📄 Star formation and feedback in smoothed particle hydrodynamic simulat…

Quicklook:
Stinson, Greg et al. (2006) · Monthly Notices of the Royal Astronomical Society
Reads: 176 · Citations: 732
DOI: 10.1111/j.1365-2966.2006.…

🔗 https://ui.adsabs.harvard.edu/abs/2006MNRAS.373.1074S/abstract

#Astronomy #Astrophysics #Galaxies #Supernovae #Hydrodynamics

Star formation and feedback in smoothed particle hydrodynamic simulations - I. Isolated galaxies

We present an analysis of star formation and feedback recipes appropriate for galactic smoothed particle hydrodynamics simulations. Using an isolated Milky Way-like galaxy, we constrain these recipes based on well-established observational results. Our star formation recipe is based on that of Katz with the additional inclusion of physically motivated supernova feedback recipes. We propose a new feedback recipe in which Type II supernovae are modelled using an analytical treatment of blastwaves. With this feedback mechanism and a tuning of other star formation parameters, the star formation in our isolated Milky Way-like galaxy follows the slope and normalization of the observed Schmidt law. In addition, we reproduce the low-density cut-off and filamentary structure of star formation observed in disc galaxies. Our final recipe will enable better comparison of N-body simulations with observations.

ADS

Fluid Flows Break Up Microswimmer Clumps

The field of active matter looks at the collective motion of particles and organisms–how birds flock and fish school. In systems of “dry” squirmers–those that have no hydrodynamic interactions with one another–clumps of squirmers can form with empty spaces in between them. This is known as motility-induced phase separation, or MIPS. Researchers wondered whether microswimmers in a fluid–which do produce hydrodynamic forces that can affect one another–would also show MIPS.

In a new study, researchers show, instead, that hydrodynamic interactions between swimmers will prevent (or destroy) these clumps. Through a combination of theoretical work and simulation, the authors found that translational flows between swimmers swept the swimmers out of clumps as they formed. Rotational flows between swimmers made them able to change direction faster, which also kept stable clumps from forming. (Image and research credit: T. Zhou and J. Brady; via APS)

Hydrodynamic interactions destroy clumps of microswimmers. This simulation shows microswimmers that are initially in a clumped formation before hydrodynamic interactions are “turned on”. Once the swimmers can affect one another through the flows their motion creates, the clumps quickly break apart. #activeMatter #biology #collectiveMotion #fluidDynamics #hydrodynamics #microswimmers #phaseSeparation #physics #science

How do fluids really slip on surfaces?

This study proposes a method to estimate slip length and reconstruct flow fields from limited data.

A key step to better understand flows where friction at the wall nearly vanishes.

🔗 https://pubs.aip.org/aip/pof/article-abstract/38/3/033605/3382598/Slip-length-estimation-and-flow-reconstruction?redirectedFrom=fulltext

#fluiddynamics #interfacialflows #SlipLength #hydrodynamics #physics

Open-source software advances design of offshore structures by testing wave-structure interactions

A Cornell doctoral student has developed an open-source software package that could transform how engineers design floating offshore structures for renewable energy and other ocean applications.

Tech Xplore

An aircraft that can reduce fuel burn by over 60% by using "laminar-flow aerodynamics" (as well as other technologies like "precision all-carbon-fiber composites") has been produced, or so it is claimed, by an aerospace startup company, Otto Aerospace, which announced its first fleet customer will be Flexjet, although deliveries won't begin until 2030.

https://ottoaerospace.com/news/otto-aerospace-secures-historic-300-aircraft-order-with-flexjet/

#aerospace #aviation #hydrodynamics

Otto Aerospace

The Otto Aerospace Phantom 3500 is a masterpiece of engineering— utilizing groundbreaking laminar flow technology, digital design tools, and modern manufacturing techniques to achieve unparalleled efficiency, luxury, and environmental stewardship. Designed for leaders, visionaries, and innovators, the Phantom 3500 sets a new standard in private jet flight where performance and sustainability exist in perfect harmony.

Otto Aerospace
Engineers Create Soft Robots That Can Literally Walk on Water

Scientists have developed HydroSpread, a novel technique for building soft robots on water, with wide-ranging possibilities in robotics, healthcare, and environmental monitoring. Picture a miniature robot, no larger than a leaf, gliding effortlessly across the surface of a pond, much like a water

SciTechDaily

Check out this absolute stonker of a figure by Philippe Delache in 1977.

(I originally found the figure reproduced in the textbook Turbulence by Uriel Frisch. I have it hanging on my office wall...)

This post inspired by @grimalkina talking about hiking and flow(s) in a totally different context.

#hydrodynamics #physics #climbing

Galiliean-invariant hydrodynamical simulations on a moving mesh

Weekly Update from the Open Journal of Astrophysics – 24/05/205

It’s  time once again for the regular Saturday update of papers published during the past week at the Open Journal of Astrophysics. Since the last update we have published three new papers, which brings the number in Volume 8 (2025) up to 62 and the total so far published by OJAp up to 297.

In chronological order of publication, the three papers published this week, with their overlays, are as follows. You can click on the images of the overlays to make them larger should you wish to do so.

The first paper to report is: “Jet-shaped filamentary ejecta in common envelope evolution” by Ron Schreier, Shlomi Hillel and Noam Soker (Technion, Haifa, Israel). This paper, which was published on Monday May 19th 2025 in the folder High-Energy Astrophysical Processes, presents three-dimensional hydrodynamical simulations of common envelope evolution of a neutron star inside the envelope of a rotating red supergiant with Rayleigh-Taylor instabilities forming filamentary ejecta.

The overlay is here:

You can find the officially accepted version on arXiv here.

Second one up is “Weighing The Options: The Unseen Companion in LAMOST J2354 is Likely a Massive White Dwarf” by M. A. Tucker, A. J. Wheeler & D. M. Rowan (Ohio State University, USA) and M. E. Huber (U. Hawaii, USA). This paper was published on Tuesday 20th May 2025 in the folder for Solar and Stellar Astrophysics. It discusses a spectroscopic study of the binary system LAMOST J235456.73+335625 (J2354) with a discussion of the implications for the nature of the dark component.

The overlay is here:

 

You can find the officially-accepted version of the paper on arXiv here.

The third and last paper of the week, published on Thursday May 22nd 2025, also in the folder Solar and Stellar Astrophysics, is “How to use Gaia parallaxes for stars with poor astrometric fits” by Kareem El-Badry (Caltech, USA).  This paper presents a method for extracting reasonable estimates of stellar parallaxes from Gaia data when the overall astrometric solution is unreliable due to errors and noise

Here is the overlay:

You can find the officially accepted version of this paper on arXiv here.

That’s all the papers for this week. Looking at the publishing workflow, I expect we will pass the 300 mark next week. We’ll see when I post the next update next Saturday.

 

#arXiv240719004v2 #arXiv250109663v3 #arXiv250411528v2 #astrometry #binaryStars #commonEnvelopeEvolution #DiamondOpenAccess #GAIA #HighEnergyAstrophysicalPhenomena #hydrodynamics #LAMOSTJ2354 #LAMOSTJ23545673335625 #OpenJournalOfAstrophysics #parallax #SolarAndStellarAstrophysics #stars #TheOpenJournalOfAstrophysics #whiteDwarfs