activity
20192026
most citedProspects for Fundamental Physics with LISA

401 citations · 636 across the 16 of their papers we have counts for

collaborators
Showing 2026Show all

7 papers · 1 filter

astro-ph.HE2026

The Structure in the Structure Function of Black Hole Light Curves

Daniel C. M. Palumbo, Alejandro Cárdenas-Avendaño, Lena Murchikova

Of the two black holes, M87 and Sgr~A, for which event-horizon-scale imaging is currently achievable, only Sgr~A at our Galactic Center exhibits sub-hour varia…

astro-ph.HE2026

Bayesian Evidence for Inspiraling Hotspot Motion in the Galactic Center

Pablo Ruales, Maciek Wielgus, Delilah E. A. Gates +1

During flaring episodes, polarimetric observations of the Galactic Center black hole Sagittarius A* (Sgr A*) reveal evolving, loop-like trajectories in the Stokes Q-U plane, the so…

astro-ph.HE2026

A Four-Dimensional Gaussian Random Field Generator for Modeling Spatiotemporal Variability in Astrophysical Sources

Alejandro Cárdenas-Avendaño, Diego Rubiera-Garcia, Frederic H. Vincent

Semi-analytic models of black-hole movies require both an emitting flow prescription and a time-dependent source variability. Existing prescriptions are often limited to either equ…

astro-ph.HE2026★ 1 cited

Light Propagation Prescriptions for Black Hole Movies

Daniel Rojas-Paternina, Alejandro Cárdenas-Avendaño

The spatiotemporal content of a black-hole movie is set jointly by source variability and by the distribution of light-travel times across the image. In the slow-light prescription…

gr-qc2026

Parameter-estimation bias induced by transient orbital resonances in extreme-mass-ratio inspirals

Edoardo Levati, Alejandro Cárdenas-Avendaño

Given the multifrequency nature of relativistic orbits, transient orbital resonances are expected to be ubiquitous during an extreme-mass-ratio inspiral (EMRI). At a resonance, the…

astro-ph.HE2026

Sensitivities of Black Hole Images from GRMHD Simulations

Pedro Naethe Motta, Mário Raia Neto, Cora Prather +1

The advent of high-fidelity imaging of supermassive black holes calls for efficient and robust data-analysis methods. In this work, we use , a differentiable, $\te…

astro-ph.HE2026

Polarization Signatures of Inspiraling Hotspots around Kerr Black Holes

Pablo Ruales, Delilah E. A. Gates, Alejandro Cárdenas-Avendaño

Polarimetric interferometry is a powerful tool for probing both black hole accretion physics and the background spacetime. Current models aimed at explaining the observed multiwave…