuring differential image motion using strobed imaging that effectively``freezes" the atmosphere, aligning our captured images with the timescale of thermal fluctuations, thereby giving a more accurate representation of dome seeing effects. Our apparatus has been situated within the Auxiliary Telescope of the Vera C. Rubin Observatory. Early results from our setup are encouraging. Not only do we observe a correlation between the characteristic differential image motion (DIM) values and local temperature fluctuations (a leading cause of variations in index of refraction), but also hint at the potential of DIM measures to characterize dome seeing with greater precision in subsequent tests. Our preliminary findings underscore the potential of DIMSUM as a powerful tool for enhancing image quality in ground-based astronomical observations. Further refinement and data collection will likely solidify its place as a useful component for managing dome seeing in major observatories like the Vera C. Rubin Observatory.

astro-ph.IM↗

arXiv2022

The feasibility of constraining DM interactions with high-redshift observations by JWST

Observations of the high redshift universe provide a promising avenue for constraining the nature of the dark matter (DM). This will be even more true with the advent of the James Webb Space Telescope (JWST). We run cosmological simulations of galaxy formation as part of the Effective Theory of Structure Formation (ETHOS) project to compare high redshift galaxies in Cold (CDM) and alternative DM models which have varying relativistic coupling and self-interaction strengths. The interacting DM scenarios produce a cutoff in the linear power spectrum on small-scales, followed by a series of "dark acoustic oscillations". We find that DM interactions suppress the abundance of galaxies below $M_\star \sim 10^8\,M_\odot$ for the models considered. The cutoff in the power spectrum delays structure formation relative to CDM. Objects in ETHOS that end up at the same final masses as their CDM counterparts are characterised by a more vigorous phase of early star formation. While galaxies with $M_\star \lesssim 10^6\,M_\odot$ make up more than 60 per cent of star formation in CDM at $z\approx 10$, they contribute only about half the star formation density in ETHOS. These differences diminish with decreasing redshift. We find that the effects of DM self-interactions are negligible compared to effects of relativistic coupling (i.e. the effective initial conditions for galaxy formation) in all properties of the galaxy population we examine. Finally, we show that the clustering strength of galaxies at high redshifts depends sensitively on DM physics, although these differences are manifest on scales that may be too small to be measurable by JWST.

astro-ph.GA↗