activity
20052026
most citedKinematic Structure of Merger Remnants

371 citations · 864 across the 12 of their papers we have counts for

collaborators

12 papers

q-fin.ST2026

Multiscaling in the Rough Bergomi Model: A Tale of Tails

Giuseppe Brandi, Tiziana Di Matteo

The rough Bergomi (rBergomi) model, characterised by its roughness parameter , has been shown to exhibit multiscaling behaviour as approaches zero. Multiscaling has profound…

astro-ph.IM2025

Bridging Literature and the Universe Via A Multi-Agent Large Language Model System

Xiaowen Zhang, Zhenyu Bi, Patrick Lachance +3

As cosmological simulations and their associated software become increasingly complex, physicists face the challenge of searching through vast amounts of literature and user manual…

q-fin.ST2025

Supervised Similarity for Firm Linkages

Ryan Samson, Adrian Banner, Luca Candelori +9

We introduce a novel proxy for firm linkages, Characteristic Vector Linkages (CVLs). We use this concept to estimate firm linkages, first through Euclidean similarity, and then by…

astro-ph.GA2024★ 1 cited

Signatures of black hole seeding in the local Universe: Predictions from the BRAHMA cosmological simulations

Aklant K Bhowmick, Laura Blecha, Paul Torrey +8

The first "seeds" of supermassive black holes (BHs) continue to be an outstanding puzzle, and it is currently unclear whether the imprints of early seed formation survive today. He…

astro-ph.GA2024★ 1 cited

The redshift evolution of the scaling relation: new insights from cosmological simulations and semi-analytic models

Shashank Dattathri, Priyamvada Natarajan, Antonio J. Porras-Valverde +4

We study the co-evolution of black holes (BHs) and their host galaxies in the ASTRID and Illustris-TNG300 cosmological simulations and the Dark Sage Semi-Analytic Model (SAM), focu…

astro-ph2007★ 104 cited

Instabilities in the time-dependent neutrino disc in Gamma-Ray Bursts

Agnieszka Janiuk, Ye-Fei Yuan, Rosalba Perna +1

We investigate the properties and evolution of accretion tori formed after the coalescence of two compact objects. At these extreme densities and temperatures, the accreting torus…