Talk:Dark matter
Add topic| This is the talk page for discussing improvements to the Dark matter article. This is not a forum for general discussion of the subject of the article. |
Article policies
|
| Find sources: Google (books · news · scholar · free images · WP refs) · FENS · JSTOR · TWL |
| Archives (index): 1, 2, 3, 4, 5, 6, 7, 8Auto-archiving period: 3 months |
| Dark matter was one of the Natural sciences good articles, but it has been removed from the list. There are suggestions below for improving the article to meet the good article criteria. Once these issues have been addressed, the article can be renominated. Editors may also seek a reassessment of the decision if they believe there was a mistake. | ||||||||||||||||
| ||||||||||||||||
| Current status: Delisted good article | ||||||||||||||||
| This It is of interest to the following WikiProjects: | ||||||||||||||||||||||||
| ||||||||||||||||||||||||
This article has been mentioned by a media organization:
|
| Dark matter in fiction was merged into this article. The discussion was closed on 11 December 2022 with a consensus to merge. The original page is now a redirect to this article. Its history now serves to provide attribution for the content in this article, and it must not be deleted as long as this article exists. |
Equilibrium Energy Partition and Planck–Like Universality in Galactic Rotation Curves
[edit]This article presents a new approach for explaining galactic rotation curves without dark matter. The framework is based on equilibrium energy partition and suggests a universal Planck-like relation governing rotational dynamics.
ResearchGate:
- DOI:
DOI: 10.5281/zenodo.18555947
Zenodo:
https://doi.org/10.5281/zenodo.18555947 ~2026-15634-57 (talk) 06:39, 12 March 2026 (UTC)
- These days theories that explain galactic rotation curves without dark matter are dime a dozen. The new theory would need to explain something more (especially the cosmological evidence) for me to pay attention. Banedon (talk) 08:51, 12 March 2026 (UTC)
Did Voyager 1 really measure Hawking radiation? Is that a prank?
[edit]Someone knowledgeable please verify this statement, in the first sentence of 4th paragraph of section "Primordial black holes"
On 5-May and 10-May-2026, it reads:
"Various observational constraints, such as gravitational microlensing data from the Subaru Telescope (HSC) and Voyager 1 measurements of Hawking radiation, have ruled out PBHs constituting 100% of dark matter in specific mass windows (e.g., evaporating tiny black holes or monochromatic intermediate-mass populations).[162]"
The second part of that sentence feels like a prank. [162] corroborates the Subaru Telescope part, but nothing corroborates the "Voyager 1 measurements of Hawking radiation" part. Neither the linked "Voyager 1" nor the "Hawking radiation" article state this, either. The latter makes it quite unlikely that Voyager 1 could measure it. Karl Missouri (talk) 19:28, 10 May 2026 (UTC)
- Pretty sure you are right. Too bad it's not so. Interesting times for resolving the Hubble "constant" dilemma. Pete Tillman (talk) 19:38, 10 May 2026 (UTC)
- Thank you. I found a reference for Voyager 1 data being used to constrain the amount of tiny PBHs, and added it as reference. Karl Missouri (talk) 14:06, 11 May 2026 (UTC)
- Delisted good articles
- Old requests for peer review
- B-Class level-4 vital articles
- Wikipedia level-4 vital articles in Physical sciences
- B-Class vital articles in Physical sciences
- B-Class Astronomy articles
- Top-importance Astronomy articles
- B-Class Astronomy articles of Top-importance
- B-Class Cosmology articles
- B-Class physics articles
- Top-importance physics articles
- B-Class physics articles of Top-importance
