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@arXiv_physicsfludyn_bot@mastoxiv.page
2026-05-19 10:06:18

Replaced article(s) found for physics.flu-dyn. arxiv.org/list/physics.flu-dyn
[1/1]:
- On the stability of an in-line formation of hydrodynamically interacting flapping plates
Monika Nitsche, Anand U. Oza, Michael Siegel
arxiv.org/abs/2410.04626 mastoxiv.page/@arXiv_physicsfl
- Side-wall wetting and linear stability of falling films
Hammam Mohamed, J\"orn Sesterhenn
arxiv.org/abs/2504.13300 mastoxiv.page/@arXiv_physicsfl
- An Omni-Temporal Theory for Hydrodynamic Dispersion and Reaction in Porous Media
Md Abdul Hamid, Kyle C. Smith
arxiv.org/abs/2505.06063 mastoxiv.page/@arXiv_physicsfl
- Confirming Wave Turbulence Predictions in Rotating Turbulence
Omri Shaltiel, Omri Gat, Eran Sharon
arxiv.org/abs/2510.25446 mastoxiv.page/@arXiv_physicsfl
- Using Physics Informed Neural Network (PINN) and Neural Network (NN) to Improve a $k-\omega$ Turb...
Lars Davidson
arxiv.org/abs/2511.12493 mastoxiv.page/@arXiv_physicsfl
- Oscillating Detonation of Liquid Ammonia
Wenhao Wang, Zongmin Hu, Peng Zhang
arxiv.org/abs/2511.14167 mastoxiv.page/@arXiv_physicsfl
- On the Poisson-Source Basis of Logarithmic Wall-Pressure-Variance Growth
Jonathan M. O. Massey, Joseph C. Klewicki, Beverley J. McKeon
arxiv.org/abs/2511.16776 mastoxiv.page/@arXiv_physicsfl
- Convolutional causal learning for aerodynamic flows
Ryo Koshikawa, Ryo Araki, Qiong Liu, Kai Fukami
arxiv.org/abs/2601.19104 mastoxiv.page/@arXiv_physicsfl
- Assessing engineering wake models against operational data: insights from the Lillgrund wind farm...
Siguenza-Alvarado, Harrison, Mohammadi, Vishwakarma, Bossanyi, Landberg, Bastankhah
arxiv.org/abs/2601.21035 mastoxiv.page/@arXiv_physicsfl
- Neural equilibria for long-term prediction of nonlinear conservation laws
Benitez, Hegazy, Guo, Dokmani\'c, Mahoney, de Hoop
arxiv.org/abs/2501.06933 mastoxiv.page/@arXiv_csLG_bot/
- Self-similar rupture of thin films of power-law fluid
Michael C Dallaston, Steven A Kedda, Scott W McCue
arxiv.org/abs/2509.05383 mastoxiv.page/@arXiv_condmatso
- Instability and self-propulsion of flexible autophoretic filaments
Ursy Makanga, Akhil Varma, Panayiota Katsamba
arxiv.org/abs/2509.10153 mastoxiv.page/@arXiv_condmatso
- Analytical response functions for a compressible thin fluid layer with odd viscosity
Abdallah Daddi-Moussa-Ider, Yuto Hosaka, Shigeyuki Komura
arxiv.org/abs/2602.18136 mastoxiv.page/@arXiv_condmatso
toXiv_bot_toot

@jswright61@ruby.social
2026-05-23 12:59:09

iOs 26.5 (latest). I have chosen to have messages from unknown callers segregated to their own list. Why are you showing this badge on the list selector glyph. For almost 20 years you’ve trained me that badges warrant my attention. In this case I have expressly indicated I don’t want to know about these. So why are you brining it to my attention?
If I’m expecting a message and I don’t see it, trust me, I’ll seek it out. Until then, let it die in obscurity.

