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applsciletetrsa>vol-01>issue-01>Boltzmann-Poisson-like approach to simulating the galactic halo response to satellite accretion Dependence on the halo density profile (Dependence on the halo density profile)

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Boltzmann-Poisson-like approach to simulating the galactic halo response to satellite accretion Dependence on the halo density profile (Dependence on the halo density profile)

G. Aguilar-Argüello

O. Valenzuela

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applsciletetrsa>vol-01>issue-01>Boltzmann-Poisson-like approach to simulating the galactic halo response to satellite accretion Dependence on the halo density profile (Dependence on the halo density profile)

Published on -

Boltzmann-Poisson-like approach to simulating the galactic halo response to satellite accretion Dependence on the halo density profile (Dependence on the halo density profile)

Unlock Only

Unlock all

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Magnetic reconnection as an erosion mechanism for magnetic switchbacks

Calculation of the Hubble Constant, the Minimum Mass, and the Proton Charge Radi

Dirac-Majorana neutrino type conversion induced by an oscillating scalar dark ma

A method for automated regression test in scientific computing libraries: illust

Foundation of classical dynamical density functional theory: uniqueness of time-

CMOS + stochastic nanomagnets: heterogeneous computers for probabilistic inferen

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Quantum Dot Source-Drain Transport Response at Microwave Frequencies

Physics-inspired Ising Computing with Ring Oscillator Activated p-bits

Mutual stress flow theorem of electromagnetic field and extension of Newton's th

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STeP-CiM: Strain-enabled Ternary Precision Computation-in-Memory based on Non-Vo

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Boltzmann-Poisson-like approach to simulating the galactic halo response to sate

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