Triggering star formation : experimental compression of a foam ball induced by Taylor-Sedov blast waves
Matter and Radiation at Extremes AIP Publishing 7:3 (2022) 036902
Abstract:
The interaction between a molecular cloud and an external agent (e.g., a supernova remnant, plasma jet, radiation, or another cloud) is a common phenomenon throughout the Universe and can significantly change the star formation rate within a galaxy. This process leads to fragmentation of the cloud and to its subsequent compression and can, eventually, initiate the gravitational collapse of a stable molecular cloud. It is, however, difficult to study such systems in detail using conventional techniques (numerical simulations and astronomical observations), since complex interactions of flows occur. In this paper, we experimentally investigate the compression of a foam ball by Taylor–Sedov blast waves, as an analog of supernova remnants interacting with a molecular cloud. The formation of a compression wave is observed in the foam ball, indicating the importance of such experiments for understanding how star formation is triggered by external agents.First Search for Unstable Sterile Neutrinos with the IceCube Neutrino Observatory
(2022)
Magnetized laser–plasma interactions in high-energy-density systems: Parallel propagation
Physics of Plasmas AIP Publishing 29:4 (2022) 042113
Time-resolved hadronic particle acceleration in the recurrent nova RS Ophiuchi.
Science (New York, N.Y.) 376:6588 (2022) 77-80
Abstract:
Recurrent novae are repeating thermonuclear explosions in the outer layers of white dwarfs, due to the accretion of fresh material from a binary companion. The shock generated when ejected material slams into the companion star's wind can accelerate particles. We report very-high-energy (VHE; [Formula: see text]) gamma rays from the recurrent nova RS Ophiuchi, up to 1 month after its 2021 outburst, observed using the High Energy Stereoscopic System (H.E.S.S.). The temporal profile of VHE emission is similar to that of lower-energy giga-electron volt emission, indicating a common origin, with a 2-day delay in peak flux. These observations constrain models of time-dependent particle energization, favoring a hadronic emission scenario over the leptonic alternative. Shocks in dense winds provide favorable environments for efficient acceleration of cosmic rays to very high energies.Search for GeV-scale dark matter annihilation in the Sun with IceCube DeepCore
Physical Review D American Physical Society (APS) 105:6 (2022) 062004