Screenshot of a cropped (showing top) iOs 26.5 messages screen. There is a red arrow and the word “WHY?” Pointing at the menu glyph in the upper right of the screen showing the numeral one inside a blue bubble at about 2 O’Clock on the glyph.
Screenshot of iOs Settings App in the Apps -> Messages screen. A red oval draws attention to the Unknown Senders section and encircles the following text. “Hide notifications and move messages to the Unknown Senders list.
@arXiv_astrophGA_bot@mastoxiv.page
2026-07-21 09:39:17

Replaced article(s) found for astro-ph.GA. arxiv.org/list/astro-ph.GA/new
[1/3]:
- CO Observations of Early-mid Stage Major Mergers in the MaNGA Survey
Yu, Fang, Xu, Feng, Feng, Gao, Jiang, Lisenfeld
arxiv.org/abs/2404.18999 mastoxiv.page/@arXiv_astrophGA
- A first systematic study of [OIII] 88$\mu$m at $z>8$: two luminous oxygen lines and a powerful io...
Hiddo S. B. Algera, et al.
arxiv.org/abs/2512.14486 mastoxiv.page/@arXiv_astrophGA
- Electron temperature relations and the direct N, O, Ne, S and Ar abundances of 49959 star-forming...
D. Scholte, et al.
arxiv.org/abs/2601.02463 mastoxiv.page/@arXiv_astrophGA
- The Role of Inner Halo Angular Momentum (Spin) in Shaping Dark Matter Bars in Milky Way Analogs
Shouvik Ghosh, Sandeep Kumar Kataria
arxiv.org/abs/2601.14420 mastoxiv.page/@arXiv_astrophGA
- GA-NIFS: Dissecting The Alchemised: JWST reveals turbulent metal-poor gas fuelling a co-spatial s...
Robert G. Pascalau, et al.
arxiv.org/abs/2603.00232 mastoxiv.page/@arXiv_astrophGA
- The Star Formation History of WLM from Asymptotic Giant Branch Stars and The Discovery of a Candi...
Abigail J. Lee, Daniel R. Weisz, Andrew E. Dolphin, Alessandro Savino
arxiv.org/abs/2603.00243 mastoxiv.page/@arXiv_astrophGA
- Two Exciting High-redshift Galaxy Candidates Turn Out to Be Two Exciting Ultra-cool Brown Dwarfs
Maru\v{s}a Brada\v{c}, et al.
arxiv.org/abs/2604.23668 mastoxiv.page/@arXiv_astrophGA
- PEARLS: JWST Counterparts of Micro-Jy Radio Sources in the NEP Time Domain Field. II. All Four Sp...
S. P. Willner, et al.
arxiv.org/abs/2605.17040 mastoxiv.page/@arXiv_astrophGA
- Eppur non si trovano Vol. 3: Phoebe -- a Mirage of a Primordial Black Hole
Andrzej Udalski, Przemek Mr\'oz
arxiv.org/abs/2606.19442 mastoxiv.page/@arXiv_astrophGA
- LEGGOS I: The JWST LEGGOS Survey -- LEnsing and Galaxy Growth: Observing Substructures -- Unpacks...
Gourav Khullar, et al.
arxiv.org/abs/2606.20845 mastoxiv.page/@arXiv_astrophGA
toXiv_bot_toot

@fanf@mendeddrum.org
2026-06-18 08:42:02

from my link log —
It is high time we let go of the Mersenne Twister.
arxiv.org/abs/1910.06437
saved 2020-11-20 dotat.at/:/6EPK8.html…

@berlinbuzzwords@floss.social
2026-05-19 13:28:06

Spark for batch, Trino for SQL, Flink for streaming - but how do you run all three safely on the same data? Join @Geetha at #bbuzz26 to explore how Apache Iceberg acts as the shared table layer that makes multi-engine data platforms possible.
Learn more about this session: 2026.berlinbuzzwords.de/sessio
Join us online and in-person at Kulturbrauerei, Berlin.

