A new cylindrical cosmological simulation method with radially varying resolution enables self-consistent N-body evolution in S¹×ℝ² topology for systems mismatched to cubic periodicity.
A., Trujillo-Gomez, S., & Primack, J
2 Pith papers cite this work. Polarity classification is still indexing.
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In TNG50, high-stellar-mass galaxies show shallow inner DM slopes regardless of central or satellite status, low-mass galaxies exhibit diverse profiles with satellites steeper especially if red and in massive hosts, and inner slopes steepen from z~1 to z=0 more strongly in the hydro run.
citing papers explorer
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Cylindrical cosmological simulations with StePS
A new cylindrical cosmological simulation method with radially varying resolution enables self-consistent N-body evolution in S¹×ℝ² topology for systems mismatched to cubic periodicity.
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The Inner Dark-Matter Structure of Galaxies
In TNG50, high-stellar-mass galaxies show shallow inner DM slopes regardless of central or satellite status, low-mass galaxies exhibit diverse profiles with satellites steeper especially if red and in massive hosts, and inner slopes steepen from z~1 to z=0 more strongly in the hydro run.