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Wave dark matter ($\psi$DM), which satisfies the Schr\"odinger-Poisson equation, has recently attracted substantial attention as a possible dark matter candidate.
The structure of star clusters. III. Some simple dynamical models
Ivan R. King · 1966
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On semi-degenerate equilibrium configurations of a collisionless self-gravitating Fermi gas
R. Ruffini and L. Stella · 1983
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Evidence against dissipation-less dark matter from observations of galaxy haloes
Ben Moore · 1994
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Observational and theoretical constraints on singular dark matter halos
Ricardo A. Flores and Joel R. Primack · 1994
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Late-time phase transition and the galactic halo as a Bose liquid
Sang-Jin Sin · 1994
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The Structure of Cold Dark Matter Halos
Julio F. Navarro, Carlos S. Frenk, and Simon D. M. White · 1996
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The dark and visible matter content of low surface brightness disc galaxies
W. J. G. de Blok and S. S. McGaugh · 1997
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Resolving the Structure of Cold Dark Matter Halos
B. Moore, F. Governato, T. Quinn, J. Stadel, and G. Lake · 1998
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On the ’coarse-grained’ evolution of collisionless stellar systems
Pierre-Henri Chavanis · 1998
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LAPACK Users’ Guide
E. Anderson, Z. Bai, C. Bischof, S. Blackford, J. Demmel, J. Dongarra, J. Du Croz, A. Greenbaum, S. Hammarling, A. McKenney, and D. Sorensen · 1999
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Repulsive dark matter
Jeremy Goodman · 2000
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Scalar fields as dark matter in spiral galaxies
F. Siddhartha Guzmán and Tonatiuh Matos · 2000
Cited alongside, same era.
Fuzzy Cold Dark Matter: The Wave Properties of Ultralight Particles
Wayne Hu, Rennan Barkana, and Andrei Gruzinov · 2000
Cited alongside, same era.
Axions in string theory
Peter Svrcek and Edward Witten · 2006
Cited alongside, same era.
High-Resolution Simulation on Structure Formation with Extremely Light Bosonic Dark Matter
Tak-Pong Woo and Tzihong Chiueh · 2009
Cited alongside, same era.
The Core-Cusp Problem
W. J. G. de Blok · 2010
Cited alongside, same era.
String axiverse
Asimina Arvanitaki, Savas Dimopoulos, Sergei Dubovsky, Nemanja Kaloper, and John March-Russell · 2010
Cited alongside, same era.
Cosmic structure as the quantum interference of a coherent dark wave
Hsi-Yu Schive, Tzihong Chiueh, and Tom Broadhurst · 2014
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Why is the dark axion mass 10 − 22 10^{-22} ev?
Tzihong Chiueh · 2014
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Understanding the Core-Halo Relation of Quantum Wave Dark Matter from 3d Simulations
Hsi-Yu Schive, Ming-Hsuan Liao, Tak-Pong Woo, Shing-Kwong Wong, Tzihong Chiueh, Tom Broadhurst, and W-Y. Pauchy Hwang · 2014
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Axion cosmology
David JE Marsh · 2016
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Small scale challenges to the λ \lambda cdm paradigm
James S Bullock and Michael Boylan-Kolchin · 2017
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Ultralight scalars as cosmological dark matter
Lam Hui, Jeremiah P Ostriker, Scott Tremaine, and Edward Witten · 2017
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GAMER: A Graphic Processing Unit Accelerated Adaptive-Mesh-Refinement Code for Astrophysics
Hsi-Yu Schive, Yu-Chih Tsai, and Tzihong Chiueh · 2010
Cited alongside, same era.
Too big to fail? The puzzling darkness of massive Milky Way subhaloes
Michael Boylan-Kolchin, James S. Bullock, and Manoj Kaplinghat · 2011
Cited alongside, same era.
Galactic Dynamics: (Second Edition)
James Binney and Scott Tremaine · 2011
Cited alongside, same era.
Mass models of the Milky Way
Paul J. McMillan · 2011
Cited alongside, same era.
The core size of the Fornax dwarf spheroidal
N. C. Amorisco, A. Agnello, and N. W. Evans · 2012
Cited alongside, same era.
Chemodynamical modelling of the galactic bulge and bar
Matthieu Portail, Christopher Wegg, Ortwin Gerhard, and Melissa Ness
Cited in the paper.
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Evolution of linear wave dark matter perturbations in the radiation-dominated era
Ui-Han Zhang and Tzihong Chiueh · 2017
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Cosmological perturbations of extreme axion in the radiation era
Ui-Han Zhang and Tzihong Chiueh · 2017
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How do stars affect ψ \psi dm halos?
James HH Chan, Hsi-Yu Schive, Tak-Pong Woo, and Tzihong Chiueh · 2017
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Gamer-2: a gpu-accelerated adaptive mesh refinement code–accuracy, performance, and scalability
Hsi-Yu Schive, John A ZuHone, Nathan J Goldbaum, Matthew J Turk, Massimo Gaspari, and Chin-Yu Cheng · 2017
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On the schrodinger-poisson–vlasov-poisson correspondence
Philip Mocz, Lachlan Lancaster, Anastasia Fialkov, and Fernando Becerra · 2018
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