Universal hepatitis B vaccination at birth – risks of revising the recommendation
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Updates every hour. Last Updated: 5-Dec-2025 08:11 ET (5-Dec-2025 13:11 GMT/UTC)
Scientists find that pure mathematical formulae used to calculate the value of pi 100 years ago has connections to fundamental physics of today – showing up in theoretical models of percolation, turbulence, and certain aspects of black holes
Researchers examined five AI models on multiple genomic tasks to see how well they performed
Models performed well overall, with each having strengths and weaknesses based on the desired task
Study provides a framework for researchers to choose optimal AI models for specific genomic tasks
Physicists and mathematicians at the University of Konstanz, ETH Zürich (Switzerland) and CNR INO in Trento (Italy) use concepts from topography to topologically classify and investigate driven-dissipative nonlinear systems and their abrupt phase transitions. To explain how this works, they use the image of a mountainous landscape.
In a paper published in Acta Mathematica Scientia, a mathematics team led by H.-L. Li in Capital Normal University investigated the linear stability/instability of the planar Couette flow to the two-dimensional compressible Euler-Euler system for (ρ, u) and (n, v) with the sound speeds c1 and c2 respectively coupled each other through the drag force on T×R. It is shown in general for the different sound speeds c1≠c2 that the perturbations of the densities (ρ, n) and the velocities (u, v) demonstrate the stability in any fixed finite time interval (0, T], besides, excluding the zero mode, the densities (ρ, n) and the irrotational components of the velocities (u, v) obey the algebraic time-growth rates, while the rotational components of the velocities (u, v) exhibit the algebraic time-decay rates due to the inviscid damping. For the case of same sound speeds c1=c2 (same sound speeds), it is proved that the relative velocity u − v decays faster than those of the velocities u, v caused by the inviscid damping, but the linear instability of the densities (ρ, n) and the irrotational components of the velocities (u, v) is also shown for some large time in spite of the inviscid damping.