works on

From the 1 of 21 linked papers with an AI index.

collaborators

21 papers

hep-th2026

Localizing Momentum Waves on Mazes

Tobi Ramella, Nicholas P. Warner

We examine the proposal and analysis of arXiv:2404.14477 for putting momentum waves on mazes of intersecting M2 and M5 branes by computing a family of simple examples of momentum w…

astro-ph.CO2026

Cosmography with DESI-DR1 Cosmic Chronometers: Direct H(z) measurements from Luminous Red Galaxy ages

Carlos A. Álvarez, Marcos M. Cueli, Balakrishna S. Haridasu +6

Providing robust redshift estimates for almost 3 million luminous red galaxies (LRGs), the Dark Energy Spectroscopic Instrument (DESI) offers a unique opportunity to test the expan…

astro-ph.SR2026

The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity

Amedeo Romagnolo, Floor S. Broekgaarden, Alex C. Gormaz-Matamala +7

The paper builds a comprehensive grid of stellar evolution models to compare 14 wind prescriptions and shows that black‑hole masses at solar metallicity are determined by whether a…

astro-ph.GA2026

How galaxies acquire their stellar mass at high redshift: High star formation efficiencies and the relative roles of dust and initial mass function

Hao Fu, Francesco Shankar, Fabio Fontanot +9

JWST has measured an unprecedented abundance of galaxies above , whose formation and evolution are still difficult to reconcile within traditional galaxy evolution mo…

astro-ph.HE2026

The impact of stellar binaries and star cluster dynamics on pair-instability supernovae

Francesco Gabrielli, Cristiano Ugolini, Lavinia Paiella +12

Pair-instability supernovae (PISNe) are among the most luminous transients in the Universe. However, they have never been confidently observed. Solving this puzzle would have key i…

astro-ph.HE2026

Can current models predict the local black hole merger rate?

Lumen Boco, Michele Bosi, Cecilia Sgalletta +2

After four observational runs, the Ligo-Virgo-Kagra collaboration estimated a local binary black hole (BBH) merger rate density of $R_{0,\textrm{LVK}}\simeq 14-26\,\textrm{Gpc}^{-3…