Bolysbek Yerkebulan

Very interesting! I haven’t worked directly with ^{11}Be, but I’ve done some work with time-dependent models in nuclear systems. To describe decay and the dynamics of weakly bound nuclei, time-dependent methods like TDHF (Time-Dependent Hartree–Fock) or TDDFT are quite effective, as well as three-body wave-packet approaches for modeling breakup and tunneling. If you’re doing numerical time evolution, I’d recommend looking into split-operator or Crank–Nicolson schemes — they conserve the wave function norm well and remain stable with larger time steps. Fascinating topic — these models really help to understand how halo nuclei behave under weak binding conditions!

That sounds great! I’ve worked with PHOEBE a bit for binary systems. For nova-like variables, you might try including the accretion disk as an additional light source and adjusting its temperature profile manually — PHOEBE doesn’t model disks perfectly out of the box. Also, star spots can be approximated quite well if you start with smaller radii and increase contrast gradually during fitting. Good luck with your modeling — nova-like systems are tricky but really fascinating!

Very interesting! In astronomy, when studying extreme states of matter — for example, in the cores of neutron stars or during galaxy collisions — we often use hydrodynamic and numerical models, as well as simulations of plasma and magnetic field evolution. Similar approaches can be applied to nuclear collisions to study how matter behaves at extremely high temperatures and densities.

I haven’t worked with gravitational wave data, but in communications we often use classic signal processing methods to deal with noise — like filtering, correlation analysis, adaptive filters, and spectral techniques. For example, matched filtering or adaptive noise suppression methods are very effective for detecting weak signals. I think similar approaches could be useful for gravitational wave analysis too.

I'm currently studying solar radio emission using a time-dependent approach to understand how different solar events affect the intensity and frequency of the emitted radiation. My work involves modeling radio bursts and investigating how the dynamics of coronal plasma lead to various types of radio emissions. Is anyone here studying similar topics, interested in this field, or using time-dependent models to analyze radio bursts?