Tootfinder

Asymptotics of shortest filling closed multi-geodesics
Yue Gao, Zhongzi Wang, Yunhui Wu
https://arxiv.org/abs/2508.17566 https://arxiv.org/pdf/2508.17566…

Asymptotics of shortest filling closed multi-geodesics
In this paper, we investigate the asymptotics of shortest filling closed multi-geodesics of closed hyperbolic surfaces as systole $\to 0$ or as genus $\to \infty$. We first show that for a closed hyperbolic surface $X_g$ of genus $g$, the length of a shortest filling closed multi-geodesic of $X_g$ is uniformly comparable to $$\left(g+\sum\limits_{\textit{closed geodesic }γ\subset X_g, \ \ell(γ)<1}\log \left(\frac{1}{\ell(γ)}\right)\right).$$ As an application, we show that as $g\to \infty$, …

Number of #bitnami container images in the #homelab cluster: 4
Number of #bitnami container images to remove: 3

When do you start feeling like a person and not a collection of impulses you don’t understand?

Crosslisted article(s) found for math.DG. https://arxiv.org/list/math.DG/new
[1/1]:
- Asymptotics of shortest filling closed multi-geodesics
Yue Gao, Zhongzi Wang, Yunhui Wu

An absolute curtain of rain closed in and caused a delay. It soon passed and the game was able to resume.
At 3-2, it was a narrower victory for the home team, the Salem Red Sox, than it ought to have been. The Carolina Mudcats had 6 errors. There could have been a 7th, but the scorers must have felt some charity for a duffed ball at 3B and let it slide.
Single A baseball is that of dream chasers and prospect pitching, not necessarily brilliant talent and discipline.

The Persistence of Nonlinear Gravitational Wave Memory
Robert R. Caldwell
https://arxiv.org/abs/2506.20751 https://arxiv.org/pdf/2506…

The Persistence of Nonlinear Gravitational Wave Memory
Nonlinear gravitational wave memory is a surprise of theoretical physics. Whereas it is understood that a gravitational wave induces oscillatory squeezing and stretching motion in a collection of freely-falling test masses, it is unexpected that the wave leaves a residual displacement of the test masses. This displacement is the tribute in memoriam to the passing wave. The memory originates in a nonlinear feature of gravitation. Whilst merging black holes are a significant source of gravitation…

3C 403: a candidate neutrino-emitting radio galaxy
Gabriele Bruni, Loredana Bassani, Sergio Alves Garre, Manuela Molina, Angela Malizia, Mariateresa Fiocchi, James Rodi, Antoine Kouchner, Alexis Coleiro, Julien Aublin, Giulia Illuminati, Francesca Panessa, Angela Bazzano, Lorenzo Natalucci, Pietro Ubertini
https://arxiv.org/abs/…

3C 403: a candidate neutrino-emitting radio galaxy
3C 403 is a well known FRII radio galaxy, whose jets extend up to the kpc scale. In this letter, we present its identification as the second most significant source among the more than 150 inspected using the 15-year neutrino dataset of the ANTARES Collaboration, possibly making it the first radio galaxy with neutrino emission. Following the previous association of blazars with netrinos events, we aimed at studying the jet properties and its possible role in neutrino production. We collected mu…

The life and times of dark matter haloes: what will I be when I grow up?
Julian Onions, Frazer Pearce, Alexander Knebe, Meghan Gray, Roan Haggar, Ulrike Kuchner, Ana Contreras-Santos, Gustavo Yepes, Weiguang Cui
https://arxiv.org/abs/2508.18778

The life and times of dark matter haloes: what will I be when I grow up?
Are the most massive objects in the Universe today the direct descendants of the most massive objects at higher redshift? We address this question by tracing the evolutionary histories of haloes in the MultiDark Planck2 simulation. By following the 100 most massive halos at $z = 0$ across cosmic time, we find that only 40\% of them were among the largest 100 halos at $z = 1$. This suggests that many of today's most massive clusters were not the most dominant structures at earlier times, while s…

Search for $\chi_{c1}\to \pi^{ }\pi^{-}\eta_c$ via $\psi(3686)\to\gamma\chi_{c1}$
BESIII Collaboration, et al.
https://arxiv.org/abs/2508.18601 https://arx…

Search for $χ_{c1}\to π^{+}π^{-}η_c$ via $ψ(3686)\toγχ_{c1}$
Utilizing $(2712.4 \pm 14.3) \times 10^6$ $ψ(3686)$ events collected with the BESIII detector at the BEPCII collider, we search for the hadronic transition process $χ_{c1} \to π^+π^-η_c$ following the decay $ψ(3686)\to γχ_{c1}$. No significant signal is observed, and an upper limit of $\mathcal{B}(χ_{c1}\toπ^+π^-η_c)$ is determined to be $3.1 times 10^{-4}$~at 90\% confidence level, which is one order of magnitude more stringent than the previous measurement.

Last Thursday, the movers ultimately arrived and did an awesome job, emptying the house and garage in 3 hours. The house sale closed with no issues on Friday at 5pm. Today, Monday the 23rd, our house purchase should close mid to late afternoon. Tomorrow, the moving truck arrives to dump our possessions into various rooms. We're almost there...
#NewBeginnings #FeelinGood
https://youtu.be/Edwsf-8F3sI?si=FDM6ees_yO_DqqCE