May has been another busy month of security updates, with Google’s Chrome browser and Android operating system, Zoom, and Apple’s iOS releasing patches to fix serious vulnerabilities. Here’s what you need to know. Via WIREDUK
the Samsung Galaxy S22, Galaxy S22+, and Galaxy S22 Ultra, as well as the Galaxy Tab S8 series, the Galaxy Watch 4 series, and the Galaxy S21 series., this time for 32 issues, of which one is rated as critical and eight are deemed high severity. The critical issue, CVE-2022-1853, impacts the IndexedDB feature, while the high-rated flaws affect areas that include DevTools, UI foundations, and the user education function.
, when the company issue emergency updates to fix several already exploited vulnerabilities in its Chromium-based browser. Earlier in May, Google released 13 fixes in Chrome v101.0.4951.61 for Android, with eight of these rated as having a high-severity impact.in Cisco Enterprise NFV Infrastructure Software that could allow an attacker to escape from the guest virtual machine to the host machine, inject commands that execute at the root level, or leak system data from the host to the virtual machine.
It goes without saying that these high-severity issues—tracked as CVE-2022-20777, CVE-2022-20779, and CVE-2022-20780—are serious, so it’s a good idea to update as soon as possible.in mid-May for its Nvidia GPU display driver to fix flaws that could allow denial of service, information disclosure, or data tampering. The list of 10 vulnerabilities includes issues in the Kernel mode layer on Windows and Linux devices.
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Deep Zoom-In Simulation of a Fuzzy Dark Matter Galactic HaloFuzzy dark matter (FDM) made of ultralight bosonic particles is a viable alternative to cold dark matter with clearly distinguishable small-scale features in collapsed structures. On large scales, it behaves gravitationally like cold dark matter deviating only by a cutoff in the initial power spectrum and can be studied using $N$-body methods. In contrast, wave interference effects near the de Broglie scale result in new phenomena unique to FDM. Interfering modes in filaments and halos yield a stochastically oscillating granular structure which condenses into solitonic cores during halo formation. Investigating these highly nonlinear wave phenomena requires the spatially resolved numerical integration of the Schr\'odinger equation. In previous papers we introduced a hybrid zoom-in scheme that combines $N$-body methods to model the large-scale gravitational potential around and the mass accretion onto pre-selected halos with simulations of the Schr\'odinger-Poisson equation to capture wave-like effects inside these halos. In this work, we present a new, substantially improved reconstruction method for the wave function inside of previously collapsed structures. We demonstrate its capabilities with a deep zoom-in simulation of a well-studied sub-${L}_{*}$-sized galactic halo from cosmological initial conditions. With a particle mass of $m=2.5\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}22}\text{ }\text{ }\mathrm{eV}$ and halo mass ${M}_{\mathrm{vir}}=1.7\ifmmode\times\else\texttimes\fi{}{10}^{11}\text{ }\text{ }{M}_{\ensuremath{\bigodot}}$ in a $(60\text{ }\text{ }{\mathrm{h}}^{\ensuremath{-}1}\text{ }\text{comoving Mpc}{)}^{3}$ cosmological box, it reaches an effective resolution of 20 comoving pc. This pushes the values of $m$ and $M$ accessible to simulations significantly closer to those relevant for studying galaxy evolution in the allowed range of FDM masses.
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