What exactly happens inside neutron stars - the final stage of a giant star - is subject to speculation. In terms of physics, the interiors of neutron stars, cold atomic gasses and nuclear systems all have one thing in common: they are gaseous systems made up of highly interactive, superfluid fermions. Researchers fed the supercomputer Piz Daint with a new simulation method, and the results are finally offering insight into unknown processes of such systems.
New simulation methods to visualise quantum effects in superfluid fermions
Phys.org - 4 Mar 2019 16:08
What exactly happens inside neutron stars - the final stage of a giant star - is subject to speculation. In terms of physics, the interiors of neutron stars, cold atomic gasses and nuclear systems all have one thing in common: they are gaseous systems made up of highly interactive, superfluid fermions. Researchers fed the supercomputer Piz Daint with a new simulation method, and the results are finally offering insight into unknown processes of such systems.
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