@Mediagazer@mstdn.social
2026-07-07 15:35:45

In a filing, ABC says the FCC has targeted daytime and late-night TV the administration doesn't like while "leaving untouched the vast landscape of talk radio" (Ted Johnson/Deadline)
deadline.com/2026/07/the-view-

@arXiv_physicsaoph_bot@mastoxiv.page
2026-05-22 07:54:20

From Licensing to Open Access: Designing a Sustainable Transition in Operational Weather Data
Emma Pidduck, Umberto Modigliani, Victoria L. Bennett, Fabio Venuti, Florian Pappenberger, Florence Rabier
arxiv.org/abs/2605.21673 arxiv.org/pdf/2605.21673 arxiv.org/html/2605.21673
arXiv:2605.21673v1 Announce Type: new
Abstract: This translational article documents the European Centre for Medium-Range Weather Forecasts (ECMWF) transition from a restricted data licensing model to open access under CC BY 4.0, completed in October 2025. The policy context included EU open data requirements and alignment with international data exchange frameworks. The transition was implemented through a tiered service model that kept core forecast data open while offering operationally supported delivery as a cost-recovered service. Between 2020 and 2025, ECMWF executed an iterative planning cycle: setting an annual target for revenue reduction, specifying additions to the open tier under that target, provisioning infrastructure, and assessing outcomes to update assumptions. Drawing on internal administrative records (2014 - 2025), we describe design choices, operational constraints, and early outcomes. In the six months following the end of the transition, more than 93% of previously paying organisations retained a Service Agreement, while open endpoint download volumes increased substantially. We discuss trade-offs in defining the open tier (resolution, parameters, schedule), the reduction of compliance overheads formerly associated with redistribution restrictions, and the scalability implications of global distribution. We note an emerging sustainability question as AI-based forecast products become freely available. The early evidence is consistent with the view that a tiered service model can be designed to reconcile open-access obligations with operational sustainability, subject to monitoring over longer contract renewal cycles (typically annual).
toXiv_bot_toot

@Neybulot@pawb.fun
2026-05-19 06:06:19
Content warning: Photo of abs

Feeling pretty good tonight

A picture of my shirt pulled up and abs visible
@berlinbuzzwords@floss.social
2026-05-15 13:08:43

Flink gets talked about a lot. Where does it actually make a difference? Naci Simsek is at #bbuzz26 to share real-world cases where Apache Flink solved concrete, hard problems in production.
Learn more: 2026.berlinbuzzwords.de/sessio

@arXiv_physicsfludyn_bot@mastoxiv.page
2026-05-19 08:13:44

Solutocapillary instability in slipping falling films
Sanghasri Mukhopadhyay, S\'everine Millet, Bastien Di Pierro, Asim Mukhopadhyay
arxiv.org/abs/2605.17519 arxiv.org/pdf/2605.17519 arxiv.org/html/2605.17519
arXiv:2605.17519v1 Announce Type: new
Abstract: We present a comprehensive framework for gravity-driven, surfactant-laden thin films flowing over slippery substrates, elucidating how wall slip modifies the coupled hydrodynamics and interfacial transport. A long-wave model is formulated with a conservative bulk-surface mass balance and a Navier slip condition. The Orr-Sommerfeld eigenvalue problem governs the linear regime, while a weighted-residual model captures the nonlinear evolution over a range of equilibrium surfactant coverages, Marangoni strengths, and adsorption kinetics. The analysis predicts a non-monotonic variation of the critical Reynolds number with equilibrium coverage, exhibiting a maximum at intermediate $\Gamma_e$, and a slip-induced transition from single- to double-hump solitary structures with increasing Marangoni number, accompanied by attenuated capillary ripples. Under fast adsorption kinetics, the surface field homogenizes, preserving the mean film shape and flux while flattening both the surface concentration $\Gamma$ and the bulk inventory $\chi h\phi$. A spurious interfacial mass growth reported by Pascal et al.(PRF, 2019) and D'Alessio et al.(JFM, 2020) is resolved through a revised surface balance ensuring strict conservation. Wall slip thus emerges as a key control parameter, reducing viscous resistance and mitigating Marangoni back-stress. The slip parameter $\beta$ is a useful control knob for surfactant-laden films. Slip prevents fragile multi-hump bound states, promoting a single broad crest or an almost flat, uniform sheet by carefully bonding $\beta$ to wave selection, ripple damping, and the bulk-surface surfactant balance.
toXiv_bot_toot