Asymptotic scaling theory of electrostatic turbulent transport in magnetised fusion plasmas
(2026)
Resonant locking between binary systems induced by gravitational waves
Physical Review D American Physical Society (APS) 113:2 (2026) 023040
Abstract:
The interaction of gravitational waves (GWs) with matter is thought to be typically negligible in the Universe. We identify an exception in the case of resonant interactions, where GWs emitted by a background binary system, such as an inspiraling supermassive black hole (SMBH) binary, cause a resonant response in a stellar-mass foreground binary and the frequencies of the two systems become, and remain, synchronized. We point out that this previously unexplored dynamical phenomenon is not only possible, but can lead to binary systems becoming resonantly locked in the host galaxy of merging SMBHs of mass , each of which has a significantly reduced merger time. We predict binary systems have been locked in the Universe’s history. Resonant locking could be detected through anomalous inspiral of binary systems.Angular-momentum pairs in spherical systems: applications to the Galactic centre
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) (2026) stag039
Abstract:
Abstract Consider a system of point masses in a spherical potential. In such systems objects execute planar orbits covering two-dimensional rings or annuli, represented by the angular-momentum vectors, which slowly reorient due to the persistent weak gravitational interaction between different rings. This process, called vector resonant relaxation, is much faster than other processes which change the size/shape of the rings. The interaction is strongest between objects with closely aligned angular-momentum vectors. In this paper, we show that nearly parallel angular-momentum vectors may form stable bound pairs in angular-momentum space. We examine the stability of such pairs against an external massive perturber, and determine the critical separation analogous to the Hill radius or tidal radius in the three-body problem, where the angular-momentum pairs are marginally disrupted, as a function of the perturber’s mass, the orbital inclination, and the radial distance. Angular-momentum pairs or multiples closer than the critical inclination will remain bound and evolve together in angular-momentum-direction space under any external influence, such as anisotropic density fluctuations, or massive perturbers. This study has applications in various astrophysical contexts, including galactic nuclei, in particular the Milky Way’s Galactic centre, globular clusters, or planetary systems. In nuclear star clusters with a central super-massive black hole, we apply this criterion to the disc of young, massive stars, and show that clusters in angular-momentum space may be used to constrain the presence of intermediate-mass black holes or the mass of the nearby gaseous torus.
Reconstructions of electron-temperature profiles from EUROfusion pedestal database using turbulence models and machine learning
Journal of Plasma Physics. 2025;91(6):E155.
Abstract:
This study makes use of plasma-profile data from the EUROfusion pedestal database (Frassinetti et al. 2020 Nucl. Fusion vol. 61, p. 016001), focusing on the electron-temperature and electron-density profiles in the edge region of H-mode ELMy JET ITER-Like-Wall (ILW) pulses. We make systematic predictions of the electron-temperature pedestal, taking engineering parameters of the plasma pulses and the density profiles as inputs. We first present a machine-learning (ML) algorithm which, given more inputs than theory-based modelling, is able to reconstruct unseen temperature profiles within 20 % of the experimental values. We find a hierarchy of the most consequential engineering parameters for such predictions. This result confirms the conceptual possibility of accurate data-driven prediction. Next, taking a simple theoretical approach that assumes a definite local relationship between the electron-density (𝑅/𝐿𝑛𝑒) and electron-temperature (𝑅/𝐿𝑇𝑒) gradients, we find that a range of power-law scalings 𝑅/𝐿𝑇𝑒 =𝐴(𝑅/𝐿𝑛𝑒)𝛼 with 𝛼 ≈0.4 correctly capture the behaviour of the electron-temperature in the steep-gradient region. Fitting 𝐴 and 𝛼 independently for each pedestal reveals a clear one-to-one correlation, suggesting an underlying constraint in pedestal physics. The measured 𝜂𝑒 =𝐿𝑛𝑒/𝐿𝑇𝑒 values across the pedestal exhibit a wide distribution, significantly exceeding the slab-ETG linear stability threshold, implying either a non-linear threshold shift or a measurably supercritical saturated turbulent state. Finally, we fit parameters for scalings that relate the turbulent heat flux to the gradients 𝑅/𝐿𝑇𝑒 and 𝑅/𝐿𝑛𝑒, similarly to models extracted from gyrokinetic simulations. The inclusion of more experimental parameters is necessary for such models to match the accuracy of our ML results.
Finding Local Parallel Electric Fields in Magnetotail Reconnection Using a Two-Spacecraft Method
(2025)