output
19982026
most citedBlack holes, gravitational waves and fundamental physics: a roadmap

742 citations

589 papers

astro-ph.SR2026

Cyclic light variations and accretion disk evolution in the LMC eclipsing binary OGLE-LMC-DPV-062

R. E. Mennickent, G. Djurašević, J. A. Rosales +4

Many intermediate-mass close binaries exhibit photometric cycles longer than their orbital periods, likely related to accretion-disk variability. Previous studies indicate that his…

cond-mat.soft2025

Insertion space in repulsive active matter

Luke K. Davis, Karel Proesmans

For equilibrium hard spheres, the statistical geometry of the insertion space, the room to accommodate another sphere, relates exactly to the equation of state. We begin to extend…

astro-ph.HE2023★ 7 cited

ATCA Study of Small Magellanic Cloud Supernova Remnant 1E 0102.2-7219

Rami Z. E. Alsaberi, M. D. Filipović, S. Dai +29

We present new and archival Australia Telescope Compact Array and Atacama Large Millimeter/submillimeter Array data of the Small Magellanic Cloud supernova remnant 1E 0102.2-7219 a…

astro-ph.SR2023★ 8 cited

V4142 Sgr: a Double Periodic Variable with an accretor surrounded by the accretion-disk's atmosphere

J. A. Rosales, R. E. Mennickent, G. Djurašević +4

Context: A detailed study of the close interacting binary V4142\,Sgr based on photometric and spectroscopic analysis is presented.This system belongs to the enigmatic class of Algo…

hep-th2023★ 9 cited

All the D-Branes of Resurgence

Ricardo Schiappa, Maximilian Schwick, Noam Tamarin

It was recently shown how to account for all instantons of hermitian matrix models via (anti-) eigenvalue-tunneling -- including both exponentially-suppressed and exponentially-enh…

astro-ph.HE2022★ 13 cited

New ASKAP Radio Supernova Remnants and Candidates in the Large Magellanic Cloud

Luke M. Bozzetto, Miroslav D. Filipović, H. Sano +34

We present a new Australian Square Kilometre Array Pathfinder (ASKAP) sample of 14 radio Supernova Remnant (SNR) candidates in the Large Magellanic Cloud (LMC). This new sample is…