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@heiseonline@social.heise.de
2025-07-31 17:01:00

"Ausgereifte" Hintertüren: Nvidia muss sich gegenüber Chinas Regierung erklären
Die Cyberspace Administration of China macht Nvidia schwere Vorwürfe. Die Firma muss beweisen, dass sie keine Hintertüren einsetzt.

@arXiv_mathRA_bot@mastoxiv.page
2025-09-17 08:11:20

A Computation of Tamarkin-Tsygan Calculus
Jun Chen, Xiabing Ruan, Jia Yang
arxiv.org/abs/2509.12984 arxiv.org/pdf/2509.12984

@kurtsh@mastodon.social
2025-09-24 23:52:24

This is an amazing, fascinating, candid & sometimes even funny book.
▶️ "107 Days" by Kamala Harris on Audible
(Narrated by Kamala Harris)
audible.com/pd/B0FFD25MJV?sour

@tante@tldr.nettime.org
2025-09-21 11:00:05

"Our government is being run by aggrieved elites who were thrown onto social platforms with everyone else in the 2010s, where they could finally read what we all think about them. And it caused them so much psychic damage that they have decided to destroy both the internet and democracy to make sure nothing like it will ever happen again."
(Original title: Petty, powerful, and pathologically online)

@arXiv_astrophGA_bot@mastoxiv.page
2025-10-08 09:57:49

A Comparison of Star Formation Rates by Different Tracers in Nearby Galaxies
Huynh Anh N. Le, Jong-Hak Woo, Yongquan Xue, Ashraf Ayubinia, Changseok Kim, Xiaozhi Lin
arxiv.org/abs/2510.05687

@arXiv_condmatstrel_bot@mastoxiv.page
2025-08-07 08:35:53

Cooperative Jahn-Teller dynamics of boron clusters in the infrared conductivity of heavy fermion metal CeB6 and unconventional superconductor ZrB12
Gennady Komandin, Elena Zhukova, Boris Gorshunov, Andrey Azarevich, Andrey Muratov, Yurii Aleshchenko, Nikolay Sluchanko
arxiv.org/abs/2508.04238

@arXiv_hepph_bot@mastoxiv.page
2025-07-24 09:18:09

Anisotropic flow coefficients for charged hadrons in $O O$ collisions at $\sqrt{s_{\mathrm{NN}}}=7$ TeV using AMPT
Jagbir Singh, Muhammad Usman Ashraf, Ahsan Mehmood Khan, Aditya Rana, Sonia Kabana
arxiv.org/abs/2507.17400

@arXiv_nuclth_bot@mastoxiv.page
2025-07-23 08:48:02

Strangeness production in $O O$ collisions at $\sqrt{s_{\mathrm{NN}}}=7$ TeV using various model approaches
J. Singh, M. U. Ashraf, A. M. Khan, S. Kabana
arxiv.org/abs/2507.16266