296 citations
- Niels BrockDK4 papers
- Queen Mary University of LondonGB2 papers
- University of CopenhagenDK2 papers
- Aarhus UniversityDK1 paper
- Columbia UniversityUS1 paper
- European Southern ObservatoryCL1 paper
- Flatiron Health (United States)US1 paper
- Flatiron Institute1 paper
- Jet Propulsion LaboratoryUS1 paper
- Leibniz Institute for Astrophysics PotsdamDE1 paper
- Leiden UniversityNL1 paper
- Lund UniversitySE1 paper
9 papers
Braided mixing in confined chiral active matter
Yue Wang, Jonas Berx
Efficient mixing of fluids is essential in many practical applications to achieve homogeneity. For microscopic systems, however, both diffusion and turbulence are ineffective metho…
Subphotospheric emission from short gamma-ray bursts: Protons mold the multi-messenger signals
Annika Rudolph, Irene Tamborra, Ore Gottlieb
The origin of the observed Band-like photon spectrum in short gamma-ray bursts (sGRBs) is a long-standing mystery. We carry out the first general relativistic magnetohydrodynamic s…
Streaming Instability for Particle-Size Distributions
Leonardo Krapp, Pablo Benítez-Llambay, Oliver Gressel +1
The streaming instability is thought to play a central role in the early stages of planet formation by enabling the efficient bypass of a number of barriers hindering the formation…
Photophoretic Levitation and Trapping of Dust in the Inner Regions of Protoplanetary Disks
Colin P. McNally, Melissa K. McClure
In protoplanetary disks, the differential gravity-driven settling of dust grains with respect to gas and with respect to grains of varying sizes determines the observability of gra…
Misaligned Disks in the Binary Protostar IRS 43
Christian Brinch, Jes K. Jørgensen, Michiel R. Hogerheijde +2
Recent high angular resolution (0.2") ALMA observations of the 1.1 mm continuum and of HCO+ J=3-2 and HCN J=3-2 gas towards the binary protostar IRS 43 reveal multiple Kepler…
Sustained Turbulence in Differentially Rotating Magnetized Fluids at Low Magnetic Prandtl Number
Farrukh Nauman, Martin E. Pessah
We show for the first time that sustained turbulence is possible at low magnetic Prandtl number for Keplerian flows with no mean magnetic flux. Our results indicate that increasing…