2025/03/31 by Joanne Tan, Tan, Joanne · 7 voices
Decision Sciences · Physics and Astronomy · Social Sciences · #Astronomy and Astrophysical Research #Astrophysics of Galaxies (astro-ph.GA) #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #Earth and Planetary Astrophysics (astro-ph.EP) #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #Instrumentation and Methods for Astrophysics (astro-ph.IM) #International Science and Diplomacy #Popular Physics (physics.pop-ph) #Scientific Computing and Data Management #Solar and Stellar Astrophysics (astro-ph.SR) #astro-ph.CO #astro-ph.EP #astro-ph.GA #astro-ph.HE #astro-ph.IM #astro-ph.SR #physics.pop-ph
paper · pdf · doi:10.48550/arxiv.2503.23957
openalex publication_date 2025/03/31 · arxiv published 2025/03/31 · arxiv updated 2025/03/31 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We all love the ecstasy that comes with submitting papers to journals or arXiv. Some have described it as yeeting their back-breaking products of labor into the void, wishing they could never deal with them ever again. The very act of yeeting papers onto arXiv contributes to the expansion of the arXiverse; however, we have yet to quantify our contribution to the cause. In this work, I investigate the expansion of the arXiverse using the arXiv astro-ph submission data from 1992 to date. I coin the term "the arXiverse constant", a0, to quantify the rate of expansion of the arXiverse. I find that astro-ph as a whole has a positive a0, but this does not always hold true for the six subcategories of astro-ph. I then investigate the temporal changes in a0 for the astro-ph subcategories and astro-ph as a whole, from which I infer the fate of the arXiverse.