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#phaseseparation — Public Fediverse posts

Live and recent posts from across the Fediverse tagged #phaseseparation, aggregated by home.social.

  1. RNA chaperone Hfq assembles into #condensates in response to stress in #Ecoli, but what leads to Hfq’s #PhaseSeparation? This study shows that #polyphosphate scaffolds the formation of Hfq condensates, which then stabilize polyA transcripts critical for recovery @PLOSBiology plos.io/4tI0xby

  2. 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
  3. PRPP amidotransferase (PPAT) is rate-limiting in purine synthesis. This study shows that PPAT forms intracellular #condensates in response to high purine demand via #PhaseSeparation (driven by TORC1-mediated macromolecular crowding of cytoplasm) @PLOSBiology plos.io/3Yw2VVb

  4. Cooking Perfect Cacio e Pepe

    In cooking, sometimes the simplest recipes are the toughest to master. Cacio e pepe — a classic three-ingredient Italian pasta — is an excellent example. Made properly, the sauce of cheese and black pepper combines with starchy water to coat the pasta in a uniform, cheesy sauce. Or, if you’re me, you wind up with a pasta sauce flecked with stringy clumps of melted cheese. Fortunately for those of us who have yet to master this one, a new research paper has us covered with tips to make the perfect cacio e pepe.

    The key to that elusive silky sauce, they found, is the starch – water – cheese combination. Your water needs just the right amount of starch — they found that between 1 – 4% starch by (cheese) mass worked. If the starch concentration is too low (which can easily happen in pasta water), you’ll get the clumpy cheese mess that so frequently happens in my kitchen. Temperature is also critical; if the water is too hot when it’s added, then it can destabilize the sauce. Check out the pre-print’s Section V for the scientific, supposedly foolproof, recipe. I know I’ll be trying it! (Image credit: O. Kadaksoo; research credit: G. Bartolucci et al. pre-print; via APS News)

    #cooking #emulsion #fluidDynamics #phaseSeparation #physics #rheology #science #softMatter

  5. Why Icy Giants Have Strange Magnetic Fields

    When Voyager 2 visited Uranus and Neptune, scientists were puzzled by the icy giants’ disorderly magnetic fields. Contrary to expectations, neither planet had a well-defined north and south magnetic pole, indicating that the planets’ thick, icy interiors must not convect the way Earth’s mantle does. Years later, other researchers suggested that the icy giants’ magnetic fields could come from a single thin, convecting layer in the planet, but how that would look remained unclear. Now a scientist thinks he has an answer.

    When simulating a mixture of water, methane, and ammonia under icy giant temperature and pressure conditions, he saw the chemicals split themselves into two layers — a water-hydrogen mix capable of convection and a hydrocarbon-rich, stagnant lower layer. Such phase separation, he argues, matches both the icy giants’ gravitational fields and their odd magnetic fields. To test whether the model holds up, we’ll need another spacecraft — one equipped with a Doppler imager — to visit Uranus and/or Neptune to measure the predicted layers firsthand. (Image credit: NASA; research credit: B. Militzer; via Physics World)

    #convection #fluidDynamics #Neptune #numericalSimulation #phaseSeparation #physics #planetaryScience #science #Uranus

  6. In developing #presynapses, the #ActiveZone structure assembles via liquid-liquid #PhaseSeparation (#LLPS). This study shows that the #kinase SAD-1 phosphorylates the scaffold protein SYD-2/Liprin-α, relieving autoinhibition & triggering LLPS #PLOSBiology plos.io/3Ne6OZg