Tootfinder

this might be one of the _least_ specific (but not completely non-specific) paragraphs in any specification i've ever read

celegans_metabolic: Metabolic network (C. elegans)
List of edges comprising the metabolic network of the nematode C. elegans.
This network has 453 nodes and 4596 edges.
Tags: Biological, Metabolic, Unweighted
https://networks.skewed.de/net/celegans_metabolic

At peace after collision, Falcons' Carter breaks out https://www.espn.com/nfl/story/_/id/45991741/falcons-rookie-rb-carter-shines-week-scary-collision

Scattering Theory in Noncanonical Phase Space: A Drift-Kinetic Collision Operator for Weakly Collisional Plasmas
Naoki Sato, Philip J. Morrison
https://arxiv.org/abs/2506.11215

Scattering Theory in Noncanonical Phase Space: A Drift-Kinetic Collision Operator for Weakly Collisional Plasmas
After developing a scattering theory for grazing collisions in general noncanonical phase spaces, we introduce a guiding center collision operator in five-dimensional phase space designed for plasma regimes characterized by long wavelengths (relative to the Larmor radius), low frequencies (relative to the cyclotron frequency), and weak collisionality (where repeated Coulomb collisions induce cumulatively small changes in particle magnetic moment). The collision operator is fully determined by t…

celegans_metabolic: Metabolic network (C. elegans)
List of edges comprising the metabolic network of the nematode C. elegans.
This network has 453 nodes and 4596 edges.
Tags: Biological, Metabolic, Unweighted
https://networks.skewed.de/net/celegans_metabolic

Finally got around to replacing the twitter links in my legislation repo with better ones:
https://github.com/cooljeanius/legislation/compare/b97b056082401d555eb3c186f6257d28b8d795c2...1a457d1969a6c98a1b152a636add19a214dd70b1

The real collusion between Donald Trump and Vladimir Putin (The Economist)
https://www.economist.com/united-states/2025/08/14/the-real-collusion-between-donald-trump-and-vladimir-putin
http://www.memeorandum.com/250815/p45#a250815p45

Collision-induced mass loss and mass gain on an extremely massive star. An analytical approach and a static proto-globular cluster test-case
Laura Ram\'irez-Galeano, Corinne Charbonnel, Tassos Fragos, Zouba\"ir Tazakkati, Jaime Roman-Garza, Mark Gieles
https://arxiv.org/abs/2506.12132

Collision-induced mass loss and mass gain on an extremely massive star. An analytical approach and a static proto-globular cluster test-case
The objective of this study is to analytically explore mass loss and gain induced by stellar collisions on a gas-accreting extremely massive star (aEMS, 10^3 <= M/M_sun <= 10^4). We also consider its contribution to the mass budget in the context of forming multiple stellar populations in a typical protoglobular cluster. We used MESA to build a series of aEMS models up to 2e4 M_sun for three [Fe/H] values, covering the metallicity range of Galactic GCs, with different treatments of super-adiaba…

A Learning Framework For Cooperative Collision Avoidance of UAV Swarms Leveraging Domain Knowledge
Shuangyao Huang, Haibo Zhang, Zhiyi Huang
https://arxiv.org/abs/2507.10913

A Learning Framework For Cooperative Collision Avoidance of UAV Swarms Leveraging Domain Knowledge
This paper presents a multi-agent reinforcement learning (MARL) framework for cooperative collision avoidance of UAV swarms leveraging domain knowledge-driven reward. The reward is derived from knowledge in the domain of image processing, approximating contours on a two-dimensional field. By modeling obstacles as maxima on the field, collisions are inherently avoided as contours never go through peaks or intersect. Additionally, counters are smooth and energy-efficient. Our framework enables tr…

Making the Subdominant Dominant: Gravothermal Pile-Up of Collisional Dark Matter Around Compact Objects
Reza Ebadi, Erwin H. Tanin
https://arxiv.org/abs/2507.11601

Making the Subdominant Dominant: Gravothermal Pile-Up of Collisional Dark Matter Around Compact Objects
The dark matter may consist of multiple species that interact differently. We show that a species that is cosmologically subdominant but highly collisional can pile up and become dominant in deep gravitational wells, such as those of white dwarfs and neutron stars.