QB uncertainty for half the NFL next offseason? 16 situations to watch and possible outcomes https://www.espn.com/nfl/story/_/id/49659412/2027-nfl-quarterback-predictions-16-teams-starter-questions-free-agency-trades…
Auch 2030: Telekom bleibt bei der WM am Ball
Die Telekom hat sich auch die Rechte für die nächste Veranstaltung 2030 gesichert. Mehrere Spiele werden trotzdem auch im Free-TV zu sehen sein.
https://www.
“Reacher” star Alan Ritchson had plans to adapt the second book in the popular “Jack Reacher” series for the Prime Video show
— before a certain “someone” got re-elected, he wrote in a comment posted to Threads on Friday.
Responding to a user who wrote that
“every year I’m sad to learn that next season won’t be the book where he kills his way through a white supremacist militia camp,”
Ritchson explained that the novel (titled “Die Trying”) is his “favorite book.”
Injury Didn't Stop CeeDee Lamb From Being Elite Deep Threat for Cowboys in 2025 https://www.si.com/nfl/cowboys/onsi/injury-didnt-stop-ceedee-lamb-elite-deep-threat-dallas-cowboys-2025
Assisting the last mile with smart glasses: towards user-centric LLM prompt engineering for visually impaired people #AI
UPLOAD-ANYON: Progress Towards an Optimised Twisted Anyon Cavity with High-Sensitivity AM-Noise Detection for an Ultralight Axion Dark Matter Search
Robert Crew, Emma Paterson, Maxim Goryachev, Eugene Ivanov, Pashupati Dhakal, Tugrul Talha Ersoz, Michael Tobar, Jeremy Bourhill
https://arxiv.org/abs/2608.19225 https://arxiv.org/pdf/2608.19225 https://arxiv.org/html/2608.19225
arXiv:2608.19225v1 Announce Type: new
Abstract: We propose a superconducting single-mode microwave haloscope based on helical cavity resonators for the detection of ultralight dark matter axions over the mass range $10^{-18}$ to $10^{-13}\,\mathrm{eV}$. Building on the single-mode helical-cavity concept introduced by Bourhill et al. [Phys. Rev. D 108, 052014 (2023); arXiv:2208.01640], we use an inverse-design framework to develop practical resonator geometries compatible with superconducting niobium fabrication. The optimisation employs a figure of merit derived to minimise the measurement time required to achieve a fixed experimental sensitivity. Relative to the heuristic M\"obius-geometry benchmark, the best subtractively manufacturable bulk-niobium design achieves a figure of merit more than three orders of magnitude larger. An experimentally informed microwave interferometric readout model, incorporating measured electronics noise and active suppression of pump amplitude noise, is used to project the sensitivity of the proposed experiment. For an acquisition time of three months, the haloscope is projected to reach $g_{a\gamma\gamma}<10^{-11}\,\mathrm{GeV}^{-1}$ across more than four orders of magnitude in axion mass. The projected sensitivity extends approximately one order of magnitude below the current exclusion limits set by CAST, providing a practical pathway towards a high-sensitivity direct search for ultralight dark matter axions.
toXiv_bot_toot
As of right now, about two thirds of Iowa is in either a severe thunderstorm watch/warning or a tornado watch. The rest is in a “hazardous weather outlook”. Check your local weather and have a source of severe weather alerts this evening.
https://forecast.weather.gov/wwamap/ww
Ah yes, DHH is certainly who we should look towards for how to govern the NixOS foundation. /s
This blog post is the wildest shit I had to read in a while.
https://fzakaria.com/2026/07/18/how-to-piss-off-your-nix-friends
Crosslisted article(s) found for astro-ph.GA. https://arxiv.org/list/astro-ph.GA/new
[1/2]:
- From Triadic Interactions to Kolmogorov Scaling: A Deterministic, Scale-Resolved Formulation of E...
Erik Bertram
https://arxiv.org/abs/2607.16381 https://mastoxiv.page/@arXiv_physicsfludyn_bot/116956890026314972
- Dynamical friction in stratified stellar envelopes
Damien Gagnier
https://arxiv.org/abs/2607.16422 https://mastoxiv.page/@arXiv_astrophSR_bot/116956909457047933
- Simultaneous radio, optical and X-ray monitoring of hard X-ray selected AGN: a variability study
L. Hern\'andez-Garc\'ia, F. Panessa, D. Williams-Baldwin, P. Ar\'evalo, A. M. Mu\~noz Arancibia
https://arxiv.org/abs/2607.16423 https://mastoxiv.page/@arXiv_astrophHE_bot/116956887664818723
- Origin of the Sloshing Spiral in the Abell 2107 Galaxy Cluster
Muhammed K{\i}yami Erdim
https://arxiv.org/abs/2607.16496 https://mastoxiv.page/@arXiv_astrophCO_bot/116956868365097623
- Determination of [Fe/H] in Fundamental mode Classical Cepheids from Gaia DR3 light curve Fourier ...
Roberto Molinaro, et al.
https://arxiv.org/abs/2607.16775 https://mastoxiv.page/@arXiv_astrophSR_bot/116956927940159880
- Escaped White Dwarf Candidates from Open Clusters
Huahui Yan, David R. Miller, Jingkun Zhao, Jincheng Guo, Chengyuan Li
https://arxiv.org/abs/2607.16815 https://mastoxiv.page/@arXiv_astrophSR_bot/116956930692481290
- Magnetic fields in Massive Star-Forming Regions (MagMaR). VIII. Magnetic field overrun by gravity...
M. Fern\'andez-L\'opez, et al.
https://arxiv.org/abs/2607.17160 https://mastoxiv.page/@arXiv_astrophSR_bot/116956996786764707
- Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots
Jun-Rong Liu, Hua Feng, Luis C. Ho
https://arxiv.org/abs/2607.17448 https://mastoxiv.page/@arXiv_astrophHE_bot/116956954089426787
- Binary White Dwarfs as Gravitational Wave Sources for LISA
Sreeta Roy, Surajit Kalita, Tomasz Bulik, Dorota Gondek-Rosi\'nska
https://arxiv.org/abs/2607.17787 https://mastoxiv.page/@arXiv_astrophSR_bot/116957044926341801
- Intracluster light and dark matter halo shapes reflect common assembly, not mutual coupling: shap...
Martin, Hatch, Cui, Fernandez, Bah\'e, Fischer, Montes, Pearce, Sabiu, Yepes, Yoo
https://arxiv.org/abs/2607.17792 https://mastoxiv.page/@arXiv_astrophCO_bot/116956974931041178
toXiv_bot_toot
Injury Didn't Stop CeeDee Lamb From Being Elite Deep Threat for Cowboys in 2025 https://www.si.com/nfl/cowboys/onsi/injury-didnt-stop-ceedee-lamb-elite-deep-threat-dallas-cowboys-2025