[2606.04044] The Cosmological Hart-Tipler Conjecture
-->
Astrophysics > Cosmology and Nongalactic Astrophysics
arXiv:2606.04044 (astro-ph)
[Submitted on 2 Jun 2026]
Title:The Cosmological Hart-Tipler Conjecture
Authors:David Kipping<br>View a PDF of the paper titled The Cosmological Hart-Tipler Conjecture, by David Kipping
View PDF<br>HTML (experimental)
Abstract:Self-reproducing automata, so-called von Neumann machines, have been repeatedly estimated to be capable of traversing the Galaxy many times given its age. Our mere existence thus seems to exclude an aggressive variant of such a probe having ever been launched in the Milky Way. The Hart-Tipler conjecture considers this to represent contra-positive evidence to the hypothesis that other extra-terrestrial technological entities have emerged in our galaxy. Recently, several authors have extended interstellar colonization calculations to cosmological volumes, but these models are loaded with specific assumptions about behavior and emergence times. Here, we present a bare-bones model of generic artificial infections (such as but not limited to von Neumann probes) at cosmological scale in order to maximize interpretability, an approach closer to the original spirit of the Hart-Tipler calculations. Our model has just three parameters, a spontaneous spawn rate, a propagation speed (u) and a start time for the calculation. Accounting for cosmological expansion, we find that half the Universe is infected by today for u=0.1c propagation starting 4.5 Gyr after the Big Bang if the spawn rate exceeds approximately once per million galaxies. For near-c propagation, this becomes a billion galaxies. Over 99.9% of cosmological volumes are filled with 0.1c if even 1-in-100,000 galaxies have ever spawned an infection. The "cosmological Hart-Tipler" problem therefore offers a remarkably sharp minimal-model constraint on the prevalence of aggressive, self-propagating technological behavior. We explore its implications, such as how anthropic reasoning implies such infections occur and its fine-tuning nature.
Comments:<br>Submitted to Astrobiology. Compiled in AASTeX Modern
Subjects:
Cosmology and Nongalactic Astrophysics (astro-ph.CO); Astrophysics of Galaxies (astro-ph.GA); Popular Physics (physics.pop-ph)
Cite as:<br>arXiv:2606.04044 [astro-ph.CO]
(or<br>arXiv:2606.04044v1 [astro-ph.CO] for this version)
https://doi.org/10.48550/arXiv.2606.04044
Focus to learn more
arXiv-issued DOI via DataCite
Submission history<br>From: David Kipping [view email]<br>[v1]<br>Tue, 2 Jun 2026 07:01:20 UTC (292 KB)
Full-text links:<br>Access Paper:
View a PDF of the paper titled The Cosmological Hart-Tipler Conjecture, by David Kipping<br>View PDF<br>HTML (experimental)<br>TeX Source
view license
Current browse context:
astro-ph.CO
next >
new<br>recent<br>| 2026-06
Change to browse by:
astro-ph<br>astro-ph.GA<br>physics<br>physics.pop-ph
References & Citations
INSPIRE HEP
NASA ADS<br>Google Scholar
Semantic Scholar
export BibTeX citation<br>Loading...
BibTeX formatted citation
×
loading...
Data provided by:
Bookmark
Bibliographic Tools
Bibliographic and Citation Tools
Bibliographic Explorer Toggle
Bibliographic Explorer (What is the Explorer?)
Connected Papers Toggle
Connected Papers (What is Connected Papers?)
Litmaps Toggle
Litmaps (What is Litmaps?)
scite.ai Toggle
scite Smart Citations (What are Smart Citations?)
Code, Data, Media
Code, Data and Media Associated with this Article
alphaXiv Toggle
alphaXiv (What is alphaXiv?)
Links to Code Toggle
CatalyzeX Code Finder for Papers (What is CatalyzeX?)
DagsHub Toggle
DagsHub (What is DagsHub?)
GotitPub Toggle
Gotit.pub (What is GotitPub?)
Huggingface Toggle
Hugging Face (What is Huggingface?)
ScienceCast Toggle
ScienceCast (What is ScienceCast?)
Demos
Demos
Replicate Toggle
Replicate (What is Replicate?)
Spaces Toggle
Hugging Face Spaces (What is Spaces?)
Spaces Toggle
TXYZ.AI (What is TXYZ.AI?)
Related Papers
Recommenders and Search Tools
Link to Influence Flower
Influence Flower (What are Influence Flowers?)
Core recommender toggle
CORE Recommender (What is CORE?)
IArxiv recommender toggle
IArxiv Recommender<br>(What is IArxiv?)
Author
Venue
Institution
Topic
About arXivLabs
arXivLabs: experimental projects with community collaborators
arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website.
Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them.
Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs .
Which authors of this paper are endorsers? |<br>Disable MathJax (What is MathJax?)